This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO
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 09 07.2030 2461290.7030 9.04 11:20:54.05 +65:20:58.3
137.15327 49.20373 galactic UMa Second-epoch detections are separated by 1.3" and 5.3 pix
The object was found in VSX 4" NADA-V21
Type: SRB
# Max. Min./Amp. JD0 Period
10.100 V 11.040 V 2457692.20000 122.000000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:54.05 +65:20:58.3: 9.94 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:54.05 +65:20:58.3: 10.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.05 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.2030* 11 20 54.05 +65 20 58.3 9.0 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
NADA-V21,2461290.7030,9.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NADA-V21 20260907.2030 9.04CV 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 09 07.2030 2461290.7030 9.81 12:39:38.73 +73:52:01.6
124.05590 43.23540 galactic Dra Second-epoch detections are separated by 1.8" and 6.3 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 1691465774520984192 | 12:39:38.62 +73:52:02.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.253+/-0.027 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:39:38.73 +73:52:01.6: 10.86 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:39:38.73 +73:52:01.6: 10.84 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.85 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691465774520984192,2461290.7030,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691465774520984192 20260907.2030 9.81CV 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 09 07.2030 2461290.7030 10.10 11:48:26.51 +67:13:50.1
132.10139 48.76085 galactic Dra Second-epoch detections are separated by 1.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1057924047860558464 | 11:48:26.39 +67:13:50.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.441+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:48:26.51 +67:13:50.1: 11.13 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:48:26.51 +67:13:50.1: 11.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057924047860558464,2461290.7030,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057924047860558464 20260907.2030 10.10CV 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 09 07.2030 2461290.7030 10.15 12:04:02.46 +65:48:34.0
130.55154 50.61182 galactic Dra Second-epoch detections are separated by 0.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1585236321164475136 | 12:04:02.52 +65:48:34.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.402+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:04:02.46 +65:48:34.0: 11.23 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:04:02.46 +65:48:34.0: 11.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1585236321164475136,2461290.7030,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1585236321164475136 20260907.2030 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.09 12:42:14.54 +73:33:18.7
123.82975 43.55702 galactic Dra Second-epoch detections are separated by 2.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691404957784005760 | 12:42:14.46 +73:33:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.135+/-0.026 (A)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:14.54 +73:33:18.7: 11.36 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:42:14.54 +73:33:18.7: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691404957784005760,2461290.7030,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691404957784005760 20260907.2030 10.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.10 12:53:34.00 +72:58:24.0
122.71472 44.15402 galactic Dra Second-epoch detections are separated by 2.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691175224277483648 | 12:53:33.91 +72:58:24.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.299+/-0.030 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:53:34.00 +72:58:24.0: 11.85 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:53:34.00 +72:58:24.0: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691175224277483648,2461290.7030,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691175224277483648 20260907.2030 10.10CV 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 09 07.2030 2461290.7030 10.15 12:51:30.52 +73:37:03.3
122.92504 43.51067 galactic Dra Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691234670920764032 | 12:51:30.06 +73:37:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.497+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:51:30.52 +73:37:03.3: 12.14 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:51:30.52 +73:37:03.3: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 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 1691234670920764032,2461290.7030,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691234670920764032 20260907.2030 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.29 11:30:07.38 +65:38:17.9
135.66136 49.43186 galactic UMa Second-epoch detections are separated by 4.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1056600167140783488 | 11:30:07.68 +65:38:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.394+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:07.38 +65:38:17.9: 11.84 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:07.38 +65:38:17.9: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 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 09 07.2030* 11 30 07.38 +65 38 17.9 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1056600167140783488,2461290.7030,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1056600167140783488 20260907.2030 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.36 11:29:16.50 +65:35:59.4
135.80782 49.42384 galactic UMa Second-epoch detections are separated by 0.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1056594562207828224 | 11:29:16.45 +65:35:59.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.289+/-0.026 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:29:16.50 +65:35:59.4: 11.82 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:29:16.50 +65:35:59.4: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 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 09 07.2030* 11 29 16.50 +65 35 59.4 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1056594562207828224,2461290.7030,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1056594562207828224 20260907.2030 10.36CV 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 09 07.2030 2461290.7030 10.11 12:53:41.82 +72:51:36.4
122.69949 44.26712 galactic Dra Second-epoch detections are separated by 2.4" and 6.5 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 1691172750376323840 | 12:53:41.98 +72:51:35.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.252+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:53:41.82 +72:51:36.4: 11.80 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:53:41.82 +72:51:36.4: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691172750376323840,2461290.7030,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691172750376323840 20260907.2030 10.11CV 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 09 07.2030 2461290.7030 10.23 12:42:14.89 +73:26:26.2
123.83698 43.67149 galactic Dra Second-epoch detections are separated by 0.6" and 6.3 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 1691402655681527424 | 12:42:14.92 +73:26:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.303+/-0.029 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:14.89 +73:26:26.2: 11.74 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:42:14.89 +73:26:26.2: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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
Gaia DR3 1691402655681527424,2461290.7030,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691402655681527424 20260907.2030 10.23CV 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 09 07.2030 2461290.7030 10.14 12:46:55.19 +73:04:48.3
123.38922 44.04416 galactic Dra Second-epoch detections are separated by 2.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689694083330986624 | 12:46:55.17 +73:04:47.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.268+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:55.19 +73:04:48.3: 11.73 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:46:55.19 +73:04:48.3: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689694083330986624,2461290.7030,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689694083330986624 20260907.2030 10.14CV 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 09 07.2030 2461290.7030 10.47 11:23:36.96 +66:22:23.1
135.99343 48.46758 galactic UMa Second-epoch detections are separated by 6.9" and 5.3 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 1057549939028820480 | 11:23:36.87 +66:22:23.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.325+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:23:36.96 +66:22:23.1: 11.72 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:23:36.96 +66:22:23.1: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.2030* 11 23 36.96 +66 22 23.1 10.5 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 1057549939028820480,2461290.7030,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057549939028820480 20260907.2030 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.29 11:26:02.21 +65:42:09.2
136.17774 49.17135 galactic UMa Second-epoch detections are separated by 3.6" and 5.3 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 1057267639418325248 | 11:26:02.32 +65:42:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.237+/-0.026 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:02.21 +65:42:09.2: 11.67 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:26:02.21 +65:42:09.2: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.2030* 11 26 02.21 +65 42 09.2 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057267639418325248,2461290.7030,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057267639418325248 20260907.2030 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.04 12:45:53.67 +73:54:16.3
123.45909 43.21805 galactic Dra Second-epoch detections are separated by 1.8" and 6.3 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 1691433304568134272 | 12:45:53.77 +73:54:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.783+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:45:53.67 +73:54:16.3: 11.67 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:45:53.67 +73:54:16.3: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691433304568134272,2461290.7030,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691433304568134272 20260907.2030 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.27 11:26:58.76 +65:57:03.0
135.86292 49.00271 galactic UMa Second-epoch detections are separated by 3.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1057379514726622208 | 11:26:58.69 +65:57:02.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.283+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:58.76 +65:57:03.0: 11.61 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:26:58.76 +65:57:03.0: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.2030* 11 26 58.76 +65 57 03.0 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057379514726622208,2461290.7030,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057379514726622208 20260907.2030 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.24 12:49:02.60 +72:43:26.6
123.18076 44.40304 galactic Dra Second-epoch detections are separated by 3.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689679308644329600 | 12:49:02.63 +72:43:26.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.638+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:49:02.60 +72:43:26.6: 11.61 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:49:02.60 +72:43:26.6: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689679308644329600,2461290.7030,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689679308644329600 20260907.2030 10.24CV 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 09 07.2030 2461290.7030 10.19 12:36:03.36 +73:40:28.3
124.41892 43.40928 galactic Dra Second-epoch detections are separated by 2.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689969919015339264 | 12:36:03.43 +73:40:28.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.306+/-0.027 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:03.36 +73:40:28.3: 11.58 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:36:03.36 +73:40:28.3: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689969919015339264,2461290.7030,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689969919015339264 20260907.2030 10.19CV 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 09 07.2030 2461290.7030 10.30 11:20:07.33 +66:09:31.7
136.61436 48.47194 galactic UMa Second-epoch detections are separated by 4.7" and 4.7 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 1057518190630630144 | 11:20:07.53 +66:09:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.248+/-0.030 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:07.33 +66:09:31.7: 11.52 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:07.33 +66:09:31.7: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.2030* 11 20 07.33 +66 09 31.7 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057518190630630144,2461290.7030,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057518190630630144 20260907.2030 10.30CV 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 09 07.2030 2461290.7030 10.38 11:20:37.18 +65:39:26.3
136.94524 48.92624 galactic UMa Second-epoch detections are separated by 0.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1057302480193123456 | 11:20:36.90 +65:39:26.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.391+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:37.18 +65:39:26.3: 11.43 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:37.18 +65:39:26.3: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.2030* 11 20 37.18 +65 39 26.3 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057302480193123456,2461290.7030,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057302480193123456 20260907.2030 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 9.98 12:45:47.50 +74:01:11.5
123.46412 43.10256 galactic Dra Second-epoch detections are separated by 1.0" and 6.3 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 1691435778469300352 | 12:45:47.47 +74:01:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.231+/-0.025 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:45:47.50 +74:01:11.5: 11.41 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:45:47.50 +74:01:11.5: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691435778469300352,2461290.7030,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691435778469300352 20260907.2030 9.98CV 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 09 07.2030 2461290.7030 9.78 12:53:30.29 +73:30:54.2
122.72940 43.61238 galactic Dra Second-epoch detections are separated by 1.6" and 6.3 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 1691221408061002752 | 12:53:30.49 +73:30:54.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.576+/-0.027 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:53:30.29 +73:30:54.2: 11.38 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:53:30.29 +73:30:54.2: 11.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691221408061002752,2461290.7030,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691221408061002752 20260907.2030 9.78CV 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 09 07.2030 2461290.7030 10.15 12:10:26.77 +65:50:26.9
129.54143 50.75814 galactic Dra Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1681252617168978688 | 12:10:26.82 +65:50:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.398+/-0.031 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:10:26.77 +65:50:26.9: 11.36 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:10:26.77 +65:50:26.9: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1681252617168978688,2461290.7030,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1681252617168978688 20260907.2030 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.04 12:39:39.22 +67:28:59.7
124.67234 49.60516 galactic Dra Second-epoch detections are separated by 0.8" and 6.3 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 1682213212374454784 | 12:39:39.02 +67:29:00.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.217+/-0.029 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:39:39.22 +67:28:59.7: 11.30 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:39:39.22 +67:28:59.7: 11.34 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.32 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1682213212374454784,2461290.7030,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1682213212374454784 20260907.2030 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.20 11:34:28.25 +65:37:24.0
135.05990 49.65334 galactic UMa Second-epoch detections are separated by 3.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1056559588289705344 | 11:34:28.19 +65:37:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.311+/-0.025 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:34:28.25 +65:37:24.0: 11.26 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:34:28.25 +65:37:24.0: 11.28 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.2030* 11 34 28.25 +65 37 24.0 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1056559588289705344,2461290.7030,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1056559588289705344 20260907.2030 10.20CV 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 09 07.2030 2461290.7030 10.04 12:39:38.32 +67:30:52.1
124.67115 49.57391 galactic Dra Second-epoch detections are separated by 2.0" and 6.4 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 1682213384173148160 | 12:39:38.39 +67:30:51.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.840+/-0.028 (M)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:39:38.32 +67:30:52.1: 11.27 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:39:38.32 +67:30:52.1: 11.28 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1682213384173148160,2461290.7030,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1682213384173148160 20260907.2030 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 9.62 12:53:53.28 +73:27:44.7
122.69090 43.66469 galactic Dra Second-epoch detections are separated by 1.9" and 6.3 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 1691220995744845440 | 12:53:53.33 +73:27:44.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.713+/-0.025 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:53:53.28 +73:27:44.7: 11.22 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:53:53.28 +73:27:44.7: 11.19 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691220995744845440,2461290.7030,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691220995744845440 20260907.2030 9.62CV 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 09 07.2030 2461290.7030 10.11 11:26:27.85 +66:10:06.9
135.77027 48.78722 galactic UMa Second-epoch detections are separated by 1.3" and 5.3 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 1057341749078272384 | 11:26:27.92 +66:10:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.397+/-0.027 (G)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:27.85 +66:10:06.9: 11.22 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:26:27.85 +66:10:06.9: 11.21 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.2030* 11 26 27.85 +66 10 06.9 10.1 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
Gaia DR3 1057341749078272384,2461290.7030,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057341749078272384 20260907.2030 10.11CV 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 09 07.2030 2461290.7030 10.09 12:34:23.76 +73:33:10.5
124.59414 43.52029 galactic Dra Second-epoch detections are separated by 0.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689962432888519936 | 12:34:23.73 +73:33:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.627+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:23.76 +73:33:10.5: 11.22 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:34:23.76 +73:33:10.5: 11.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689962432888519936,2461290.7030,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689962432888519936 20260907.2030 10.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.11 11:34:22.27 +65:55:34.6
134.86301 49.37849 galactic Dra Second-epoch detections are separated by 1.1" and 5.4 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 1056628651363836288 | 11:34:22.16 +65:55:36.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.593+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:34:22.27 +65:55:34.6: 11.22 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:34:22.27 +65:55:34.6: 11.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1056628651363836288,2461290.7030,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1056628651363836288 20260907.2030 10.11CV 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 09 07.2030 2461290.7030 9.91 12:48:42.34 +73:27:29.0
123.20078 43.66877 galactic Dra Second-epoch detections are separated by 1.0" and 6.4 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 1691206839532681344 | 12:48:42.38 +73:27:28.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.026 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:48:42.34 +73:27:29.0: 11.12 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:48:42.34 +73:27:29.0: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691206839532681344,2461290.7030,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691206839532681344 20260907.2030 9.91CV 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 09 07.2030 2461290.7030 10.01 11:20:19.26 +65:31:55.2
137.08532 49.01679 galactic UMa Second-epoch detections are separated by 1.8" and 5.3 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 1057252486773793792 | 11:20:19.44 +65:31:56.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:19.26 +65:31:55.2: 11.11 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:19.26 +65:31:55.2: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 07.2030* 11 20 19.26 +65 31 55.2 10.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057252486773793792,2461290.7030,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057252486773793792 20260907.2030 10.01CV 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 09 07.2030 2461290.7030 10.04 12:37:43.86 +67:42:59.6
124.92611 49.35859 galactic Dra Second-epoch detections are separated by 0.4" and 6.3 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 1682229705048883200 | 12:37:43.94 +67:42:59.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.668+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:37:43.86 +67:42:59.6: 11.09 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:37:43.86 +67:42:59.6: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1682229705048883200,2461290.7030,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1682229705048883200 20260907.2030 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 10.04 11:49:17.77 +67:13:47.7
131.98493 48.79157 galactic Dra Second-epoch detections are separated by 0.7" and 5.5 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 1057173596815246336 | 11:49:17.73 +67:13:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.631+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:49:17.77 +67:13:47.7: 10.95 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:49:17.77 +67:13:47.7: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1057173596815246336,2461290.7030,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1057173596815246336 20260907.2030 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 9.95 11:28:22.07 +66:03:23.3
135.59671 48.97874 galactic Dra Second-epoch detections are separated by 1.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1057381748109602816 | 11:28:22.10 +66:03:23.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.310+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:28:22.07 +66:03:23.3: 10.91 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:28:22.07 +66:03:23.3: 10.92 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1057381748109602816,2461290.7030,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1057381748109602816 20260907.2030 9.95CV 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 09 07.2030 2461290.7030 9.85 12:46:44.06 +72:49:39.6
123.41695 44.29615 galactic Dra Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689684462605506048 | 12:46:43.94 +72:49:40.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.650+/-0.024 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:44.06 +72:49:39.6: 10.88 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:46:44.06 +72:49:39.6: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.88 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689684462605506048,2461290.7030,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689684462605506048 20260907.2030 9.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 9.48 12:53:43.31 +73:41:36.2
122.71115 43.43388 galactic Dra Second-epoch detections are separated by 0.8" and 6.3 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 1691318096365487744 | 12:53:43.43 +73:41:35.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.574+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:53:43.31 +73:41:36.2: 10.87 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:53:43.31 +73:41:36.2: 10.89 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.88 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691318096365487744,2461290.7030,9.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691318096365487744 20260907.2030 9.48CV 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 09 07.2030 2461290.7030 9.58 12:48:15.30 +73:57:58.5
123.23321 43.16014 galactic Dra Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1691525526105947264 | 12:48:15.15 +73:57:58.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.292+/-0.023 (F)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:48:15.30 +73:57:58.5: 10.84 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:48:15.30 +73:57:58.5: 10.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1691525526105947264,2461290.7030,9.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1691525526105947264 20260907.2030 9.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2030 2461290.7030 9.68 12:44:23.08 +73:32:59.5
123.62100 43.56895 galactic Dra Second-epoch detections are separated by 0.9" and 6.4 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 1691398360714235904 | 12:44:23.13 +73:33:00.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.628+/-0.024 (K)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:44:23.08 +73:32:59.5: 10.57 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:44:23.08 +73:32:59.5: 10.57 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691398360714235904,2461290.7030,9.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691398360714235904 20260907.2030 9.68CV 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
***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
First image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Last image: 2461290.70338551 07.09.2026 04:52:42.508 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 126
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.22
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 32078
Objects passed selection criteria: 31926
Measurements per detected object (mean, median, min, max): 2.0 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.0 2.0 2 4
Average stars detected per image: 17654.5
Average stars matched: 16792.5 (95.1174 %)
Memory usage VmPeak: 257664 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 6 23:58:03 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
Last image: 2461290.70266336 07.09.2026 04:51:40.114 UTC
WARNING: VaST exited with code 1 on the field Dra-03-Q2b1x1 as too few input images were matched to the reference image - wrong pointing? clouds? very bad focus?
Blind plate solve of the unmatched second-epoch image fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits to check the telescope pointing
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.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_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits was not set. Trying to guess...
The guess is 605 arcmin.
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/lib/make_outxyls_for_astrometric_calibration found 267 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out3950528.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3950528.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
log-odds ratio 169.963 (6.51755e+73), 67 match, 1 conflict, 125 distractors, 701 index.
RA,Dec = (179.921,69.9368), pixel scale 5.89399 arcsec/pix.
Hit/miss: Hit/miss: -----------------------++++-----+++++-----++++---------------+-+-+----++++----++++------------+++-++
Field 1: solved with index index-4111.fits.
Field 1 solved: writing to file ./out3950528.solved to indicate this.
Field: out3950528.xyls
Field center: (RA,Dec) = (179.935711, 69.952187) deg.
Field center: (RA H:M:S, Dec D:M:S) = (11:59:44.571, +69:57:07.873).
Field size: 15.5907 x 10.3938 degrees
Field rotation angle: up is 178.025 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits' -> 'fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Sep 6 23:57 fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
-rw-r--r-- 1 apache apache 12K Sep 6 23:57 out3950528.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits for reading... done!
Creating new image file (wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits (fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out3950528.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3950528.axy"...
Only searching for solutions within 15.375 degrees of RA,Dec (179.933,69.9514)
Field 1 did not solve (index index-4116.fits, field objects 1-100).
log-odds ratio 21.8214 (2.99846e+09), 7 match, 0 conflict, 19 distractors, 50 index.
RA,Dec = (180.072,70.0078), pixel scale 5.94249 arcsec/pix.
Hit/miss: Hit/miss: -+-+-----+--+--+---+-----+(best)-------+------------------------------------------------------------------
Field 1: solved with index index-4115.fits.
Field 1 solved: writing to file ./out3950528.solved to indicate this.
Field: out3950528.xyls
Field center: (RA,Dec) = (180.043617, 70.006282) deg.
Field center: (RA H:M:S, Dec D:M:S) = (12:00:10.468, +70:00:22.616).
Field size: 15.7173 x 10.5412 degrees
Field rotation angle: up is 177.956 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Sep 6 23:57 fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
-rw-r--r-- 1 apache apache 12K Sep 6 23:57 out3950528.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits for reading... done!
Creating new image file (wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 1564 sources.
Solving...
Reading file "./wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.axy"...
Verifying WCS using indices with quads of size [63.497, 951.859] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
log-odds ratio 119.761 (1.02671e+52), 12 match, 0 conflict, 142 distractors, 13 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: --++-+---+--+-+----++-----------------------------+-------------------------+-------------+---------
--> log-odds 119.761
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 199.718 (5.45171e+86), 20 match, 0 conflict, 159 distractors, 22 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: -+++++--++--+-+----++-----------------------------+---------+-----+---------+-------------+---------
--> log-odds 199.718
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 354.534 (9.38276e+153), 42 match, 0 conflict, 417 distractors, 51 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---+-----------+----++-------+---------+-+---+--------++----------+--+---------
--> log-odds 354.534
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 663.337 (1.21261e+288), 77 match, 0 conflict, 572 distractors, 94 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---++-++-----+-+----+++--+--+++-----+--+-+---+--------++----+---+-+-++-----+---
--> log-odds 663.337
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1142.09 (inf), 140 match, 0 conflict, 751 distractors, 188 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---++-+++----+-+---++++--+-++++-+---++-+-++--+---+---++++-+-+---+-+-++-----+---
--> log-odds 1142.09
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 2109.48 (inf), 259 match, 1 conflict, 913 distractors, 369 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---++++++----+++---++++--+-++++-+---+++++++--++-++-+-++++-+++---+-+++++-+--+++-
--> log-odds 2109.48
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 3369.48 (inf), 428 match, 0 conflict, 851 distractors, 734 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---+++++++---+++---++++-++-++++-+---+++++++--++-++-+-++++-+++++-+-+++++-+--++++
--> log-odds 3369.48
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 5021.55 (inf), 669 match, 0 conflict, 766 distractors, 1445 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---+++++++---+++---++++-++-++++-+---+++++++--++-++-+-++++-+++++-+-+++++-+--++++
--> log-odds 5021.55
Verifying WCS using indices with quads of size [63.497, 951.859] arcmin
Verifying WCS with index 87 of 109 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
log-odds ratio 119.761 (1.02671e+52), 12 match, 0 conflict, 142 distractors, 13 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: --++-+---+--+-+----++-----------------------------+-------------------------+-------------+---------
--> log-odds 119.761
Verifying WCS with index 88 of 109 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 199.718 (5.45171e+86), 20 match, 0 conflict, 159 distractors, 22 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: -+++++--++--+-+----++-----------------------------+---------+-----+---------+-------------+---------
--> log-odds 199.718
Verifying WCS with index 89 of 109 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 354.534 (9.38276e+153), 42 match, 0 conflict, 417 distractors, 51 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---+-----------+----++-------+---------+-+---+--------++----------+--+---------
--> log-odds 354.534
Verifying WCS with index 90 of 109 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 663.337 (1.21261e+288), 77 match, 0 conflict, 572 distractors, 94 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---++-++-----+-+----+++--+--+++-----+--+-+---+--------++----+---+-+-++-----+---
--> log-odds 663.337
Verifying WCS with index 91 of 109 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1142.09 (inf), 140 match, 0 conflict, 751 distractors, 188 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---++-+++----+-+---++++--+-++++-+---++-+-++--+---+---++++-+-+---+-+-++-----+---
--> log-odds 1142.09
Verifying WCS with index 92 of 109 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 2109.48 (inf), 259 match, 1 conflict, 913 distractors, 369 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---++++++----+++---++++--+-++++-+---+++++++--++-++-+-++++-+++---+-+++++-+--+++-
--> log-odds 2109.48
Verifying WCS with index 93 of 109 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 3369.48 (inf), 428 match, 0 conflict, 851 distractors, 734 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---+++++++---+++---++++-++-++++-+---+++++++--++-++-+-++++-+++++-+-+++++-+--++++
--> log-odds 3369.48
Verifying WCS with index 94 of 109 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 5021.55 (inf), 669 match, 0 conflict, 766 distractors, 1445 index.
RA,Dec = (180.046,70.0071), pixel scale 5.96403 arcsec/pix.
Hit/miss: Hit/miss: ++++++--++--+-+-+++++---+++++++---+++---++++-++-++++-+---+++++++--++-++-+-++++-+++++-+-+++++-+--++++
--> log-odds 5021.55
Got 16 solutions.
Field: wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Field center: (RA,Dec) = (180.044283, 70.006240) deg.
Field center: (RA H:M:S, Dec D:M:S) = (12:00:10.628, +70:00:22.464).
Field size: 15.7171 x 10.5412 degrees
Field rotation angle: up is 177.97 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.new"...
renamed 'wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.new' -> 'wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits'
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Generating wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat from image00003.cat
Catalog wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits created.
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Image size: 937.5'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 12:00:10.067 +70:00:19.37 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 280 stars ###
'wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/correct_sextractor_wcs_catalog_usingxy2sky3957354.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
###################################
# Check the image center offset between the reference and the blindly solved unmatched second-epoch image (pointing accuracy)
Reference image center 11:59:37.825 +69:59:43.99
Second-epoch image center 12:00:10.067 +70:00:19.37
Angular distance between the image centers 0.0470 deg.
###################################
The second-epoch image center is consistent with the reference image center (offset 0.0470 deg.) - the star matching failure is probably not a pointing problem
____ VaST output ____
--==VaST 1.0rc90==--
Parsing command line arguments...
opt 'F': Will NOT create flag images for SExtractor
opt '5': 5.000000 pix is the new fixed star matching radius!
opt 'b': Using 500 reference stars for image matching!
opt '3': Will try to select best aperture for each source!
opt 'y': 0 SysRem iterations will be conducted!
opt 't 4': robust linear magnitude calibration (vary zero-point and slope)
opt 'x': 99 is the maximum acceptable SExtractor flag!
WARNING: disabling the mag-size filter in order not to reject blended stars.
opt 'u': Stick with UTC time system, no conversion to TT will be done!
opt 'f': Run ./find_candidates manually!
opt 'k': "JD" keyword in FITS image header will be ignored!
INFO from vast_remove_directory(): Could not open directory: symlinks_to_images
INFO from vast_remove_directory(): Could not open directory: converted_images
INFO from vast_remove_directory(): Could not open directory: unpacked_images
Checking the list of input images specified on the command line ...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits is already a symlink and we do not allow symlinks on symlinks
Looking for the list of input images with time corrections in vast_list_of_input_images_with_time_corrections.txt ... list not found.
This is OK if you specify the input images on the command line, not through this text file.
Checking write permissions for the current directory (/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO)... OK
Found a system-wide installation of SExtractor
Cleaning old outNNNNN.dat files.
Done with cleaning!
VaST was started with the following command line:
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
Preparing to process 4 input FITS images...
######## Forcing special settings for the transient detection ########
transient search mode: disabling the mag-size filter as it should be switched off when running a transient search!
transient search mode: disabling the bad image filter as it will not help during the transient search!
transient search mode: will not try to gues image saturation limit
transient search mode: no UTC-to-TT time system conversion will be performed!!!
transient search mode: setting the maximum acceptable SExtractor flag to 3
transient search mode: disabling rejectin of images with elliptical stars
transient search mode: not discarding large sources
################
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
Setting the fixed star match radius of 5.00 pix
We have 4 images to process.
SExtractor catalog cache: restored Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits catalog from cache
SExtractor catalog cache: restored Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits catalog from cache
Running SExtractor in 3 parallel threads...
Using the catalog image00001.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Using the catalog image00002.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
The gain value (GAIN=0.370) from default.sex will be used for image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
The above guess is based on the non-default gain value specified in default.sex by user
Parent process says: we are done fork()ing.
Waiting for thread 2 to finish...
autodetect_aperture() is running SExtractor on /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
The gain value (GAIN=0.370) from default.sex will be used for image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
The above guess is based on the non-default gain value specified in default.sex by user
autodetect_aperture() is doing a preliminary SExtractor run to determine an appropriate aperture size
sex -c default.sex -PARAMETERS_NAME autodetect_aper.param -CATALOG_NAME autodetect_aper_image00003.cat /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits > image00003.cat.sex_log 2>&1
autodetect_aperture() is running SExtractor on /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
autodetect_aperture() is doing a preliminary SExtractor run to determine an appropriate aperture size
sex -c default.sex -PARAMETERS_NAME autodetect_aper.param -CATALOG_NAME autodetect_aper_image00004.cat /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits > image00004.cat.sex_log 2>&1
autodetect_aperture() is doing the main SExtractor run
sex -PARAMETERS_NAME default.param -PHOT_APERTURES 6.1,6.1,5.5,6.7,7.4,8.0 -VERBOSE_TYPE NORMAL -CATALOG_NAME image00003.cat /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits > image00003.cat.sex_log 2>&1
autodetect_aperture() is doing the main SExtractor run
sex -PARAMETERS_NAME default.param -PHOT_APERTURES 6.3,6.3,5.7,7.0,7.6,8.2 -VERBOSE_TYPE NORMAL -CATALOG_NAME image00004.cat /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits > image00004.cat.sex_log 2>&1
autodetect_aperture() is done with image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
Waiting for thread 1 to finish...
autodetect_aperture() is done with image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Done with SExtractor!
TIMING SExtractor: 4 seconds
Matching stars between images!
No manually selected comparison stars file manually_selected_comparison_stars.lst which is fine.
Processing /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
9576x6388 FITS image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Trying to guess the time system by parsing the comment string 'Time of observation (UTC)'
Time system set from the comment to DATE-OBS keyword: 'Time of observation (UTC)'
The input time system is identified as: UTC (blank if unknown)
Setting observation date using DATE-OBS keyword: 2026-02-11T07:10:16.1285513
Setting observation time using DATE-OBS keyword: 2026-02-11T07:10:16.1285513
Observing time converted to the "standard" FITS header format:
DATE-OBS= 2026-02-11T07:10:16.128
EXPTIME = 20.000
Using the catalog image00001.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Exposure 20 sec, 11.02.2026 07:10:16.128 UTC = JD(UTC) 2461082.79891352 mid. exp.
The reference image star 7584.385 16.233 is rejected, see bad_region.lst
The reference image star 9185.027 24.779 is rejected, see bad_region.lst
The reference image star 8517.393 20.721 is rejected, see bad_region.lst
The reference image star 9103.176 25.412 is rejected, see bad_region.lst
The reference image star 8234.938 30.670 is rejected, see bad_region.lst
The reference image star 8098.668 34.939 is rejected, see bad_region.lst
The reference image star 9529.264 41.173 is rejected, see bad_region.lst
The reference image star 9317.180 35.775 is rejected, see bad_region.lst
The reference image star 7674.408 44.883 is rejected, see bad_region.lst
The reference image star 7512.371 42.754 is rejected, see bad_region.lst
Excluding more reference image stars falling at bad regions!.. (will not print them all)
SExtractor output filtering results:
* passed selection: 5797, (5797 good for image matching)
* rejected as having no flux measurement: 0
* rejected as having SNR<3.0: 0
* rejected inside rectangles defined in bad_region.lst: 1823
* rejected close to frame edge: 25
* rejected as being too small (<1.5 pix): 0
* rejected as being too large (>6.1 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 0
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
Please note: the CCD position-dependent magnitude correction will not be applied.
get_detection_limit_sn(): Detection limit: -7.54
Detection limit from the magnitude-SNR relation= -7.5 (5.0 sigma detection)
The simple faintest star detection limit= -9.6
80 percent brightest stars detection limit= -10.5
Selected detection limit= -10.5
Final detection limit= -10.5 (after subtracting MAG_TRANSIENT_ABOVE_THE_REFERENCE_FRAME_LIMIT=0.0)
Parameter box for transient search: 10.06.4 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 0
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
6120 * detected, using 527/ 500 * for reference/current image matching, fraction_of_ambiguous_matches= 0.006373, number_of_ambiguous_matches=39
refining the coordinate transformation... [CVPOLY iter 1: order=1 pairs=5629 inliers=5629 rms 0.22 -> 0.22 pix, max corner correction 0.1 pix] fraction_of_ambiguous_matches= 0.002614, number_of_ambiguous_matches=16
5628 * matched, [CVPOLY iter 2: order=2 pairs=5628 inliers=5628 rms 0.12 -> 0.12 pix, max corner correction 0.1 pix] fraction_of_ambiguous_matches= 0.001471, number_of_ambiguous_matches=9
5628 * matched (2nd iteration). [CVPOLY iter 3: order=1 pairs=5628 inliers=5628 rms 0.12 -> 0.12 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000654, number_of_ambiguous_matches=4
5628 * matched (3rd iteration). Success!
rotation [degrees] = -0.009
6120 stars detected, 5628 stars matched
Performing magnitude calibration using automatically selected comparison stars
Expecting to find at least 40 * for magnitude calibration
We have N_good_stars = 5189, N_manually_selected_comparison_stars = 0
Using 5189 stars for magnitude calibration (before filtering).
Iteratively removing outliers from the linear mag-mag relation (unweighted fit)...
Iteratively removing outliers from the mag-mag relation (weighted linear/polynomial fit)...
Computing robust linear magnitude calibration.
Used 5181 stars for magnitude calibration (after filtering).
get_detection_limit_sn(): Detection limit: -7.55
6289 objects stored in memory (1000000 max.)
Magnitude calibration is performed successfully!
Saving observations to the cache... OK
memory: 199856 kB used, 232708 kB peak, 65263848 kB available RAM
processed 2 of 4 images ( 50.0%)
Processing /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
9576x6388 FITS image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Trying to guess the time system by parsing the comment string 'Time of observation (UTC)'
Time system set from the comment to DATE-OBS keyword: 'Time of observation (UTC)'
The input time system is identified as: UTC (blank if unknown)
Setting observation date using DATE-OBS keyword: 2026-09-07T04:51:40.1145276
Setting observation time using DATE-OBS keyword: 2026-09-07T04:51:40.1145276
Observing time converted to the "standard" FITS header format:
DATE-OBS= 2026-09-07T04:51:40.114
EXPTIME = 20.000
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
The star 8254.289 93.764 is rejected, see bad_region.lst
The star 9096.680 219.505 is rejected, see bad_region.lst
The star 8486.183 329.706 is rejected, see bad_region.lst
The star 8897.681 2953.083 is rejected, see bad_region.lst
The star 8877.875 3154.428 is rejected, see bad_region.lst
The star 9098.277 3289.998 is rejected, see bad_region.lst
The star 9489.023 3640.421 is rejected, see bad_region.lst
The star 9136.677 3944.510 is rejected, see bad_region.lst
The star 9451.151 3944.097 is rejected, see bad_region.lst
The star 9328.483 4293.025 is rejected, see bad_region.lst
Excluding more stars falling at bad regions!.. (will not print them all)
SExtractor output filtering results:
* passed selection: 170
* rejected as having no flux measurement: 0
* rejected as having SNR<3.0: 0
* rejected inside rectangles defined in bad_region.lst: 108
* rejected close to frame edge: 2
* rejected as being too small (<1.5 pix): 0
* rejected as being too large (>6.1 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 0
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
170 * detected, using 100/ 170 * for reference/current image matching, fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
refining the coordinate transformation... [CVPOLY iter 1: order=2 pairs=86 inliers=86 rms 3.92 -> 0.41 pix, max corner correction 10.6 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
86 * matched, [CVPOLY iter 2: order=1 pairs=86 inliers=86 rms 0.41 -> 0.41 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
86 * matched (2nd iteration). [CVPOLY iter 3: order=1 pairs=86 inliers=86 rms 0.41 -> 0.41 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
86 * matched (3rd iteration). Success!
rotation [degrees] = 172.453
170 stars detected, 86 stars matched
Performing magnitude calibration using automatically selected comparison stars
Expecting to find at least 40 * for magnitude calibration
We have N_good_stars = 27, N_manually_selected_comparison_stars = 0
get_detection_limit_sn(): Detection limit: -7.82
[01;31m ERROR!!! Magnitude calibration failure. Dropping image. [33;00m
6289 objects stored in memory (1000000 max.)
memory: 230456 kB used, 232708 kB peak, 65263848 kB available RAM
processed 3 of 4 images ( 75.0%)
Processing /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
9576x6388 FITS image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
Trying to guess the time system by parsing the comment string 'Time of observation (UTC)'
Time system set from the comment to DATE-OBS keyword: 'Time of observation (UTC)'
The input time system is identified as: UTC (blank if unknown)
Setting observation date using DATE-OBS keyword: 2026-09-07T04:52:42.5083431
Setting observation time using DATE-OBS keyword: 2026-09-07T04:52:42.5083431
Observing time converted to the "standard" FITS header format:
DATE-OBS= 2026-09-07T04:52:42.508
EXPTIME = 20.000
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
The star 8363.173 88.440 is rejected, see bad_region.lst
The star 8254.755 98.646 is rejected, see bad_region.lst
The star 9097.073 224.256 is rejected, see bad_region.lst
The star 7996.054 244.880 is rejected, see bad_region.lst
The star 8486.775 334.523 is rejected, see bad_region.lst
The star 9218.115 598.739 is rejected, see bad_region.lst
The star 8899.107 2957.902 is rejected, see bad_region.lst
The star 8879.235 3159.105 is rejected, see bad_region.lst
The star 9099.687 3294.805 is rejected, see bad_region.lst
The star 9490.502 3645.001 is rejected, see bad_region.lst
Excluding more stars falling at bad regions!.. (will not print them all)
SExtractor output filtering results:
* passed selection: 160
* rejected as having no flux measurement: 0
* rejected as having SNR<3.0: 0
* rejected inside rectangles defined in bad_region.lst: 121
* rejected close to frame edge: 2
* rejected as being too small (<1.6 pix): 0
* rejected as being too large (>6.3 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 0
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
160 * detected, using 100/ 160 * for reference/current image matching, fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
refining the coordinate transformation... [CVPOLY iter 1: order=2 pairs=76 inliers=76 rms 2.59 -> 0.44 pix, max corner correction 8.4 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
76 * matched, [CVPOLY iter 2: order=1 pairs=76 inliers=76 rms 0.44 -> 0.44 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
76 * matched (2nd iteration). [CVPOLY iter 3: order=1 pairs=76 inliers=76 rms 0.44 -> 0.44 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
76 * matched (3rd iteration). Success!
rotation [degrees] = 172.475
160 stars detected, 76 stars matched
Performing magnitude calibration using automatically selected comparison stars
Expecting to find at least 40 * for magnitude calibration
We have N_good_stars = 24, N_manually_selected_comparison_stars = 0
get_detection_limit_sn(): Detection limit: -7.86
[01;31m ERROR!!! Magnitude calibration failure. Dropping image. [33;00m
6289 objects stored in memory (1000000 max.)
memory: 238280 kB used, 238316 kB peak, 65263848 kB available RAM
processed 4 of 4 images (100.0%)
TIMING matching_and_photometry: 0 seconds
Done with measurements! =)
Total number of measurements 11917 (11917 measurements stored in RAM)
Freeing up some memory... Sorting the measurements cached in memory...
Writing lightcurve (outNNNNN.dat) files...
TIMING lightcurve_write: 0 seconds
The lightcurve files have been written, freeing up more memory...
Creating vast_image_details.log ...
Writing summary file: vast_summary.log ... OK
Selecting the best aperture for each source
Aperture with index 0 (REFERENCE_APERTURE_DIAMETER +0.00*REFERENCE_APERTURE_DIAMETER) seems best for 1481 stars
Aperture with index 1 (REFERENCE_APERTURE_DIAMETER +0.00*REFERENCE_APERTURE_DIAMETER) seems best for 0 stars
Aperture with index 2 (REFERENCE_APERTURE_DIAMETER -0.10*REFERENCE_APERTURE_DIAMETER) seems best for 1976 stars
Aperture with index 3 (REFERENCE_APERTURE_DIAMETER +0.10*REFERENCE_APERTURE_DIAMETER) seems best for 648 stars
Aperture with index 4 (REFERENCE_APERTURE_DIAMETER +0.20*REFERENCE_APERTURE_DIAMETER) seems best for 563 stars
Aperture with index 5 (REFERENCE_APERTURE_DIAMETER +0.30*REFERENCE_APERTURE_DIAMETER) seems best for 960 stars
done! =)
TIMING select_aperture: 1 seconds
WARNING: Can't open candidates-transients.lst for reading! -- No candidates found?
Non-zero exit code of lib/transient_list
ERROR running lib/create_list_of_candidate_transients.sh
Computing lightcurve statistics... Will not compute variability indexes for objects having <1 points in lightcurve
You may disable this by commenting out the line '#define DROP_LIGHTCURVES_WITH_SMALL_NUMBER_OF_POINTS_FROM_ALL_PLOTS' in src/vast_limits.h an re-compiling VaST with 'make'
Computing, please wait a bit
.......................................................
vast_lightcurve_statistics.log: 5585 objects, the longest string is 384 bytes.
Allocating memory for resorting the file.
----***** VaST processing WARNING *****----
You asked VaST to process 4 images, but only 1 were actually matched to the reference one.
Please investigate this!
**************************************************************
This error might be a bug, but it is far more likely that it is caused by
inappropriate input data. A few simple things to check in the diagnostic
messages printed above (or the vast*.log files):
* How many of the input images are matched?
* Does the number of detected stars on each image look reasonable?
* Do images have a sufficient overlap of at least about 20 percent?
You may run
./sextract_single_image /path/to/my/image/file.fit
to see how well VaST detects stars with the current SExtractor settings
(star detection settings can be changed in the default.sex configuration
file, see various examples in the VaST directory).
If you cannot identify the problem, please e-mail Kirill Sokolovsky
Please try to describe the problem in details and, if possible, attach vast_summary.log
file and a few example images. If the images are too big to be sent by e-mail, please
upload them through a web-form http://scan.sai.msu.ru/upload/
**************************************************************
Low percentage of matched images - we'll declare this an unsuccessful VaST run (exit code 1)
_____________________
ERROR running VaST on the field Dra-03-Q2b1x1 (less than 4 images processed)
exp_start= 11.02.2026 07:10:16.128 exp= 20.000 JD= 2461082.79891352 ap= 6.1 rotation= 0.000 *detected= 5797 *matched= 5797 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
exp_start= 22.02.2026 06:20:43.009 exp= 20.000 JD= 2461093.76450242 ap= 6.4 rotation= -0.009 *detected= 6120 *matched= 5628 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
exp_start= 07.09.2026 04:51:40.114 exp= 20.000 JD= 2461290.70266336 ap= 6.1 rotation= 172.453 *detected= 170 *matched= 86 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
exp_start= 07.09.2026 04:52:42.508 exp= 20.000 JD= 2461290.70338551 ap= 6.3 rotation= 172.475 *detected= 160 *matched= 76 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.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: 2461290.70266336
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits exists and is non-empty
wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits exists and is non-empty
wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits exists and is non-empty
wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (1st reference image)
verification OK: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:59:37.825 +69:59:43.99 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits (1st new image)
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Image size: 937.5'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 12:00:10.067 +70:00:19.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:37.825 +69:59:43.99
Second-epoch image center 12:00:10.067 +70:00:19.37
Angular distance between the image centers 0.0470 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits (2nd new image)
verification OK: wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
Image size: 937.5'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 12:00:11.406 +70:00:53.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:37.825 +69:59:43.99
Second-epoch image center 12:00:11.406 +70:00:53.43
Angular distance between the image centers 0.0516 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 12:00:10.067 +70:00:19.37
Second-epoch second image center 12:00:11.406 +70:00:53.43
Angular distance between the image centers 0.00965 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits &> /tmp/tmp.a1oGVlke3B
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits &> /tmp/tmp.2wdo7W1KmS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits &> /tmp/tmp.a4d8G2wEqe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits &> /tmp/tmp.JX20QQcRZm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Found non-empty wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
The reference image (wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits) and catalog (wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat) found
'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat' -> 'wcsmag.cat'
Read 42210 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3623 to 206.9070 deg, Dec +62.7295 to +75.5590 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.3623 to 206.9070 deg, Dec 62.7295 to 75.5590 deg
Loaded 8398 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4346 out of 4840 total matches.
Matched with Tycho-2 4840 out of 42210 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.724350
a=0.000000 b=1.000000 c=22.724350
From vast_summary.log: estimated ref. image limiting mag.: -7.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 42210 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3623 to 206.9070 deg, Dec +62.7295 to +75.5590 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.3623 to 206.9070 deg, Dec 62.7295 to 75.5590 deg
Loaded 8398 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4346 out of 4840 total matches.
Matched with Tycho-2 4840 out of 42210 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Forced-photometry filter: calibrated wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -> calib.txt_param_ref_wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (aperture=4.7)
Read 42755 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3622 to 206.9063 deg, Dec +62.7295 to +75.5596 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.3622 to 206.9063 deg, Dec 62.7295 to 75.5596 deg
Loaded 8399 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4309 out of 4838 total matches.
Matched with Tycho-2 4838 out of 42755 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Forced-photometry filter: calibrated wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits -> calib.txt_param_ref_wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
cp: cannot create regular file 'local_wcs_cache/': Not a directory
Found 52 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.1 pix Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
2.4 pix fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
2.4 pix fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
Limiting magnitude estimates:
15.5 mag. Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
15.5 mag. Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
10.4 mag. fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
10.4 mag. fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
All-image limiting magnitude estimate: 10.4 (SNR ) 10.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.a1oGVlke3B (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2006, bad_region=8242, passed=42199
Got 42199 stars (including 32315 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
util/solve_plate_with_UCAC5 got 42199 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 35759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 35759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 35759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4907 stars left (next iteration limit 5397)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits N_match=4907 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.434 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.320 sigma_q4_arcsec=0.324 n_q1=1489 n_q2=837 n_q3=1616 n_q4=965 worst_quadrant_to_overall_ratio=1.233
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -region wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.2wdo7W1KmS (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits' -> 'wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS-calibrated image found: wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Checking if the catalog wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS catalog name: wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2163, bad_region=8480, passed=42737
Got 42737 stars (including 32497 good ones) from the SExtractor catalog wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat
util/solve_plate_with_UCAC5 got 42737 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 4902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 36093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 763 to 829 (Dec 62.7 to 75.6)
Done reading UCAC5 zone files...
Matched 4902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 36093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 36093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4897 stars left (next iteration limit 5386)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits N_match=4897 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.348 sigma_q4_arcsec=0.344 n_q1=1485 n_q2=827 n_q3=1620 n_q4=965 worst_quadrant_to_overall_ratio=1.160
The image catalog is written to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits -region wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.a4d8G2wEqe (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_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.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_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=70, bad_region=468, passed=1869
Got 1869 stars (including 1376 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat
util/solve_plate_with_UCAC5 got 1869 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 1262 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1254 matched stars entering correct_measured_positions(), 1234 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1254 matched stars entering correct_measured_positions(), 1422 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 1263 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1254 matched stars entering correct_measured_positions(), 1420 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Accuracy estimation diagnostic: 1254 matched stars entering correct_measured_positions(), 1418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 1254 stars left (next iteration limit 1379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 1254 catalog matches do not cover the frame (699/22/306/227 per quadrant, need 78 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits N_match=1254 sigma_overall_arcsec=0.960 sigma_q1_arcsec=0.942 sigma_q2_arcsec=1.740 sigma_q3_arcsec=0.962 sigma_q4_arcsec=0.945 n_q1=699 n_q2=22 n_q3=306 n_q4=227 worst_quadrant_to_overall_ratio=1.812
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits -region wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.JX20QQcRZm (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_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.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_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
Checking if the catalog wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
WCS catalog name: wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=72, bad_region=515, passed=1891
Got 1891 stars (including 1356 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits.wcscat
util/solve_plate_with_UCAC5 got 1891 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 1235 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1225 matched stars entering correct_measured_positions(), 1202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1225 matched stars entering correct_measured_positions(), 1395 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 1236 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1225 matched stars entering correct_measured_positions(), 1394 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
Accuracy estimation diagnostic: 1225 matched stars entering correct_measured_positions(), 1394 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Excluding outliers - 1225 stars left (next iteration limit 1347)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 1225 catalog matches do not cover the frame (698/36/246/245 per quadrant, need 76 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits N_match=1225 sigma_overall_arcsec=0.928 sigma_q1_arcsec=0.869 sigma_q2_arcsec=1.461 sigma_q3_arcsec=0.939 sigma_q4_arcsec=1.064 n_q1=698 n_q2=36 n_q3=246 n_q4=245 worst_quadrant_to_overall_ratio=1.574
The image catalog is written to wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits -region wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-51-40_20.00sec_-0.00C_LIGHT_0175.fits'
Saving fully-calibrated image wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Dra-03-Q2b1x1_235338_TTUQ2b1x1_3827167_UoouZbmO/wcs_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176.fits'
Preparing the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:14.54 +73:33:18.7: 11.36 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:04:02.46 +65:48:34.0: 11.23 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:48:26.51 +67:13:50.1: 11.13 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:51:30.52 +73:37:03.3: 12.14 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:30:07.38 +65:38:17.9: 11.84 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:39:38.73 +73:52:01.6: 10.86 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:53:34.00 +72:58:24.0: 11.85 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:54.05 +65:20:58.3: 9.94 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:29:16.50 +65:35:59.4: 11.82 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:53:41.82 +72:51:36.4: 11.80 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:51:30.52 +73:37:03.3: 12.10 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:53:41.82 +72:51:36.4: 11.76 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:48:26.51 +67:13:50.1: 11.18 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:39:38.73 +73:52:01.6: 10.84 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:04:02.46 +65:48:34.0: 11.26 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:54.05 +65:20:58.3: 10.22 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:42:14.54 +73:33:18.7: 11.36 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:30:07.38 +65:38:17.9: 11.89 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:29:16.50 +65:35:59.4: 11.84 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:53:34.00 +72:58:24.0: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry reference-image weighted average: 10.05 +/- 0.00
Forced photometry reference-image weighted average: 10.85 +/- 0.00
Forced photometry reference-image weighted average: 11.25 +/- 0.00
Forced photometry filter KEPT candidate at 11:48:26.51 +67:13:50.1: ref_mag=11.15 +/- 0.00 new_mean_mag=10.0905 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 11.36 +/- 0.00
Forced photometry filter KEPT candidate at 12:53:41.82 +72:51:36.4: ref_mag=11.78 +/- 0.01 new_mean_mag=10.1202 delta=1.66 (need > 0.90)
Forced photometry filter KEPT candidate at 11:20:54.05 +65:20:58.3: ref_mag=10.05 +/- 0.00 new_mean_mag=9.0132 delta=1.03 (need > 0.90)
Forced photometry filter KEPT candidate at 12:39:38.73 +73:52:01.6: ref_mag=10.85 +/- 0.00 new_mean_mag=9.7570 delta=1.09 (need > 0.90)
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter KEPT candidate at 12:04:02.46 +65:48:34.0: ref_mag=11.25 +/- 0.00 new_mean_mag=10.0391 delta=1.21 (need > 0.90)
Forced photometry filter KEPT candidate at 12:42:14.54 +73:33:18.7: ref_mag=11.36 +/- 0.00 new_mean_mag=10.0442 delta=1.32 (need > 0.90)
Forced photometry filter KEPT candidate at 11:30:07.38 +65:38:17.9: ref_mag=11.87 +/- 0.01 new_mean_mag=10.2902 delta=1.57 (need > 0.90)
Forced photometry filter KEPT candidate at 11:29:16.50 +65:35:59.4: ref_mag=11.83 +/- 0.01 new_mean_mag=10.3529 delta=1.47 (need > 0.90)
Forced photometry filter KEPT candidate at 12:53:34.00 +72:58:24.0: ref_mag=11.82 +/- 0.01 new_mean_mag=10.0911 delta=1.73 (need > 0.90)
Forced photometry filter KEPT candidate at 12:51:30.52 +73:37:03.3: ref_mag=12.12 +/- 0.01 new_mean_mag=10.1469 delta=1.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:42:14.89 +73:26:26.2: 11.74 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:42:14.89 +73:26:26.2: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Forced photometry filter KEPT candidate at 12:42:14.89 +73:26:26.2: ref_mag=11.75 +/- 0.01 new_mean_mag=10.2015 delta=1.55 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:55.19 +73:04:48.3: 11.73 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:46:55.19 +73:04:48.3: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.00
Forced photometry filter KEPT candidate at 12:46:55.19 +73:04:48.3: ref_mag=11.72 +/- 0.00 new_mean_mag=10.0618 delta=1.65 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:23:36.96 +66:22:23.1: 11.72 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:23:36.96 +66:22:23.1: 11.73 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:45:53.67 +73:54:16.3: 11.67 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:07.33 +66:09:31.7: 11.52 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:02.21 +65:42:09.2: 11.67 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:49:02.60 +72:43:26.6: 11.61 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:58.76 +65:57:03.0: 11.61 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:36:03.36 +73:40:28.3: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.00
Forced photometry filter KEPT candidate at 11:23:36.96 +66:22:23.1: ref_mag=11.72 +/- 0.00 new_mean_mag=10.4758 delta=1.25 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:49:02.60 +72:43:26.6: 11.62 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:45:53.67 +73:54:16.3: 11.65 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:07.33 +66:09:31.7: 11.53 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:26:02.21 +65:42:09.2: 11.70 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:26:58.76 +65:57:03.0: 11.61 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:36:03.36 +73:40:28.3: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.00
Forced photometry reference-image weighted average: 11.61 +/- 0.00
Forced photometry reference-image weighted average: 11.61 +/- 0.00
Forced photometry reference-image weighted average: 11.52 +/- 0.00
Forced photometry reference-image weighted average: 11.66 +/- 0.00
Forced photometry filter KEPT candidate at 12:36:03.36 +73:40:28.3: ref_mag=11.58 +/- 0.00 new_mean_mag=10.2038 delta=1.37 (need > 0.90)
Forced photometry reference-image weighted average: 11.68 +/- 0.00
Forced photometry filter KEPT candidate at 11:26:58.76 +65:57:03.0: ref_mag=11.61 +/- 0.00 new_mean_mag=10.2732 delta=1.34 (need > 0.90)
Forced photometry filter KEPT candidate at 11:20:07.33 +66:09:31.7: ref_mag=11.52 +/- 0.00 new_mean_mag=10.2730 delta=1.25 (need > 0.90)
Forced photometry filter KEPT candidate at 12:49:02.60 +72:43:26.6: ref_mag=11.61 +/- 0.00 new_mean_mag=10.2329 delta=1.38 (need > 0.90)
Forced photometry filter KEPT candidate at 11:26:02.21 +65:42:09.2: ref_mag=11.68 +/- 0.00 new_mean_mag=10.2633 delta=1.42 (need > 0.90)
Forced photometry filter KEPT candidate at 12:45:53.67 +73:54:16.3: ref_mag=11.66 +/- 0.00 new_mean_mag=10.0050 delta=1.65 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:37.18 +65:39:26.3: 11.43 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:37.18 +65:39:26.3: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.00
Forced photometry filter KEPT candidate at 11:20:37.18 +65:39:26.3: ref_mag=11.45 +/- 0.00 new_mean_mag=10.3717 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:45:47.50 +74:01:11.5: 11.41 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:53:30.29 +73:30:54.2: 11.38 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:45:47.50 +74:01:11.5: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.00
Forced photometry filter KEPT candidate at 12:45:47.50 +74:01:11.5: ref_mag=11.38 +/- 0.00 new_mean_mag=9.9547 delta=1.43 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:53:30.29 +73:30:54.2: 11.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.00
Forced photometry filter KEPT candidate at 12:53:30.29 +73:30:54.2: ref_mag=11.38 +/- 0.00 new_mean_mag=9.7606 delta=1.62 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:10:26.77 +65:50:26.9: 11.36 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:10:26.77 +65:50:26.9: 11.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.00
Forced photometry filter KEPT candidate at 12:10:26.77 +65:50:26.9: ref_mag=11.37 +/- 0.00 new_mean_mag=10.1131 delta=1.26 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:53:53.28 +73:27:44.7: 11.22 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:34:23.76 +73:33:10.5: 11.22 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:39:39.22 +67:28:59.7: 11.30 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:39:38.32 +67:30:52.1: 11.27 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:34:28.25 +65:37:24.0: 11.26 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:26:27.85 +66:10:06.9: 11.22 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:26:27.85 +66:10:06.9: 11.21 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:34:28.25 +65:37:24.0: 11.28 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:34:23.76 +73:33:10.5: 11.22 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:39:38.32 +67:30:52.1: 11.28 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:53:53.28 +73:27:44.7: 11.19 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:39:39.22 +67:28:59.7: 11.34 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Forced photometry reference-image weighted average: 11.27 +/- 0.00
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Forced photometry reference-image weighted average: 11.32 +/- 0.00
Forced photometry reference-image weighted average: 11.21 +/- 0.00
Forced photometry reference-image weighted average: 11.27 +/- 0.00
Forced photometry filter KEPT candidate at 11:26:27.85 +66:10:06.9: ref_mag=11.22 +/- 0.00 new_mean_mag=10.1094 delta=1.11 (need > 0.90)
Forced photometry filter KEPT candidate at 11:34:28.25 +65:37:24.0: ref_mag=11.27 +/- 0.00 new_mean_mag=10.1890 delta=1.08 (need > 0.90)
Forced photometry filter KEPT candidate at 12:34:23.76 +73:33:10.5: ref_mag=11.22 +/- 0.00 new_mean_mag=10.0844 delta=1.13 (need > 0.90)
Forced photometry filter KEPT candidate at 12:39:39.22 +67:28:59.7: ref_mag=11.32 +/- 0.00 new_mean_mag=9.9600 delta=1.36 (need > 0.90)
Forced photometry filter KEPT candidate at 12:39:38.32 +67:30:52.1: ref_mag=11.27 +/- 0.00 new_mean_mag=9.9369 delta=1.34 (need > 0.90)
Forced photometry filter KEPT candidate at 12:53:53.28 +73:27:44.7: ref_mag=11.21 +/- 0.00 new_mean_mag=9.5759 delta=1.63 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:34:22.27 +65:55:34.6: 11.22 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:34:22.27 +65:55:34.6: 11.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.00
Forced photometry filter KEPT candidate at 11:34:22.27 +65:55:34.6: ref_mag=11.23 +/- 0.00 new_mean_mag=10.0515 delta=1.18 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:48:42.34 +73:27:29.0: 11.12 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:48:42.34 +73:27:29.0: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Forced photometry filter KEPT candidate at 12:48:42.34 +73:27:29.0: ref_mag=11.11 +/- 0.00 new_mean_mag=9.8818 delta=1.23 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:20:19.26 +65:31:55.2: 11.11 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:20:19.26 +65:31:55.2: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.00
Forced photometry filter KEPT candidate at 11:20:19.26 +65:31:55.2: ref_mag=11.10 +/- 0.00 new_mean_mag=9.9614 delta=1.13 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:37:43.86 +67:42:59.6: 11.09 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:37:43.86 +67:42:59.6: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Forced photometry filter KEPT candidate at 12:37:43.86 +67:42:59.6: ref_mag=11.11 +/- 0.00 new_mean_mag=9.9445 delta=1.17 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:49:17.77 +67:13:47.7: 10.95 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:49:17.77 +67:13:47.7: 10.96 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:46:44.06 +72:49:39.6: 10.88 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:28:22.07 +66:03:23.3: 10.91 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:44:23.08 +73:32:59.5: 10.57 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:48:15.30 +73:57:58.5: 10.84 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:53:43.31 +73:41:36.2: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.00
Forced photometry filter KEPT candidate at 11:49:17.77 +67:13:47.7: ref_mag=10.96 +/- 0.00 new_mean_mag=10.0320 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:28:22.07 +66:03:23.3: 10.92 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:53:43.31 +73:41:36.2: 10.89 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:46:44.06 +72:49:39.6: 10.87 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:44:23.08 +73:32:59.5: 10.57 +/- 0.00 detection
Forced photometry on wcs_Dra-03-Q2b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:48:15.30 +73:57:58.5: 10.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.00
Forced photometry filter KEPT candidate at 11:28:22.07 +66:03:23.3: ref_mag=10.91 +/- 0.00 new_mean_mag=9.9431 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 10.88 +/- 0.00
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry reference-image weighted average: 10.88 +/- 0.00
Forced photometry filter KEPT candidate at 12:46:44.06 +72:49:39.6: ref_mag=10.88 +/- 0.00 new_mean_mag=9.8608 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 12:44:23.08 +73:32:59.5: ref_mag=10.57 +/- 0.00 new_mean_mag=9.6201 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 12:48:15.30 +73:57:58.5: ref_mag=10.83 +/- 0.00 new_mean_mag=9.5531 delta=1.28 (need > 0.90)
Forced photometry filter KEPT candidate at 12:53:43.31 +73:41:36.2: ref_mag=10.88 +/- 0.00 new_mean_mag=9.4227 delta=1.46 (need > 0.90)
Adding exclusion_list_local.txt__out03529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38747.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 68s
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: 32s
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Considering the candidate 52545_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 52545_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 52718_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 52718_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
Rejecting candidate due to large distance (34.7") between the two second-epoch detections
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Considering the candidate 52720_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 52720_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
Rejecting candidate due to large distance (31.7") between the two second-epoch detections
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Considering the candidate 52754_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 52754_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
Rejecting candidate due to large distance (31.4") between the two second-epoch detections
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Considering the candidate 52914_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 52914_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
Rejecting candidate due to large distance (31.8") between the two second-epoch detections
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Considering the candidate 53091_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 53091_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
Rejecting candidate due to large distance (32.1") between the two second-epoch detections
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Considering the candidate 53122_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 53122_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
Rejecting candidate due to large distance (31.0") between the two second-epoch detections
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Considering the candidate 53142_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 53142_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
Rejecting candidate due to large distance (32.0") between the two second-epoch detections
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Considering the candidate 05008_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 05008_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
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Considering the candidate 34695_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 34695_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
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Considering the candidate 09844_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 09844_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
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Considering the candidate 03729_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 03729_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
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Considering the candidate 35712_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 35712_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
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Considering the candidate 05352_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 05352_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
**** FOUND 11:26:57.59 +65:24:07.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37736_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 37736_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35326_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 35326_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05853_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 05853_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05780_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 05780_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38155_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 38155_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36040_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 36040_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29382_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 29382_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09076_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 09076_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06506_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 06506_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34027_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 34027_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07268_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 07268_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38747_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 38747_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08161_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 08161_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
**** FOUND 11:22:39.84 +66:03:25.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35342_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 35342_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08756_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 08756_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06137_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 06137_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
**** FOUND 11:29:02.32 +65:41:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06950_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 06950_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33967_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 33967_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35855_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 35855_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03529_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 03529_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06951_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 06951_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
**** FOUND 11:18:43.20 +65:35:12.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08788_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 08788_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05313_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 05313_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08875_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 08875_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35915_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 35915_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08101_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 08101_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35734_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 35734_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06394_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 06394_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35981_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 35981_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07797_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
The candidate 07797_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176 did not pass the final checks
**** FOUND 11:22:21.38 +65:59:52.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06558_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 06558_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09639_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 09639_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09764_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 09764_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07442_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 07442_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38258_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 38258_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35072_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 35072_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29000_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 29000_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35699_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
Preparing report for the candidate 35699_fd_Dra-03-Q2b1x1_2026-09-06_23-52-42_20.00sec_0.00C_LIGHT_0176
make_report_in_HTML.sh Phase 2 (HTML assembly): 13s
make_report_in_HTML.sh TOTAL: 113s
Prepared the HTML report for the field Dra-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
12:10:26.77 +65:50:26.9
12:04:02.46 +65:48:34.0
11:20:54.05 +65:20:58.3
11:34:28.25 +65:37:24.0
11:29:16.50 +65:35:59.4
11:30:07.38 +65:38:17.9
11:34:22.27 +65:55:34.6
11:26:02.21 +65:42:09.2
11:20:19.26 +65:31:55.2
11:20:37.18 +65:39:26.3
11:26:58.76 +65:57:03.0
11:28:22.07 +66:03:23.3
11:26:27.85 +66:10:06.9
11:20:07.33 +66:09:31.7
12:39:39.22 +67:28:59.7
12:39:38.32 +67:30:52.1
11:23:36.96 +66:22:23.1
12:37:43.86 +67:42:59.6
11:49:17.77 +67:13:47.7
11:48:26.51 +67:13:50.1
12:48:15.30 +73:57:58.5
12:46:55.19 +73:04:48.3
12:45:47.50 +74:01:11.5
12:45:53.67 +73:54:16.3
12:39:38.73 +73:52:01.6
12:53:43.31 +73:41:36.2
12:51:30.52 +73:37:03.3
12:36:03.36 +73:40:28.3
12:44:23.08 +73:32:59.5
12:42:14.54 +73:33:18.7
12:34:23.76 +73:33:10.5
12:53:30.29 +73:30:54.2
12:53:53.28 +73:27:44.7
12:48:42.34 +73:27:29.0
12:42:14.89 +73:26:26.2
12:53:34.00 +72:58:24.0
12:53:41.82 +72:51:36.4
12:46:44.06 +72:49:39.6
12:49:02.60 +72:43:26.6
########### Completed Dra-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
11:20:54.05 +65:20:58.3
12:39:38.73 +73:52:01.6
11:48:26.51 +67:13:50.1
12:04:02.46 +65:48:34.0
12:42:14.54 +73:33:18.7
12:53:34.00 +72:58:24.0
12:51:30.52 +73:37:03.3
11:30:07.38 +65:38:17.9
11:29:16.50 +65:35:59.4
12:53:41.82 +72:51:36.4
12:42:14.89 +73:26:26.2
12:46:55.19 +73:04:48.3
11:23:36.96 +66:22:23.1
11:26:02.21 +65:42:09.2
12:45:53.67 +73:54:16.3
11:26:58.76 +65:57:03.0
12:49:02.60 +72:43:26.6
12:36:03.36 +73:40:28.3
11:20:07.33 +66:09:31.7
11:20:37.18 +65:39:26.3
12:45:47.50 +74:01:11.5
12:53:30.29 +73:30:54.2
12:10:26.77 +65:50:26.9
12:39:39.22 +67:28:59.7
11:34:28.25 +65:37:24.0
12:39:38.32 +67:30:52.1
12:53:53.28 +73:27:44.7
11:26:27.85 +66:10:06.9
12:34:23.76 +73:33:10.5
11:34:22.27 +65:55:34.6
12:48:42.34 +73:27:29.0
11:20:19.26 +65:31:55.2
12:37:43.86 +67:42:59.6
11:49:17.77 +67:13:47.7
11:28:22.07 +66:03:23.3
12:46:44.06 +72:49:39.6
12:53:43.31 +73:41:36.2
12:48:15.30 +73:57:58.5
12:44:23.08 +73:32:59.5
###################################################################################
11:20:54.05 +65:20:58.3 -- not an asteroid (will add it to exclusion list)
12:39:38.73 +73:52:01.6 -- not an asteroid (will add it to exclusion list)
11:48:26.51 +67:13:50.1 -- not an asteroid (will add it to exclusion list)
12:04:02.46 +65:48:34.0 -- not an asteroid (will add it to exclusion list)
12:42:14.54 +73:33:18.7 -- not an asteroid (will add it to exclusion list)
12:53:34.00 +72:58:24.0 -- not an asteroid (will add it to exclusion list)
12:51:30.52 +73:37:03.3 -- not an asteroid (will add it to exclusion list)
11:30:07.38 +65:38:17.9 -- not an asteroid (will add it to exclusion list)
11:29:16.50 +65:35:59.4 -- not an asteroid (will add it to exclusion list)
12:53:41.82 +72:51:36.4 -- not an asteroid (will add it to exclusion list)
12:42:14.89 +73:26:26.2 -- not an asteroid (will add it to exclusion list)
12:46:55.19 +73:04:48.3 -- not an asteroid (will add it to exclusion list)
11:23:36.96 +66:22:23.1 -- not an asteroid (will add it to exclusion list)
11:26:02.21 +65:42:09.2 -- not an asteroid (will add it to exclusion list)
12:45:53.67 +73:54:16.3 -- not an asteroid (will add it to exclusion list)
11:26:58.76 +65:57:03.0 -- not an asteroid (will add it to exclusion list)
12:49:02.60 +72:43:26.6 -- not an asteroid (will add it to exclusion list)
12:36:03.36 +73:40:28.3 -- not an asteroid (will add it to exclusion list)
11:20:07.33 +66:09:31.7 -- not an asteroid (will add it to exclusion list)
11:20:37.18 +65:39:26.3 -- not an asteroid (will add it to exclusion list)
12:45:47.50 +74:01:11.5 -- not an asteroid (will add it to exclusion list)
12:53:30.29 +73:30:54.2 -- not an asteroid (will add it to exclusion list)
12:10:26.77 +65:50:26.9 -- not an asteroid (will add it to exclusion list)
12:39:39.22 +67:28:59.7 -- not an asteroid (will add it to exclusion list)
11:34:28.25 +65:37:24.0 -- not an asteroid (will add it to exclusion list)
12:39:38.32 +67:30:52.1 -- not an asteroid (will add it to exclusion list)
12:53:53.28 +73:27:44.7 -- not an asteroid (will add it to exclusion list)
11:26:27.85 +66:10:06.9 -- not an asteroid (will add it to exclusion list)
12:34:23.76 +73:33:10.5 -- not an asteroid (will add it to exclusion list)
11:34:22.27 +65:55:34.6 -- not an asteroid (will add it to exclusion list)
12:48:42.34 +73:27:29.0 -- not an asteroid (will add it to exclusion list)
11:20:19.26 +65:31:55.2 -- not an asteroid (will add it to exclusion list)
12:37:43.86 +67:42:59.6 -- not an asteroid (will add it to exclusion list)
11:49:17.77 +67:13:47.7 -- not an asteroid (will add it to exclusion list)
11:28:22.07 +66:03:23.3 -- not an asteroid (will add it to exclusion list)
12:46:44.06 +72:49:39.6 -- not an asteroid (will add it to exclusion list)
12:53:43.31 +73:41:36.2 -- not an asteroid (will add it to exclusion list)
12:48:15.30 +73:57:58.5 -- not an asteroid (will add it to exclusion list)
12:44:23.08 +73:32:59.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
11:20:07.33 +66:09:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:20:19.26 +65:31:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:20:37.18 +65:39:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:20:54.05 +65:20:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:23:36.96 +66:22:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:26:02.21 +65:42:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:26:27.85 +66:10:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:26:58.76 +65:57:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:28:22.07 +66:03:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:29:16.50 +65:35:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:30:07.38 +65:38:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:22.27 +65:55:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:34:28.25 +65:37:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:48:26.51 +67:13:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:49:17.77 +67:13:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:04:02.46 +65:48:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:10:26.77 +65:50:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:34:23.76 +73:33:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:03.36 +73:40:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:37:43.86 +67:42:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:38.32 +67:30:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:38.73 +73:52:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:39.22 +67:28:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:14.54 +73:33:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:14.89 +73:26:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:23.08 +73:32:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:47.50 +74:01:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:53.67 +73:54:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:44.06 +72:49:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:55.19 +73:04:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:15.30 +73:57:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:42.34 +73:27:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:02.60 +72:43:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:30.52 +73:37:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:30.29 +73:30:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:34.00 +72:58:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:41.82 +72:51:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:43.31 +73:41:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:53.28 +73:27:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
11:20:07.33 +66:09:31.7 -- not a known variable star
11:20:19.26 +65:31:55.2 -- not a known variable star
11:20:37.18 +65:39:26.3 -- not a known variable star
11:20:54.05 +65:20:58.3 -- a known variable star
11:23:36.96 +66:22:23.1 -- not a known variable star
11:26:02.21 +65:42:09.2 -- not a known variable star
11:26:27.85 +66:10:06.9 -- not a known variable star
11:26:58.76 +65:57:03.0 -- not a known variable star
11:28:22.07 +66:03:23.3 -- not a known variable star
11:29:16.50 +65:35:59.4 -- not a known variable star
11:30:07.38 +65:38:17.9 -- not a known variable star
11:34:22.27 +65:55:34.6 -- not a known variable star
11:34:28.25 +65:37:24.0 -- not a known variable star
11:48:26.51 +67:13:50.1 -- not a known variable star
11:49:17.77 +67:13:47.7 -- not a known variable star
12:04:02.46 +65:48:34.0 -- not a known variable star
12:10:26.77 +65:50:26.9 -- not a known variable star
12:34:23.76 +73:33:10.5 -- not a known variable star
12:36:03.36 +73:40:28.3 -- not a known variable star
12:37:43.86 +67:42:59.6 -- not a known variable star
12:39:38.32 +67:30:52.1 -- not a known variable star
12:39:38.73 +73:52:01.6 -- not a known variable star
12:39:39.22 +67:28:59.7 -- not a known variable star
12:42:14.54 +73:33:18.7 -- not a known variable star
12:42:14.89 +73:26:26.2 -- not a known variable star
12:44:23.08 +73:32:59.5 -- not a known variable star
12:45:47.50 +74:01:11.5 -- not a known variable star
12:45:53.67 +73:54:16.3 -- not a known variable star
12:46:44.06 +72:49:39.6 -- not a known variable star
12:46:55.19 +73:04:48.3 -- not a known variable star
12:48:15.30 +73:57:58.5 -- not a known variable star
12:48:42.34 +73:27:29.0 -- not a known variable star
12:49:02.60 +72:43:26.6 -- not a known variable star
12:51:30.52 +73:37:03.3 -- not a known variable star
12:53:30.29 +73:30:54.2 -- not a known variable star
12:53:34.00 +72:58:24.0 -- not a known variable star
12:53:41.82 +72:51:36.4 -- not a known variable star
12:53:43.31 +73:41:36.2 -- not a known variable star
12:53:53.28 +73:27:44.7 -- not a known variable star
Found 38 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
39 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
11:20:07.33 +66:09:31.7
11:20:19.26 +65:31:55.2
11:20:37.18 +65:39:26.3
11:20:54.05 +65:20:58.3
11:23:36.96 +66:22:23.1
11:26:02.21 +65:42:09.2
11:26:27.85 +66:10:06.9
11:26:58.76 +65:57:03.0
11:28:22.07 +66:03:23.3
11:29:16.50 +65:35:59.4
11:30:07.38 +65:38:17.9
11:34:22.27 +65:55:34.6
11:34:28.25 +65:37:24.0
11:48:26.51 +67:13:50.1
11:49:17.77 +67:13:47.7
12:04:02.46 +65:48:34.0
12:10:26.77 +65:50:26.9
12:34:23.76 +73:33:10.5
12:36:03.36 +73:40:28.3
12:37:43.86 +67:42:59.6
12:39:38.32 +67:30:52.1
12:39:38.73 +73:52:01.6
12:39:39.22 +67:28:59.7
12:42:14.54 +73:33:18.7
12:42:14.89 +73:26:26.2
12:44:23.08 +73:32:59.5
12:45:47.50 +74:01:11.5
12:45:53.67 +73:54:16.3
12:46:44.06 +72:49:39.6
12:46:55.19 +73:04:48.3
12:48:15.30 +73:57:58.5
12:48:42.34 +73:27:29.0
12:49:02.60 +72:43:26.6
12:51:30.52 +73:37:03.3
12:53:30.29 +73:30:54.2
12:53:34.00 +72:58:24.0
12:53:41.82 +72:51:36.4
12:53:43.31 +73:41:36.2
12:53:53.28 +73:27:44.7
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461290.70266336 -observatory V36
11:38:18.61 +03:31:57.7 Mercury (-0.9mag)
13:35:49.77 -14:29:02.3 Venus (-4.7mag)
07:13:44.16 +22:59:14.2 Mars (1.2mag)
09:08:58.36 +16:57:52.4 Jupiter (-1.8mag)
00:51:45.31 +02:38:47.0 Saturn (0.4mag)
04:13:41.22 +21:01:59.2 Uranus (5.7mag)
00:13:45.34 -00:03:10.0 Neptune (7.7mag)
20:25:35.99 -23:39:35.8 Pluto (14.5mag)
07:40:40.78 +23:52:51.8 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 362 Sep 6 23:58 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461290.70266336:
09:09:03.64 +16:57:26.6 Io (6.2mag)
09:08:55.61 +16:58:07.1 Europa (6.3mag)
09:09:08.84 +16:56:59.6 Ganymede (5.7mag)
09:08:33.48 +16:59:55.0 Callisto (6.9mag)
09:06:44.42 +17:14:22.1 Himalia (15.7mag)
09:09:01.52 +16:57:37.9 Thebe (16.6mag)
09:06:21.72 +17:08:21.1 Elara (17.7mag)
09:12:52.14 +16:25:28.5 Pasiphae (17.9mag)
09:10:03.83 +17:15:37.4 Carme (19.0mag)
00:51:41.74 +02:39:10.4 Titan (8.3mag)
00:51:38.65 +02:38:42.0 Rhea (9.6mag)
00:52:00.77 +02:41:18.4 Iapetus (11.0mag)
00:51:59.30 +02:38:13.2 Hyperion (14.3mag)
00:50:32.18 +02:28:31.7 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 6 23:58 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461290.70266336:
22:04:10.09 +00:54:27.1 JWST
17:32:40.02 +36:50:35.1 Chandra
09:55:35.61 -55:27:37.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 6 23:58 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461290.70266336 -observatory V36
03:40:22.15 +19:20:09.1 17.4mag P/1996 R2 (Lagerkvist)
18:02:52.62 -34:12:47.5 14.3mag P/2010 H2 (Vales)
07:19:23.98 -70:17:46.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:40.93 +33:41:52.2 17.7mag C/2017 K2 (PANSTARRS)
04:51:17.31 +45:27:48.4 15.8mag P/2021 N1 (ZTF)
04:51:17.31 +45:27:48.4 15.8mag P/2021 N1 (ZTF)
04:51:17.31 +45:27:48.4 15.8mag P/2021 N1 (ZTF)
04:51:17.31 +45:27:48.4 15.8mag P/2021 N1 (ZTF)
04:51:17.31 +45:27:48.4 15.8mag P/2021 N1 (ZTF)
22:13:33.66 +28:40:55.0 17.4mag C/2022 E2 (ATLAS)
07:10:07.27 +25:58:49.9 16.9mag C/2022 N2 (PANSTARRS)
10:49:24.61 +27:13:46.0 17.1mag C/2022 QE78 (ATLAS)
09:48:36.60 +05:14:00.9 18.0mag C/2022 R6 (PANSTARRS)
15:29:33.53 -15:38:27.7 14.8mag C/2023 R1 (PANSTARRS)
08:38:18.59 +32:53:11.1 15.8mag C/2024 E1 (Wierzchos)
15:06:34.90 +15:19:26.9 17.9mag C/2024 G6 (ATLAS)
18:33:40.07 +43:10:43.4 13.7mag C/2024 J3 (ATLAS)
20:26:17.94 +49:18:24.5 17.4mag C/2024 R4 (PANSTARRS)
05:35:33.48 -13:01:30.7 15.1mag C/2024 T5 (ATLAS)
07:11:35.90 +18:33:44.0 17.8mag C/2025 J1 (Borisov)
11:17:49.71 +18:46:35.3 16.8mag C/2025 V2 (Rankin)
13:19:32.79 +00:07:26.0 16.8mag C/2025 Y1 (ATLAS)
16:41:08.09 +74:03:01.4 16.1mag C/2026 A2 (Bok)
03:05:50.59 +46:08:16.5 17.4mag C/2026 B2 (Sun-Gao)
12:13:11.02 +11:16:30.9 17.5mag A/2026 E1
22:25:56.14 -35:02:05.8 13.4mag 10P/Tempel
01:19:20.75 +37:00:44.8 17.9mag 11P/Tempel-Swift-LINEAR
11:48:06.46 -05:27:40.1 16.3mag 29P/Schwassmann-Wachmann
12:08:22.75 -05:03:53.9 17.6mag 63P/Wild
00:44:43.29 -07:03:48.7 15.4mag 65P/Gunn
06:39:08.98 +19:15:33.2 17.1mag 78P/Gehrels
03:17:16.63 +14:59:49.6 16.7mag 88P/Howell
05:37:54.54 +28:35:41.2 17.5mag 112P/Urata-Niijima
07:31:31.30 +24:50:25.8 17.9mag 114P/Wiseman-Skiff
10:27:40.91 +20:53:15.8 14.8mag 123P/West-Hartley
12:46:23.42 -21:18:21.2 17.4mag 124P/Mrkos
06:17:18.19 +20:38:31.3 15.9mag 128P/Shoemaker-Holt
02:32:35.17 -17:37:23.0 15.2mag 161P/Hartley-IRAS
09:37:45.82 +13:48:00.0 12.1mag 169P/NEAT
03:24:21.88 +08:28:57.8 14.5mag 220P/McNaught
04:47:49.17 +36:17:27.3 15.2mag 260P/McNaught
08:31:37.46 +35:42:39.8 17.3mag 295P/LINEAR
15:25:10.36 -00:14:18.6 17.9mag 391P/Kowalski
09:27:42.24 +16:51:18.5 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.2K Sep 6 23:58 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +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
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
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
-rw-r--r-- 1 apache apache 5.7K Sep 6 23:58 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
-rw-r--r-- 1 apache apache 190K Sep 6 23:58 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
00:34:06.502 +12:42:13.91 AT 2026ypz 2026-08-08.10 20
21:30:05.008 +02:38:33.95 AT 2026ypy 2026-08-06.53 20.21
21:00:04.179 -04:29:11.16 AT 2026ypx 2026-08-10.99 20.06
02:37:12.256 +15:20:39.63 AT 2026ypw 2026-08-12.19 20.13
20:30:21.422 +77:41:45.40 AT 2026ypv 2026-08-02.23 20.4969
13:32:08.201 +00:21:43.54 AT 2026ypu 2026-08-05.16 19.6868
14:07:14.862 +00:31:05.95 AT 2026ypt 2026-08-08.16 20.0684
17:39:38.555 +44:15:43.22 AT 2026yps 2026-07-22.33 20.9161
23:51:42.078 +03:04:27.33 AT 2026ypr 2026-08-12.07 20.05
02:34:15.880 +40:31:56.36 AT 2026ypq 2026-08-11.58 18.82
15:38:07.902 +06:01:37.84 AT 2026ypp 2026-08-11.26 20.34
15:24:17.953 +11:26:31.29 AT 2026ypo 2026-08-11.26 20.8
14:21:16.003 +25:15:33.98 AT 2026ypn 2026-08-11.26 18.72
16:23:56.085 +09:36:23.21 AT 2026ypm 2026-08-11.28 20.97
20:54:11.595 +10:54:51.15 SN 2026ypl 2026-08-09.34 20.4
00:40:25.122 +24:26:45.82 AT 2026ypk 2026-08-07.45 20.4501
17:05:06.872 +77:16:36.60 AT 2026ypj 2026-08-11.31 18.807
20:49:46.878 -06:36:38.40 AT 2026ypi 2026-08-09.29 20.4359
00:12:21.150 -17:28:55.44 AT 2026yph 2026-08-08.42 20.4034
00:48:58.972 +17:28:17.78 AT 2026ypg 2026-08-05.48 20.2336
-rw-r--r-- 1 apache apache 88K Sep 6 23:58 tns_transients_list.txt
