This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.33 11:13:18.23 +74:17:12.3
131.52250 41.16366 galactic Dra Second-epoch detections are separated by 1.8" 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 1079056180309730432 | 11:13:18.18 +74:17:11.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.461+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:13:18.23 +74:17:12.3: 12.26 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:13:18.23 +74:17:12.3: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 1079056180309730432,2461274.9473,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1079056180309730432 20260822.4473 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.40 12:02:08.84 +75:06:19.5
127.13995 41.61763 galactic Dra Second-epoch detections are separated by 0.6" 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 1691097433830032128 | 12:02:08.79 +75:06:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.567+/-0.032 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:02:08.84 +75:06:19.5: 12.34 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:02:08.84 +75:06:19.5: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 1691097433830032128,2461274.9473,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691097433830032128 20260822.4473 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.51 10:27:00.45 +70:34:02.8
138.23086 42.00750 galactic UMa Second-epoch detections are separated by 1.4" 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 1076525379420579072 | 10:27:00.39 +70:34:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.315+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:27:00.45 +70:34:02.8: 12.39 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:27:00.45 +70:34:02.8: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 27 00.45 +70 34 02.8 11.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1076525379420579072,2461274.9473,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1076525379420579072 20260822.4473 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.56 10:34:33.19 +72:15:53.7
136.08946 41.18424 galactic UMa 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 1077285004516430720 | 10:34:33.26 +72:15:54.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.342+/-0.036 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:34:33.19 +72:15:53.7: 12.45 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:34:33.19 +72:15:53.7: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 34 33.19 +72 15 53.7 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1077285004516430720,2461274.9473,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1077285004516430720 20260822.4473 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.54 10:59:59.12 +72:59:36.3
133.49314 41.77224 galactic Dra Second-epoch detections are separated by 1.9" and 6.1 pix
The object was found in VSX 1" ASASSN-V J105959.28+725936.3
Type: ROT
# Max. Min./Amp. JD0 Period
13.050 g Y 0.150 g 2459524.06900 3.698400000000
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:59:59.12 +72:59:36.3: 12.48 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:59:59.12 +72:59:36.3: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 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
ASASSN-V J105959.28+725936.3,2461274.9473,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J105959.28+725936.3 20260822.4473 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.59 10:42:06.71 +72:46:22.3
135.07784 41.16605 galactic UMa Second-epoch detections are separated by 2.0" 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 1077322795933140608 | 10:42:06.61 +72:46:23.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:42:06.71 +72:46:22.3: 12.52 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:42:06.71 +72:46:22.3: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 42 06.71 +72 46 22.3 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1077322795933140608,2461274.9473,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1077322795933140608 20260822.4473 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.59 10:32:20.40 +70:40:47.3
137.69718 42.23453 galactic UMa Second-epoch detections are separated by 1.3" 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 1076538294386697344 | 10:32:20.52 +70:40:47.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.538+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:32:20.40 +70:40:47.3: 12.57 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:32:20.40 +70:40:47.3: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 32 20.40 +70 40 47.3 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1076538294386697344,2461274.9473,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1076538294386697344 20260822.4473 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.62 10:36:42.10 +72:02:37.6
136.12004 41.45895 galactic UMa Second-epoch detections are separated by 1.5" 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 1077219613638939008 | 10:36:42.10 +72:02:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.363+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:42.10 +72:02:37.6: 12.58 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:42.10 +72:02:37.6: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 36 42.10 +72 02 37.6 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1077219613638939008,2461274.9473,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1077219613638939008 20260822.4473 11.62CV 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 08 22.4473 2461274.9473 11.61 10:30:54.79 +70:10:04.2
138.29263 42.52248 galactic UMa Second-epoch detections are separated by 2.2" 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 1073489284218949760 | 10:30:54.76 +70:10:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.338+/-0.023 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:30:54.79 +70:10:04.2: 12.61 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:30:54.79 +70:10:04.2: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 30 54.79 +70 10 04.2 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1073489284218949760,2461274.9473,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1073489284218949760 20260822.4473 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.65 11:23:18.84 +74:21:21.2
130.68414 41.41919 galactic Dra Second-epoch detections are separated by 3.2" and 5.3 pix
The object was found in VSX 1" Gaia DR3 1078886511921636736
Type: ROT
# Max. Min./Amp. JD0 Period
12.390 G 12.420 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:23:18.84 +74:21:21.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:23:18.84 +74:21:21.2: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 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 1078886511921636736,2461274.9473,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1078886511921636736 20260822.4473 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.69 10:37:24.65 +70:40:42.7
137.28003 42.51906 galactic UMa Second-epoch detections are separated by 4.0" 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 | Large-amplitude variable Gaia DR2 1073527728470386816 | 10:37:24.65 +70:40:42.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.299+/-0.027 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:37:24.65 +70:40:42.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:37:24.65 +70:40:42.7: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 37 24.65 +70 40 42.7 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1073527728470386816,2461274.9473,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1073527728470386816 20260822.4473 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.68 10:32:11.85 +71:56:13.6
136.56041 41.30598 galactic UMa Second-epoch detections are separated by 1.4" 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 | target | 10:32:11.85 +71:56:13.6 (user input) | T | P | (position from user input) J-Ks=0.401+/-0.025 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:32:11.85 +71:56:13.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:32:11.85 +71:56:13.6: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 32 11.85 +71 56 13.6 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.68CV 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
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.70 11:18:50.50 +74:05:56.2
131.20145 41.50917 galactic Dra Second-epoch detections are separated by 0.7" 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 | DocumentRef: VOTx388158 | 11:18:50.50 +74:05:56.2 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:50.50 +74:05:56.2: 12.69 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:50.50 +74:05:56.2: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
DocumentRef: VOTx388158,2461274.9473,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx388158 20260822.4473 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.66 11:54:31.97 +74:40:38.4
127.93681 41.89333 galactic Dra Second-epoch detections are separated by 0.5" 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 | target | 11:54:31.97 +74:40:38.4 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:54:31.97 +74:40:38.4: 12.69 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:54:31.97 +74:40:38.4: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.75 10:43:23.73 +72:04:55.8
135.56053 41.76238 galactic UMa Second-epoch detections are separated by 1.1" 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 | target | 10:43:23.73 +72:04:55.8 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:43:23.73 +72:04:55.8: 12.76 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:43:23.73 +72:04:55.8: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 43 23.73 +72 04 55.8 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.81 10:42:54.25 +71:03:22.5
136.48286 42.52813 galactic UMa Second-epoch detections are separated by 1.2" and 6.0 pix
The object was found in VSX 0" Gaia DR3 1073914863938220160
Type: ROT
# Max. Min./Amp. JD0 Period
12.620 G 12.640 G G
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:42:54.25 +71:03:22.5: 12.83 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:42:54.25 +71:03:22.5: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 42 54.25 +71 03 22.5 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1073914863938220160,2461274.9473,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1073914863938220160 20260822.4473 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.98 10:39:59.67 +71:01:29.4
136.75442 42.39887 galactic UMa Second-epoch detections are separated by 0.7" 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 | target | 10:39:59.67 +71:01:29.4 (user input) | T | P | (position from user input) J-Ks=0.423+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:39:59.67 +71:01:29.4: 13.26 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:39:59.67 +71:01:29.4: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 39 59.67 +71 01 29.4 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.96 10:56:08.27 +73:43:28.2
133.24771 41.01301 galactic Dra Second-epoch detections are separated by 2.0" 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 | DocumentRef: VOTx400114 | 10:56:08.27 +73:43:28.2 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.585+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:56:08.27 +73:43:28.2: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:56:08.27 +73:43:28.2: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx400114,2461274.9473,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx400114 20260822.4473 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.93 11:07:02.60 +74:09:48.8
132.09245 41.05506 galactic Dra Second-epoch detections are separated by 2.2" and 6.0 pix
The object was found in VSX 3" Gaia DR3 1079009657224065024
Type: ROT
# Max. Min./Amp. JD0 Period
12.820 G 12.870 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:07:02.60 +74:09:48.8: 13.21 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:07:02.60 +74:09:48.8: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1079009657224065024,2461274.9473,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1079009657224065024 20260822.4473 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.91 10:54:06.74 +73:30:44.3
133.56428 41.10490 galactic Dra Second-epoch detections are separated by 2.5" 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 | target | 10:54:06.74 +73:30:44.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:54:06.74 +73:30:44.3: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:54:06.74 +73:30:44.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.91 10:36:41.43 +70:21:59.0
137.62450 42.71082 galactic UMa 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 | DocumentRef: VOTx462646 | 10:36:41.43 +70:21:59.0 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.341+/-0.032 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:41.43 +70:21:59.0: 13.17 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:41.43 +70:21:59.0: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 36 41.43 +70 21 59.0 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx462646,2461274.9473,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx462646 20260822.4473 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.89 10:33:39.84 +70:46:24.1
137.50308 42.24077 galactic UMa Second-epoch detections are separated by 1.3" 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 | target | 10:33:39.84 +70:46:24.1 (user input) | T | P | (position from user input) J-Ks=0.233+/-0.033 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:33:39.84 +70:46:24.1: 13.16 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:33:39.84 +70:46:24.1: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 33 39.84 +70 46 24.1 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.95 10:36:07.44 +71:55:42.1
136.26654 41.51616 galactic UMa Second-epoch detections are separated by 0.7" 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 | target | 10:36:07.44 +71:55:42.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:07.44 +71:55:42.1: 13.05 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:07.44 +71:55:42.1: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 36 07.44 +71 55 42.1 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.87 10:34:10.40 +70:39:15.6
137.57070 42.35668 galactic UMa Second-epoch detections are separated by 1.9" 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 | target | 10:34:10.40 +70:39:15.6 (user input) | T | P | (position from user input) J-Ks=0.355+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:34:10.40 +70:39:15.6: 13.05 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:34:10.40 +70:39:15.6: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 34 10.40 +70 39 15.6 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.82 11:01:53.90 +73:41:26.1
132.82715 41.26610 galactic Dra Second-epoch detections are separated by 1.8" 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 | target | 11:01:53.90 +73:41:26.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:01:53.90 +73:41:26.1: 12.99 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:01:53.90 +73:41:26.1: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.71 11:45:06.71 +74:47:17.8
128.67804 41.59166 galactic Dra Second-epoch detections are separated by 2.8" 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 | target | 11:45:06.71 +74:47:17.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:45:06.71 +74:47:17.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:45:06.71 +74:47:17.8: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.84 10:35:32.06 +70:44:33.3
137.37780 42.36769 galactic UMa Second-epoch detections are separated by 1.9" 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 | target | 10:35:32.06 +70:44:33.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:35:32.06 +70:44:33.3: 12.97 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:35:32.06 +70:44:33.3: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 35 32.06 +70 44 33.3 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.87 10:33:58.40 +70:54:59.8
137.34668 42.15280 galactic UMa Second-epoch detections are separated by 1.9" 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 | DocumentRef: VOTx867993 | 10:33:58.40 +70:54:59.8 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:33:58.40 +70:54:59.8: 12.96 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:33:58.40 +70:54:59.8: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 33 58.40 +70 54 59.8 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx867993,2461274.9473,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx867993 20260822.4473 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.81 11:09:57.31 +74:03:33.8
131.93629 41.24674 galactic Dra Second-epoch detections are separated by 2.1" 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 | DocumentRef: VOTx874152 | 11:09:57.31 +74:03:33.8 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:09:57.31 +74:03:33.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:09:57.31 +74:03:33.8: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx874152,2461274.9473,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx874152 20260822.4473 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.88 10:37:18.65 +71:52:48.2
136.21655 41.61326 galactic UMa Second-epoch detections are separated by 1.5" 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 | target | 10:37:18.65 +71:52:48.2 (user input) | T | P | (position from user input) J-Ks=0.288+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:37:18.65 +71:52:48.2: 12.95 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:37:18.65 +71:52:48.2: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 37 18.65 +71 52 48.2 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.87 10:30:02.92 +70:27:27.4
138.09067 42.26359 galactic UMa Second-epoch detections are separated by 1.9" and 6.3 pix
The object was found in VSX 1" Gaia DR3 1076510806595781120
Type: ROT
# Max. Min./Amp. JD0 Period
12.680 G 12.720 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:30:02.92 +70:27:27.4: 12.93 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:30:02.92 +70:27:27.4: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 30 02.92 +70 27 27.4 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1076510806595781120,2461274.9473,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1076510806595781120 20260822.4473 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.72 11:05:13.12 +74:06:33.7
132.27094 41.03598 galactic Dra Second-epoch detections are separated by 0.4" 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 | DocumentRef: VOTx859382 | 11:05:13.12 +74:06:33.7 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:05:13.12 +74:06:33.7: 12.95 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:05:13.12 +74:06:33.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx859382,2461274.9473,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx859382 20260822.4473 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.86 11:10:00.32 +73:22:27.1
132.39857 41.83817 galactic Dra Second-epoch detections are separated by 2.2" 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 | target | 11:10:00.32 +73:22:27.1 (user input) | T | P | (position from user input) J-Ks=0.590+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:10:00.32 +73:22:27.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:10:00.32 +73:22:27.1: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.92 10:52:21.02 +72:23:00.6
134.58815 41.94354 galactic UMa Second-epoch detections are separated by 0.5" 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 | target | 10:52:21.02 +72:23:00.6 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:52:21.02 +72:23:00.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:52:21.02 +72:23:00.6: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 52 21.02 +72 23 00.6 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.94 11:02:20.79 +73:13:41.9
133.12787 41.67099 galactic Dra Second-epoch detections are separated by 1.8" 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 | target | 11:02:20.79 +73:13:41.9 (user input) | T | P | (position from user input) J-Ks=0.553+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:02:20.79 +73:13:41.9: 12.92 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:02:20.79 +73:13:41.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.84 10:51:31.75 +72:15:40.3
134.75356 42.00455 galactic UMa Second-epoch detections are separated by 1.5" 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 | target | 10:51:31.75 +72:15:40.3 (user input) | T | P | (position from user input) J-Ks=0.638+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:51:31.75 +72:15:40.3: 12.89 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:51:31.75 +72:15:40.3: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 51 31.75 +72 15 40.3 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.79 10:37:30.27 +70:26:34.2
137.48586 42.69979 galactic UMa Second-epoch detections are separated by 1.3" 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 | target | 10:37:30.27 +70:26:34.2 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:37:30.27 +70:26:34.2: 12.89 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:37:30.27 +70:26:34.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 37 30.27 +70 26 34.2 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.85 10:34:03.16 +70:40:57.7
137.55456 42.32908 galactic UMa Second-epoch detections are separated by 0.5" 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 | target | 10:34:03.16 +70:40:57.7 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:34:03.16 +70:40:57.7: 12.88 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:34:03.16 +70:40:57.7: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 34 03.16 +70 40 57.7 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.70 11:16:27.27 +74:26:14.2
131.17903 41.13452 galactic Dra Second-epoch detections are separated by 0.9" 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 | target | 11:16:27.27 +74:26:14.2 (user input) | T | P | (position from user input) J-Ks=0.535+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:27.27 +74:26:14.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:27.27 +74:26:14.2: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.74 10:41:27.49 +71:34:59.2
136.14468 42.05022 galactic UMa Second-epoch detections are separated by 3.0" 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 | target | 10:41:27.49 +71:34:59.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:41:27.49 +71:34:59.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:41:27.49 +71:34:59.2: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 41 27.49 +71 34 59.2 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.81 10:48:06.07 +72:09:58.2
135.11109 41.92157 galactic UMa Second-epoch detections are separated by 1.1" 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 | target | 10:48:06.07 +72:09:58.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:48:06.07 +72:09:58.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:48:06.07 +72:09:58.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 48 06.07 +72 09 58.2 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.69 11:16:03.56 +74:05:55.2
131.42563 41.41918 galactic Dra Second-epoch detections are separated by 0.7" 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 | target | 11:16:03.56 +74:05:55.2 (user input) | T | P | (position from user input) J-Ks=0.666+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:03.56 +74:05:55.2: 12.82 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:03.56 +74:05:55.2: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.74 10:45:13.29 +71:15:41.7
136.10979 42.48902 galactic UMa 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 1073953003247775104 | 10:45:07.66 +71:15:10.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:45:13.29 +71:15:41.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:45:13.29 +71:15:41.7: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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!
TCP 2026 08 22.4473* 10 45 13.29 +71 15 41.7 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1073953003247775104,2461274.9473,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1073953003247775104 20260822.4473 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.84 10:36:41.59 +70:59:34.0
137.05583 42.24557 galactic UMa Second-epoch detections are separated by 1.7" 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 | DocumentRef: VOTx1407063 | 10:36:41.59 +70:59:34.0 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:41.59 +70:59:34.0: 12.81 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:41.59 +70:59:34.0: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 36 41.59 +70 59 34.0 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx1407063,2461274.9473,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx1407063 20260822.4473 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.76 11:06:15.04 +73:42:08.5
132.47509 41.41964 galactic Dra Second-epoch detections are separated by 2.7" 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 | ATO J166.5629+73.7024 | 11:06:15.04 +73:42:08.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.587+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:06:15.04 +73:42:08.5: 12.78 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:06:15.04 +73:42:08.5: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J166.5629+73.7024,2461274.9473,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J166.5629+73.7024 20260822.4473 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.79 10:44:24.84 +71:44:51.1
135.76228 42.07172 galactic UMa Second-epoch detections are separated by 3.1" 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 | target | 10:44:24.84 +71:44:51.1 (user input) | T | P | (position from user input) J-Ks=0.312+/-0.034 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:44:24.84 +71:44:51.1: 12.77 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:44:24.84 +71:44:51.1: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 44 24.84 +71 44 51.1 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.74 10:59:51.51 +73:23:14.2
133.21016 41.43991 galactic Dra Second-epoch detections are separated by 1.8" 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 | target | 10:59:51.51 +73:23:14.2 (user input) | T | P | (position from user input) J-Ks=0.499+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:59:51.51 +73:23:14.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:59:51.51 +73:23:14.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.75 10:41:32.89 +71:37:57.6
136.09443 42.01686 galactic UMa Second-epoch detections are separated by 0.6" 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 | target | 10:41:32.89 +71:37:57.6 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.027 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:41:32.89 +71:37:57.6: 12.76 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:41:32.89 +71:37:57.6: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 41 32.89 +71 37 57.6 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.70 11:01:36.82 +73:51:31.3
132.72764 41.11428 galactic Dra Second-epoch detections are separated by 1.8" 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 | target | 11:01:36.82 +73:51:31.3 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.029 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:01:36.82 +73:51:31.3: 12.76 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:01:36.82 +73:51:31.3: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.65 10:39:33.57 +70:59:24.8
136.82134 42.40185 galactic UMa Second-epoch detections are separated by 2.4" 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 | target | 10:39:33.57 +70:59:24.8 (user input) | T | P | (position from user input) J-Ks=0.307+/-0.026 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:39:33.57 +70:59:24.8: 12.73 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:39:33.57 +70:59:24.8: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 39 33.57 +70 59 24.8 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.66 11:01:59.65 +73:25:09.6
133.01673 41.49716 galactic Dra Second-epoch detections are separated by 1.0" 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 | target | 11:01:59.65 +73:25:09.6 (user input) | T | P | (position from user input) J-Ks=0.321+/-0.029 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:01:59.65 +73:25:09.6: 12.75 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:01:59.65 +73:25:09.6: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.79 10:26:54.12 +71:00:24.8
137.82364 41.68942 galactic UMa Second-epoch detections are separated by 2.2" 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 | target | 10:26:54.12 +71:00:24.8 (user input) | T | P | (position from user input) J-Ks=0.504+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:26:54.12 +71:00:24.8: 12.71 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:26:54.12 +71:00:24.8: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 26 54.12 +71 00 24.8 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.76 10:44:40.02 +72:01:47.8
135.50265 41.86464 galactic UMa Second-epoch detections are separated by 0.5" 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 | target | 10:44:40.02 +72:01:47.8 (user input) | T | P | (position from user input) J-Ks=0.472+/-0.029 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:44:40.02 +72:01:47.8: 12.72 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:44:40.02 +72:01:47.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 44 40.02 +72 01 47.8 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.70 11:00:44.88 +73:23:18.8
133.13857 41.47404 galactic Dra Second-epoch detections are separated by 3.1" 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 1078903588711826048 | 11:00:44.66 +73:23:19.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.503+/-0.027 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:00:44.88 +73:23:18.8: 12.69 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:00:44.88 +73:23:18.8: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 1078903588711826048,2461274.9473,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1078903588711826048 20260822.4473 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.71 10:49:11.50 +73:10:04.3
134.21220 41.17494 galactic Dra Second-epoch detections are separated by 0.6" 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 1077428662582672640 | 10:49:11.52 +73:10:04.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.822+/-0.028 (M)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:49:11.50 +73:10:04.3: 12.70 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:49:11.50 +73:10:04.3: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 1077428662582672640,2461274.9473,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1077428662582672640 20260822.4473 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.70 11:17:57.01 +74:15:39.7
131.17171 41.33752 galactic Dra 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 | target | 11:17:57.01 +74:15:39.7 (user input) | T | P | (position from user input) J-Ks=0.293+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:57.01 +74:15:39.7: 12.68 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:57.01 +74:15:39.7: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.71 10:41:03.16 +70:49:14.5
136.84630 42.60997 galactic UMa Second-epoch detections are separated by 2.4" 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 | target | 10:41:03.16 +70:49:14.5 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:41:03.16 +70:49:14.5: 12.68 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:41:03.16 +70:49:14.5: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 41 03.16 +70 49 14.5 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.71 11:35:21.99 +74:33:45.8
129.58945 41.56753 galactic Dra Second-epoch detections are separated by 2.7" 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 | target | 11:35:21.99 +74:33:45.8 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.033 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:35:21.99 +74:33:45.8: 12.67 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:35:21.99 +74:33:45.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.63 10:45:00.33 +71:48:07.1
135.66771 42.05855 galactic UMa Second-epoch detections are separated by 2.0" 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 1076986860770818432 | 10:45:00.47 +71:48:07.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.745+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:45:00.33 +71:48:07.1: 12.66 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:45:00.33 +71:48:07.1: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 45 00.33 +71 48 07.1 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1076986860770818432,2461274.9473,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1076986860770818432 20260822.4473 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.72 10:49:57.77 +73:04:30.1
134.22672 41.28279 galactic Dra Second-epoch detections are separated by 1.6" 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 | target | 10:49:57.77 +73:04:30.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:49:57.77 +73:04:30.1: 12.65 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:49:57.77 +73:04:30.1: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.72 11:44:31.90 +74:56:58.0
128.65227 41.42723 galactic Dra Second-epoch detections are separated by 2.9" and 5.2 pix
The object was found in VSX 0" NSVS 880674
Type: EW
# Max. Min./Amp. JD0 Period
12.805 g Y 0.384 g 2458606.95300 0.438441800000
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:44:31.90 +74:56:58.0: 12.65 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:44:31.90 +74:56:58.0: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 880674,2461274.9473,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 880674 20260822.4473 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.68 11:42:27.92 +74:49:23.4
128.87930 41.49894 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 | target | 11:42:27.92 +74:49:23.4 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.032 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:42:27.92 +74:49:23.4: 12.65 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:42:27.92 +74:49:23.4: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.68CV 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
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.64 10:31:19.89 +69:49:23.9
138.58352 42.79491 galactic UMa Second-epoch detections are separated by 1.9" and 6.2 pix
The object was found in VSX 1" Gaia DR3 1073425684343259520
Type: ROT
# Max. Min./Amp. JD0 Period
12.350 G 12.380 G K
The object was not found in astcheck.
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:31:19.89 +69:49:23.9: 12.63 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:31:19.89 +69:49:23.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 31 19.89 +69 49 23.9 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1073425684343259520,2461274.9473,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1073425684343259520 20260822.4473 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.70 10:53:32.36 +71:47:36.6
134.96192 42.47250 galactic UMa Second-epoch detections are separated by 1.3" 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 | DocumentRef: VOTx2486189 | 10:53:32.36 +71:47:36.6 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.283+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:53:32.36 +71:47:36.6: 12.63 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:53:32.36 +71:47:36.6: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 53 32.36 +71 47 36.6 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2486189,2461274.9473,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2486189 20260822.4473 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.68 10:35:33.10 +72:29:38.0
135.81298 41.06274 galactic UMa Second-epoch detections are separated by 2.3" 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 1077291975247397248 | 10:35:33.19 +72:29:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.579+/-0.035 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:35:33.10 +72:29:38.0: 12.63 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:35:33.10 +72:29:38.0: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 35 33.10 +72 29 38.0 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1077291975247397248,2461274.9473,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1077291975247397248 20260822.4473 11.68CV 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
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.69 10:35:58.67 +70:32:47.9
137.51973 42.53733 galactic UMa Second-epoch detections are separated by 1.8" 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 1073525224505213824 | 10:35:58.66 +70:32:48.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.728+/-0.030 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:35:58.67 +70:32:47.9: 12.62 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:35:58.67 +70:32:47.9: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 35 58.67 +70 32 47.9 11.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1073525224505213824,2461274.9473,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1073525224505213824 20260822.4473 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.52 10:35:49.91 +70:42:30.3
137.38433 42.40948 galactic UMa Second-epoch detections are separated by 1.7" 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 | target | 10:35:49.91 +70:42:30.3 (user input) | T | P | (position from user input) J-Ks=0.310+/-0.027 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:35:49.91 +70:42:30.3: 12.62 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:35:49.91 +70:42:30.3: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 35 49.91 +70 42 30.3 11.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.52 11:14:10.03 +74:11:06.8
131.52055 41.28089 galactic Dra Second-epoch detections are separated by 1.6" 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 1079047860957811072 | 11:14:09.76 +74:11:07.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.588+/-0.027 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:14:10.03 +74:11:06.8: 12.59 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:14:10.03 +74:11:06.8: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1079047860957811072,2461274.9473,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1079047860957811072 20260822.4473 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.61 10:42:33.78 +70:43:57.8
136.79526 42.75757 galactic UMa Second-epoch detections are separated by 1.1" 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 | target | 10:42:33.78 +70:43:57.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:42:33.78 +70:43:57.8: 12.57 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:42:33.78 +70:43:57.8: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 42 33.78 +70 43 57.8 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.58 10:28:59.44 +72:13:20.8
136.54217 40.92905 galactic UMa Second-epoch detections are separated by 1.1" 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 1076921130591192704 | 10:28:59.35 +72:13:19.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.647+/-0.032 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:28:59.44 +72:13:20.8: 12.55 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:28:59.44 +72:13:20.8: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 28 59.44 +72 13 20.8 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1076921130591192704,2461274.9473,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1076921130591192704 20260822.4473 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.46 10:36:10.46 +70:36:52.7
137.44129 42.49798 galactic UMa Second-epoch detections are separated by 1.1" 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 1073537452276345856 | 10:36:10.49 +70:36:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.329+/-0.030 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:10.46 +70:36:52.7: 12.52 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:10.46 +70:36:52.7: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 36 10.46 +70 36 52.7 11.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1073537452276345856,2461274.9473,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1073537452276345856 20260822.4473 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.57 11:18:14.07 +74:10:41.0
131.20093 41.41984 galactic Dra Second-epoch detections are separated by 0.7" 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 1078857267488492800 | 11:18:14.01 +74:10:41.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.233+/-0.028 (F)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:14.07 +74:10:41.0: 12.52 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:14.07 +74:10:41.0: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 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 1078857267488492800,2461274.9473,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1078857267488492800 20260822.4473 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.52 10:36:41.64 +70:42:55.2
137.30650 42.45210 galactic UMa Second-epoch detections are separated by 1.5" 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 1073540239710911488 | 10:36:41.68 +70:42:56.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:41.64 +70:42:55.2: 12.51 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:41.64 +70:42:55.2: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 36 41.64 +70 42 55.2 11.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1073540239710911488,2461274.9473,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1073540239710911488 20260822.4473 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.55 10:41:13.28 +70:44:47.5
136.89766 42.67528 galactic UMa 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 1073906269707974016 | 10:41:13.31 +70:44:48.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.382+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:41:13.28 +70:44:47.5: 12.47 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:41:13.28 +70:44:47.5: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 41 13.28 +70 44 47.5 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1073906269707974016,2461274.9473,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1073906269707974016 20260822.4473 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.48 10:30:13.32 +70:21:37.9
138.16789 42.34343 galactic UMa Second-epoch detections are separated by 2.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:30:13.32 +70:21:37.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:30:13.32 +70:21:37.9: 12.45 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:30:13.32 +70:21:37.9: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 30 13.32 +70 21 37.9 11.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.55 10:28:49.29 +70:32:55.4
138.10390 42.12688 galactic UMa 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 | DocumentRef: VOTx2782060 | 10:28:49.22 +70:32:55.7 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE J-Ks=0.398+/-0.028 (G)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:28:49.29 +70:32:55.4: 12.46 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:28:49.29 +70:32:55.4: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 28 49.29 +70 32 55.4 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2782060,2461274.9473,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2782060 20260822.4473 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.46 11:50:18.11 +74:57:24.4
128.17674 41.54298 galactic Dra Second-epoch detections are separated by 2.0" 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 1079327622243140992 | 11:50:18.24 +74:57:23.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.735+/-0.031 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:50:18.11 +74:57:24.4: 12.46 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:50:18.11 +74:57:24.4: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 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 1079327622243140992,2461274.9473,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1079327622243140992 20260822.4473 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.56 11:11:24.29 +74:05:25.7
131.80119 41.26999 galactic Dra Second-epoch detections are separated by 1.1" 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 1079040649708018176 | 11:11:24.10 +74:05:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.034+/-0.035 (A)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:11:24.29 +74:05:25.7: 12.41 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:11:24.29 +74:05:25.7: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 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 1079040649708018176,2461274.9473,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1079040649708018176 20260822.4473 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.52 11:41:45.75 +74:48:46.1
128.94165 41.49234 galactic Dra Second-epoch detections are separated by 1.1" 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 | DocumentRef: VOTx2854218 | 11:41:45.75 +74:48:46.1 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:41:45.75 +74:48:46.1: 12.40 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:41:45.75 +74:48:46.1: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 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
DocumentRef: VOTx2854218,2461274.9473,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2854218 20260822.4473 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.42 10:39:30.16 +71:01:11.2
136.79982 42.37651 galactic UMa Second-epoch detections are separated by 1.1" 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 | target | 10:39:30.16 +71:01:11.2 (user input) | T | P | (position from user input) J-Ks=0.482+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:39:30.16 +71:01:11.2: 12.39 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:39:30.16 +71:01:11.2: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 39 30.16 +71 01 11.2 11.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.45 10:42:33.99 +72:31:21.6
135.25339 41.38132 galactic UMa Second-epoch detections are separated by 1.1" 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 | DocumentRef: VOTx3034090 | 10:42:34.14 +72:31:21.9 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE J-Ks=0.574+/-0.026 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:42:33.99 +72:31:21.6: 12.38 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:42:33.99 +72:31:21.6: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 42 33.99 +72 31 21.6 11.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3034090,2461274.9473,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3034090 20260822.4473 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.39 11:09:18.68 +73:48:38.4
132.15611 41.43807 galactic Dra Second-epoch detections are separated by 2.2" 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 | DocumentRef: VOTx3064255 | 11:09:18.27 +73:48:39.6 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.568+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:09:18.68 +73:48:38.4: 12.37 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:09:18.68 +73:48:38.4: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
DocumentRef: VOTx3064255,2461274.9473,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3064255 20260822.4473 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.37 11:45:40.72 +74:50:57.2
128.60382 41.54685 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 | DocumentRef: VOTx3096118 | 11:45:40.72 +74:50:57.2 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.623+/-0.028 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:45:40.72 +74:50:57.2: 12.36 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:45:40.72 +74:50:57.2: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 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
DocumentRef: VOTx3096118,2461274.9473,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3096118 20260822.4473 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.36 11:04:46.84 +73:53:22.1
132.45940 41.20659 galactic Dra Second-epoch detections are separated by 1.8" 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 | target | 11:04:46.84 +73:53:22.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:04:46.84 +73:53:22.1: 12.31 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:04:46.84 +73:53:22.1: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9473,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4473 11.36CV 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 08 22.4473 2461274.9473 11.38 11:01:45.12 +73:30:27.1
132.97169 41.41387 galactic Dra Second-epoch detections are separated by 2.6" 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 1078907570145462272 | 11:01:44.98 +73:30:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:01:45.12 +73:30:27.1: 12.31 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:01:45.12 +73:30:27.1: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 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 1078907570145462272,2461274.9473,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1078907570145462272 20260822.4473 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4473 2461274.9473 11.30 10:45:07.86 +71:15:10.9
136.12476 42.49106 galactic UMa Second-epoch detections are separated by 1.8" 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 1073953003247775104 | 10:45:07.66 +71:15:10.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.753+/-0.033 (K)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:45:07.86 +71:15:10.9: 12.28 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:45:07.86 +71:15:10.9: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4473* 10 45 07.86 +71 15 10.9 11.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1073953003247775104,2461274.9473,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1073953003247775104 20260822.4473 11.30CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
First image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Last image: 2461274.94756905 22.08.2026 10:44:19.966 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7481
Objects passed selection criteria: 7424
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 4240.75
Average stars matched: 4059.75 (95.7319 %)
Memory usage VmPeak: 233708 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 05:49:58 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
First image: 2461082.79891352 11.02.2026 07:10:16.128 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Last image: 2461274.94756905 22.08.2026 10:44:19.966 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 122
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 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): 39741
Objects passed selection criteria: 39574
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 23362.2
Average stars matched: 22375.5 (95.7763 %)
Memory usage VmPeak: 262388 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 05:50:40 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
SExtractor catalog cache: saved Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.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: 2461274.94694641
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits exists and is non-empty
wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits exists and is non-empty
wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits exists and is non-empty
wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (1st reference image)
verification OK: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Image size: 941.8'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-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits (1st new image)
verification OK: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
Image size: 942.1'x627.6' 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: 12:00:53.800 +69:59:22.09 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 12:00:53.800 +69:59:22.09
Angular distance between the image centers 0.1085 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits (2nd new image)
verification OK: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Image size: 942.1'x627.6' 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: 12:00:51.565 +69:59:53.33 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 12:00:51.565 +69:59:53.33
Angular distance between the image centers 0.1051 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 12:00:53.800 +69:59:22.09
Second-epoch second image center 12:00:51.565 +69:59:53.33
Angular distance between the image centers 0.00924 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits &> /tmp/tmp.DfVF2fiUO8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits &> /tmp/tmp.MFL4fvkpGS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits &> /tmp/tmp.OgdfBoc2jf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits &> /tmp/tmp.4AxGhcWzQG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Found non-empty wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
The reference image (wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits) and catalog (wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat) found
'wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat' -> 'wcsmag.cat'
Read 7645 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.6391 to 206.7194 deg, Dec +62.8277 to +75.5472 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.6391 to 206.7194 deg, Dec 62.8277 to 75.5472 deg
Loaded 8255 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4552 out of 4756 total matches.
Matched with Tycho-2 4756 out of 7645 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.845850
a=0.000000 b=1.000000 c=22.845850
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7645 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.6391 to 206.7194 deg, Dec +62.8277 to +75.5472 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.6391 to 206.7194 deg, Dec 62.8277 to 75.5472 deg
Loaded 8255 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4552 out of 4756 total matches.
Matched with Tycho-2 4756 out of 7645 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Forced-photometry filter: calibrated wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -> calib.txt_param_ref_wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (aperture=6.1)
Read 8065 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.6392 to 206.7189 deg, Dec +62.8276 to +75.5471 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.6392 to 206.7189 deg, Dec 62.8276 to 75.5471 deg
Loaded 8255 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4558 out of 4791 total matches.
Matched with Tycho-2 4791 out of 8065 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Forced-photometry filter: calibrated wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits -> calib.txt_param_ref_wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.2 pix Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
2.7 pix fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
2.7 pix fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Limiting magnitude estimates:
15.3 mag. Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
15.3 mag. Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
11.8 mag. fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
11.8 mag. fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
All-image limiting magnitude estimate: 11.8 (SNR ) 9.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.DfVF2fiUO8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Checking if the catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS catalog name: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=549, bad_region=0, passed=7645
Got 7645 stars (including 7087 good ones) from the SExtractor catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
util/solve_plate_with_UCAC5 got 7645 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 7645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 7645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 7645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4900 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits N_match=4900 sigma_overall_arcsec=0.351 sigma_q1_arcsec=0.454 sigma_q2_arcsec=0.346 sigma_q3_arcsec=0.322 sigma_q4_arcsec=0.320 n_q1=1163 n_q2=1145 n_q3=1247 n_q4=1345 worst_quadrant_to_overall_ratio=1.292
The image catalog is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -region wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MFL4fvkpGS (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits' -> 'wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS-calibrated image found: wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Checking if the catalog wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS catalog name: wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=588, bad_region=0, passed=8065
Got 8065 stars (including 7468 good ones) from the SExtractor catalog wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat
util/solve_plate_with_UCAC5 got 8065 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 4892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 8065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 8065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 8065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4892 stars left (next iteration limit 5381)
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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits N_match=4892 sigma_overall_arcsec=0.374 sigma_q1_arcsec=0.456 sigma_q2_arcsec=0.380 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.345 n_q1=1158 n_q2=1133 n_q3=1251 n_q4=1350 worst_quadrant_to_overall_ratio=1.220
The image catalog is written to wcs_Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits -region wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OgdfBoc2jf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
Checking if the catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
WCS catalog name: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=20, bad_region=0, passed=660
Got 660 stars (including 640 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat
util/solve_plate_with_UCAC5 got 660 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 766 to 828 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 595 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 593 matched stars entering correct_measured_positions(), 521 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 593 matched stars entering correct_measured_positions(), 568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 766 to 828 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 595 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 592 matched stars entering correct_measured_positions(), 568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 592 matched stars entering correct_measured_positions(), 568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 592 stars left (next iteration limit 652)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=592 robust_rms=5.343 arcsec worst_quadrant_rms=77.077 arcsec
SIP_REFIT: SIP order 3 trial: matched=592 robust_rms=0.562 arcsec worst_quadrant_rms=0.794 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=592 robust_rms_before=1.193 arcsec robust_rms_before_corrected=0.496 arcsec robust_rms_after=0.562 arcsec worst_quadrant_rms_before=0.716 worst_quadrant_rms_after=0.794
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.716 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits N_match=592 sigma_overall_arcsec=0.467 sigma_q1_arcsec=0.540 sigma_q2_arcsec=0.652 sigma_q3_arcsec=0.375 sigma_q4_arcsec=0.648 n_q1=184 n_q2=69 n_q3=274 n_q4=65 worst_quadrant_to_overall_ratio=1.397
The image catalog is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits -region wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4AxGhcWzQG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Checking if the catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
WCS catalog name: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=21, bad_region=0, passed=672
Got 672 stars (including 651 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat
util/solve_plate_with_UCAC5 got 672 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 766 to 828 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 609 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 607 matched stars entering correct_measured_positions(), 522 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 607 matched stars entering correct_measured_positions(), 565 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 766 to 828 (Dec 63.3 to 75.2)
Done reading UCAC5 zone files...
Matched 608 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 606 matched stars entering correct_measured_positions(), 568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 606 matched stars entering correct_measured_positions(), 568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 606 stars left (next iteration limit 667)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=606 robust_rms=4.631 arcsec worst_quadrant_rms=82.739 arcsec
SIP_REFIT: SIP order 3 trial: matched=606 robust_rms=0.564 arcsec worst_quadrant_rms=0.792 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=606 robust_rms_before=1.235 arcsec robust_rms_before_corrected=0.490 arcsec robust_rms_after=0.564 arcsec worst_quadrant_rms_before=0.691 worst_quadrant_rms_after=0.792
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.691 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits N_match=606 sigma_overall_arcsec=0.496 sigma_q1_arcsec=0.591 sigma_q2_arcsec=0.721 sigma_q3_arcsec=0.372 sigma_q4_arcsec=0.707 n_q1=194 n_q2=67 n_q3=280 n_q4=65 worst_quadrant_to_overall_ratio=1.452
The image catalog is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits -region wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits to local_wcs_cache/
'wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'local_wcs_cache/wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
Saving the final (post-refit) wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits to local_wcs_cache/
'wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits' -> 'local_wcs_cache/wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits'
Saving the final (post-refit) wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits to local_wcs_cache/
'wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits' -> 'local_wcs_cache/wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits'
Saving the final (post-refit) wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits to local_wcs_cache/
'wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits' -> 'local_wcs_cache/wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits sigma_overall=0.351 worst_q_ratio=1.292
ref2=Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits sigma_overall=0.374 worst_q_ratio=1.220
new1=fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits sigma_overall=0.467 worst_q_ratio=1.397
new2=fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits sigma_overall=0.496 worst_q_ratio=1.452
reference average sigma_overall=0.3625 worst_q_ratio=1.256
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294_astrometric_residuals.png (4900 matched stars from wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266_astrometric_residuals.png (4892 matched stars from wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196_astrometric_residuals.png (592 matched stars from wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197_astrometric_residuals.png (606 matched stars from wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits'
Saving fully-calibrated image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits'
Preparing the HTML report for the field Dra-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Dra-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
SExtractor catalog cache: saved Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.cat to cache
SExtractor catalog cache: saved Dra-03-Q1b1x1_2026-02-22_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Creating symlink local_wcs_cache/wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits exists and is non-empty
wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits exists and is non-empty
wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits exists and is non-empty
wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (1st reference image)
verification OK: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Image size: 941.8'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-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits (1st new image)
verification OK: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
Image size: 942.1'x627.6' 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: 12:00:53.800 +69:59:22.09 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 12:00:53.800 +69:59:22.09
Angular distance between the image centers 0.1085 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits (2nd new image)
verification OK: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Image size: 942.1'x627.6' 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: 12:00:51.565 +69:59:53.33 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 12:00:51.565 +69:59:53.33
Angular distance between the image centers 0.1051 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 12:00:53.800 +69:59:22.09
Second-epoch second image center 12:00:51.565 +69:59:53.33
Angular distance between the image centers 0.00924 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits &> /tmp/tmp.ZB0WOPk8BS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits &> /tmp/tmp.i00miozbbN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits &> /tmp/tmp.GYAFvwzrVn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits &> /tmp/tmp.QOciUiEqCN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Found non-empty wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits and wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
The reference image (wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits) and catalog (wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat) found
'wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat' -> 'wcsmag.cat'
Read 42210 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3623 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 22.746700
a=0.000000 b=1.000000 c=22.746700
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 42210 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.3623 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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Forced-photometry filter: calibrated wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -> calib.txt_param_ref_wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits (aperture=4.9)
Read 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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Forced-photometry filter: calibrated wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits -> calib.txt_param_ref_wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 107 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
2.1 pix Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
2.6 pix fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
2.6 pix fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Limiting magnitude estimates:
15.4 mag. Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
15.5 mag. Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
11.8 mag. fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
12.0 mag. fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
All-image limiting magnitude estimate: 11.8 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ZB0WOPk8BS (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits' -> 'wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits'
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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS-calibrated image found: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
Checking if the catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits
WCS catalog name: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2006, bad_region=4, passed=42192
Got 42192 stars (including 40113 good ones) from the SExtractor catalog wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat
util/solve_plate_with_UCAC5 got 42192 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
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 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 4902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 42192 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 42192 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 42192 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4902 stars left (next iteration limit 5392)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits N_match=4902 sigma_overall_arcsec=0.336 sigma_q1_arcsec=0.447 sigma_q2_arcsec=0.325 sigma_q3_arcsec=0.311 sigma_q4_arcsec=0.302 n_q1=1157 n_q2=1145 n_q3=1253 n_q4=1347 worst_quadrant_to_overall_ratio=1.331
The image catalog is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits -region wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.i00miozbbN (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits' -> 'wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS-calibrated image found: wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
Checking if the catalog wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat corresponding to the image wcs_Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits
WCS catalog name: wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=2163, bad_region=8, passed=42729
Got 42729 stars (including 40489 good ones) from the SExtractor catalog wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat
util/solve_plate_with_UCAC5 got 42729 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 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 4891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 42729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 42729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 42729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4891 stars left (next iteration limit 5380)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits N_match=4891 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.439 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.328 sigma_q4_arcsec=0.314 n_q1=1153 n_q2=1123 n_q3=1254 n_q4=1361 worst_quadrant_to_overall_ratio=1.249
The image catalog is written to wcs_Dra-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits -region wcs_Dra-03-Q1b1x1_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-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GYAFvwzrVn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
Checking if the catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
WCS catalog name: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=55, bad_region=24, passed=4490
Got 4490 stars (including 4400 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat
util/solve_plate_with_UCAC5 got 4490 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 4171 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4158 matched stars entering correct_measured_positions(), 4157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4157 matched stars entering correct_measured_positions(), 4487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
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 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 4173 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4160 matched stars entering correct_measured_positions(), 4488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Accuracy estimation diagnostic: 4160 matched stars entering correct_measured_positions(), 4488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 4160 stars left (next iteration limit 4572)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4160 robust_rms=6.028 arcsec worst_quadrant_rms=29.504 arcsec
SIP_REFIT: SIP order 3 trial: matched=4160 robust_rms=1.075 arcsec worst_quadrant_rms=1.360 arcsec
SIP_REFIT: SIP order 5 trial: matched=4160 robust_rms=1.002 arcsec worst_quadrant_rms=1.235 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4160 robust_rms_before=1.477 arcsec robust_rms_before_corrected=1.018 arcsec robust_rms_after=1.002 arcsec worst_quadrant_rms_before=1.222 worst_quadrant_rms_after=1.235
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.222 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits N_match=4160 sigma_overall_arcsec=0.922 sigma_q1_arcsec=1.043 sigma_q2_arcsec=1.153 sigma_q3_arcsec=0.805 sigma_q4_arcsec=0.909 n_q1=983 n_q2=543 n_q3=1981 n_q4=653 worst_quadrant_to_overall_ratio=1.250
The image catalog is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits -region wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QOciUiEqCN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
WCS_IMAGE_NAME=wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
WCS-calibrated image found: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Checking if the catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat corresponding to the image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
WCS catalog name: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=54, bad_region=27, passed=4684
Got 4684 stars (including 4595 good ones) from the SExtractor catalog wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat
util/solve_plate_with_UCAC5 got 4684 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 4353 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4332 matched stars entering correct_measured_positions(), 4331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4332 matched stars entering correct_measured_positions(), 4681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
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 766 to 828 (Dec 63.3 to 75.3)
Done reading UCAC5 zone files...
Matched 4357 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4334 matched stars entering correct_measured_positions(), 4682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.00"
Accuracy estimation diagnostic: 4334 matched stars entering correct_measured_positions(), 4682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.01"
Excluding outliers - 4334 stars left (next iteration limit 4765)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4334 robust_rms=6.307 arcsec worst_quadrant_rms=26.777 arcsec
SIP_REFIT: SIP order 3 trial: matched=4334 robust_rms=1.117 arcsec worst_quadrant_rms=1.375 arcsec
SIP_REFIT: SIP order 5 trial: matched=4334 robust_rms=1.022 arcsec worst_quadrant_rms=1.184 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4334 robust_rms_before=1.561 arcsec robust_rms_before_corrected=1.021 arcsec robust_rms_after=1.022 arcsec worst_quadrant_rms_before=1.223 worst_quadrant_rms_after=1.184
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.223 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits N_match=4334 sigma_overall_arcsec=0.924 sigma_q1_arcsec=1.035 sigma_q2_arcsec=1.111 sigma_q3_arcsec=0.824 sigma_q4_arcsec=0.961 n_q1=1054 n_q2=585 n_q3=2023 n_q4=672 worst_quadrant_to_overall_ratio=1.203
The image catalog is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits -region wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-43-26_20.00sec_-0.00C_LIGHTs_0196.fits
Saving fully-calibrated image wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Dra-03-Q1b1x1_054500_TTUQ1b1x1_2078664_D4HDRYCO/wcs_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197.fits
Preparing the HTML report for the field Dra-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:59:59.12 +72:59:36.3: 12.48 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:13:18.23 +74:17:12.3: 12.26 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:27:00.45 +70:34:02.8: 12.39 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:34:33.19 +72:15:53.7: 12.45 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 12:02:08.84 +75:06:19.5: 12.34 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:42.10 +72:02:37.6: 12.58 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:42:06.71 +72:46:22.3: 12.52 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:30:54.79 +70:10:04.2: 12.61 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:23:18.84 +74:21:21.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:32:20.40 +70:40:47.3: 12.57 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:34:33.19 +72:15:53.7: 12.51 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:27:00.45 +70:34:02.8: 12.42 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 12:02:08.84 +75:06:19.5: 12.36 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:59:59.12 +72:59:36.3: 12.47 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:13:18.23 +74:17:12.3: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:23:18.84 +74:21:21.2: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter KEPT candidate at 10:34:33.19 +72:15:53.7: ref_mag=12.48 +/- 0.01 new_mean_mag=11.5597 delta=0.92 (need > 0.90)
Forced photometry filter KEPT candidate at 10:27:00.45 +70:34:02.8: ref_mag=12.41 +/- 0.01 new_mean_mag=11.5040 delta=0.90 (need > 0.90)
Forced photometry filter KEPT candidate at 12:02:08.84 +75:06:19.5: ref_mag=12.35 +/- 0.01 new_mean_mag=11.3969 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Forced photometry filter KEPT candidate at 10:59:59.12 +72:59:36.3: ref_mag=12.47 +/- 0.01 new_mean_mag=11.5343 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 11:13:18.23 +74:17:12.3: ref_mag=12.27 +/- 0.01 new_mean_mag=11.3254 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:32:20.40 +70:40:47.3: 12.53 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:30:54.79 +70:10:04.2: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:42.10 +72:02:37.6: 12.61 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:42:06.71 +72:46:22.3: 12.48 +/- 0.01 detection
Forced photometry filter KEPT candidate at 11:23:18.84 +74:21:21.2: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6500 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 10:32:20.40 +70:40:47.3: ref_mag=12.55 +/- 0.01 new_mean_mag=11.5964 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter KEPT candidate at 10:30:54.79 +70:10:04.2: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6089 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 10:36:42.10 +72:02:37.6: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6192 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 10:42:06.71 +72:46:22.3: ref_mag=12.50 +/- 0.01 new_mean_mag=11.5899 delta=0.91 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:37:24.65 +70:40:42.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:32:11.85 +71:56:13.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:37:24.65 +70:40:42.7: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 10:37:24.65 +70:40:42.7: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6606 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:32:11.85 +71:56:13.6: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 10:32:11.85 +71:56:13.6: ref_mag=12.68 +/- 0.01 new_mean_mag=11.6818 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:50.50 +74:05:56.2: 12.69 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:50.50 +74:05:56.2: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 11:18:50.50 +74:05:56.2: ref_mag=12.70 +/- 0.01 new_mean_mag=11.6806 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:54:31.97 +74:40:38.4: 12.69 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:54:31.97 +74:40:38.4: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 11:54:31.97 +74:40:38.4: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6316 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:43:23.73 +72:04:55.8: 12.76 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:43:23.73 +72:04:55.8: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 10:43:23.73 +72:04:55.8: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7472 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:42:54.25 +71:03:22.5: 12.83 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:42:54.25 +71:03:22.5: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 10:42:54.25 +71:03:22.5: ref_mag=12.79 +/- 0.01 new_mean_mag=11.8160 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:39:59.67 +71:01:29.4: 13.26 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:39:59.67 +71:01:29.4: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 10:39:59.67 +71:01:29.4: ref_mag=13.21 +/- 0.02 new_mean_mag=11.9676 delta=1.24 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:56:08.27 +73:43:28.2: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:56:08.27 +73:43:28.2: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 10:56:08.27 +73:43:28.2: ref_mag=13.24 +/- 0.02 new_mean_mag=11.9507 delta=1.29 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:07:02.60 +74:09:48.8: 13.21 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:07:02.60 +74:09:48.8: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 11:07:02.60 +74:09:48.8: ref_mag=13.21 +/- 0.02 new_mean_mag=11.9349 delta=1.28 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:54:06.74 +73:30:44.3: 13.22 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:54:06.74 +73:30:44.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 10:54:06.74 +73:30:44.3: ref_mag=13.19 +/- 0.02 new_mean_mag=11.9090 delta=1.28 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:41.43 +70:21:59.0: 13.17 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:41.43 +70:21:59.0: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 10:36:41.43 +70:21:59.0: ref_mag=13.15 +/- 0.02 new_mean_mag=11.8588 delta=1.29 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:33:39.84 +70:46:24.1: 13.16 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:33:39.84 +70:46:24.1: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 10:33:39.84 +70:46:24.1: ref_mag=13.16 +/- 0.02 new_mean_mag=11.8786 delta=1.28 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:07.44 +71:55:42.1: 13.05 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:07.44 +71:55:42.1: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 10:36:07.44 +71:55:42.1: ref_mag=13.07 +/- 0.02 new_mean_mag=11.9564 delta=1.11 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:34:10.40 +70:39:15.6: 13.05 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:34:10.40 +70:39:15.6: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 10:34:10.40 +70:39:15.6: ref_mag=13.04 +/- 0.02 new_mean_mag=11.8540 delta=1.18 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:01:53.90 +73:41:26.1: 12.99 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:01:53.90 +73:41:26.1: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 11:01:53.90 +73:41:26.1: ref_mag=12.98 +/- 0.02 new_mean_mag=11.8248 delta=1.16 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:45:06.71 +74:47:17.8: 12.98 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:45:06.71 +74:47:17.8: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter KEPT candidate at 11:45:06.71 +74:47:17.8: ref_mag=12.97 +/- 0.02 new_mean_mag=11.6950 delta=1.28 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:35:32.06 +70:44:33.3: 12.97 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:35:32.06 +70:44:33.3: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 10:35:32.06 +70:44:33.3: ref_mag=12.98 +/- 0.02 new_mean_mag=11.8433 delta=1.13 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:33:58.40 +70:54:59.8: 12.96 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:33:58.40 +70:54:59.8: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 10:33:58.40 +70:54:59.8: ref_mag=12.96 +/- 0.02 new_mean_mag=11.8003 delta=1.16 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:09:57.31 +74:03:33.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:09:57.31 +74:03:33.8: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 11:09:57.31 +74:03:33.8: ref_mag=12.94 +/- 0.02 new_mean_mag=11.8087 delta=1.13 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:37:18.65 +71:52:48.2: 12.95 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:37:18.65 +71:52:48.2: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 10:37:18.65 +71:52:48.2: ref_mag=12.96 +/- 0.02 new_mean_mag=11.8889 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:30:02.92 +70:27:27.4: 12.93 +/- 0.03 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:30:02.92 +70:27:27.4: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 10:30:02.92 +70:27:27.4: ref_mag=12.91 +/- 0.02 new_mean_mag=11.8745 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:05:13.12 +74:06:33.7: 12.95 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:05:13.12 +74:06:33.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter KEPT candidate at 11:05:13.12 +74:06:33.7: ref_mag=12.88 +/- 0.02 new_mean_mag=11.7159 delta=1.16 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:10:00.32 +73:22:27.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:10:00.32 +73:22:27.1: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 11:10:00.32 +73:22:27.1: ref_mag=12.94 +/- 0.01 new_mean_mag=11.8422 delta=1.10 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:52:21.02 +72:23:00.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:52:21.02 +72:23:00.6: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 10:52:21.02 +72:23:00.6: ref_mag=12.94 +/- 0.02 new_mean_mag=11.9164 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:02:20.79 +73:13:41.9: 12.92 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:02:20.79 +73:13:41.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter KEPT candidate at 11:02:20.79 +73:13:41.9: ref_mag=12.93 +/- 0.02 new_mean_mag=11.9327 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:51:31.75 +72:15:40.3: 12.89 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:51:31.75 +72:15:40.3: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 10:51:31.75 +72:15:40.3: ref_mag=12.90 +/- 0.01 new_mean_mag=11.7889 delta=1.11 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:37:30.27 +70:26:34.2: 12.89 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:37:30.27 +70:26:34.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 10:37:30.27 +70:26:34.2: ref_mag=12.88 +/- 0.01 new_mean_mag=11.7800 delta=1.10 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:34:03.16 +70:40:57.7: 12.88 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:34:03.16 +70:40:57.7: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 10:34:03.16 +70:40:57.7: ref_mag=12.91 +/- 0.02 new_mean_mag=11.8400 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:27.27 +74:26:14.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:27.27 +74:26:14.2: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 11:16:27.27 +74:26:14.2: ref_mag=12.85 +/- 0.01 new_mean_mag=11.6724 delta=1.18 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:41:27.49 +71:34:59.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:41:27.49 +71:34:59.2: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 10:41:27.49 +71:34:59.2: ref_mag=12.84 +/- 0.01 new_mean_mag=11.7378 delta=1.11 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:48:06.07 +72:09:58.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:16:03.56 +74:05:55.2: 12.82 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:48:06.07 +72:09:58.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 10:48:06.07 +72:09:58.2: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8193 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:16:03.56 +74:05:55.2: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 11:16:03.56 +74:05:55.2: ref_mag=12.84 +/- 0.01 new_mean_mag=11.6901 delta=1.15 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:45:13.29 +71:15:41.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:45:13.29 +71:15:41.7: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 10:45:13.29 +71:15:41.7: ref_mag=12.82 +/- 0.01 new_mean_mag=11.7517 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:41.59 +70:59:34.0: 12.81 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:41.59 +70:59:34.0: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 10:36:41.59 +70:59:34.0: ref_mag=12.81 +/- 0.01 new_mean_mag=11.8494 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:06:15.04 +73:42:08.5: 12.78 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:06:15.04 +73:42:08.5: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 11:06:15.04 +73:42:08.5: ref_mag=12.77 +/- 0.01 new_mean_mag=11.7258 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:44:24.84 +71:44:51.1: 12.77 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:44:24.84 +71:44:51.1: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 10:44:24.84 +71:44:51.1: ref_mag=12.77 +/- 0.01 new_mean_mag=11.7485 delta=1.02 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:59:51.51 +73:23:14.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:59:51.51 +73:23:14.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 10:59:51.51 +73:23:14.2: ref_mag=12.73 +/- 0.01 new_mean_mag=11.7448 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:41:32.89 +71:37:57.6: 12.76 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:41:32.89 +71:37:57.6: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter KEPT candidate at 10:41:32.89 +71:37:57.6: ref_mag=12.74 +/- 0.01 new_mean_mag=11.7501 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:01:36.82 +73:51:31.3: 12.76 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:01:36.82 +73:51:31.3: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 11:01:36.82 +73:51:31.3: ref_mag=12.77 +/- 0.01 new_mean_mag=11.6945 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:39:33.57 +70:59:24.8: 12.73 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:39:33.57 +70:59:24.8: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 10:39:33.57 +70:59:24.8: ref_mag=12.72 +/- 0.01 new_mean_mag=11.6399 delta=1.08 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:01:59.65 +73:25:09.6: 12.75 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:01:59.65 +73:25:09.6: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 11:01:59.65 +73:25:09.6: ref_mag=12.76 +/- 0.01 new_mean_mag=11.6602 delta=1.10 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:26:54.12 +71:00:24.8: 12.71 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:26:54.12 +71:00:24.8: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 10:26:54.12 +71:00:24.8: ref_mag=12.73 +/- 0.01 new_mean_mag=11.7848 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:44:40.02 +72:01:47.8: 12.72 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:44:40.02 +72:01:47.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 10:44:40.02 +72:01:47.8: ref_mag=12.71 +/- 0.01 new_mean_mag=11.7513 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:00:44.88 +73:23:18.8: 12.69 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:00:44.88 +73:23:18.8: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 11:00:44.88 +73:23:18.8: ref_mag=12.66 +/- 0.01 new_mean_mag=11.6770 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:49:11.50 +73:10:04.3: 12.70 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:49:11.50 +73:10:04.3: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 10:49:11.50 +73:10:04.3: ref_mag=12.69 +/- 0.01 new_mean_mag=11.6886 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:17:57.01 +74:15:39.7: 12.68 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:17:57.01 +74:15:39.7: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 11:17:57.01 +74:15:39.7: ref_mag=12.68 +/- 0.01 new_mean_mag=11.6984 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:41:03.16 +70:49:14.5: 12.68 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:41:03.16 +70:49:14.5: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 10:41:03.16 +70:49:14.5: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7163 delta=0.98 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:35:21.99 +74:33:45.8: 12.67 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:35:21.99 +74:33:45.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 11:35:21.99 +74:33:45.8: ref_mag=12.69 +/- 0.01 new_mean_mag=11.6514 delta=1.04 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:45:00.33 +71:48:07.1: 12.66 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:45:00.33 +71:48:07.1: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 10:45:00.33 +71:48:07.1: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6373 delta=0.99 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:49:57.77 +73:04:30.1: 12.65 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:49:57.77 +73:04:30.1: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 10:49:57.77 +73:04:30.1: ref_mag=12.64 +/- 0.01 new_mean_mag=11.7140 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:44:31.90 +74:56:58.0: 12.65 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:44:31.90 +74:56:58.0: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 11:44:31.90 +74:56:58.0: ref_mag=12.65 +/- 0.01 new_mean_mag=11.7186 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:42:27.92 +74:49:23.4: 12.65 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:42:27.92 +74:49:23.4: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 11:42:27.92 +74:49:23.4: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6789 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:31:19.89 +69:49:23.9: 12.63 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:31:19.89 +69:49:23.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 10:31:19.89 +69:49:23.9: ref_mag=12.63 +/- 0.01 new_mean_mag=11.6299 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:53:32.36 +71:47:36.6: 12.63 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:53:32.36 +71:47:36.6: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 10:53:32.36 +71:47:36.6: ref_mag=12.60 +/- 0.01 new_mean_mag=11.6934 delta=0.90 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:35:33.10 +72:29:38.0: 12.63 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:35:33.10 +72:29:38.0: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter KEPT candidate at 10:35:33.10 +72:29:38.0: ref_mag=12.62 +/- 0.01 new_mean_mag=11.6706 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:35:58.67 +70:32:47.9: 12.62 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:35:58.67 +70:32:47.9: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 10:35:58.67 +70:32:47.9: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6739 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:35:49.91 +70:42:30.3: 12.62 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:35:49.91 +70:42:30.3: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 10:35:49.91 +70:42:30.3: ref_mag=12.61 +/- 0.01 new_mean_mag=11.5221 delta=1.09 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:14:10.03 +74:11:06.8: 12.59 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:14:10.03 +74:11:06.8: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 11:14:10.03 +74:11:06.8: ref_mag=12.58 +/- 0.01 new_mean_mag=11.5109 delta=1.07 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:42:33.78 +70:43:57.8: 12.57 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:42:33.78 +70:43:57.8: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 10:42:33.78 +70:43:57.8: ref_mag=12.55 +/- 0.01 new_mean_mag=11.6125 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:28:59.44 +72:13:20.8: 12.55 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:28:59.44 +72:13:20.8: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 10:28:59.44 +72:13:20.8: ref_mag=12.54 +/- 0.01 new_mean_mag=11.5781 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:10.46 +70:36:52.7: 12.52 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:10.46 +70:36:52.7: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter KEPT candidate at 10:36:10.46 +70:36:52.7: ref_mag=12.50 +/- 0.01 new_mean_mag=11.4693 delta=1.03 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:50:32.08 +72:53:34.5: 12.51 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:50:32.08 +72:53:34.5: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter REJECTED candidate at 10:50:32.08 +72:53:34.5: ref_mag=12.47 +/- 0.01 new_mean_mag=11.5778 delta=0.89 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:18:14.07 +74:10:41.0: 12.52 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:18:14.07 +74:10:41.0: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter KEPT candidate at 11:18:14.07 +74:10:41.0: ref_mag=12.51 +/- 0.01 new_mean_mag=11.5415 delta=0.97 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:36:41.64 +70:42:55.2: 12.51 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:36:41.64 +70:42:55.2: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 10:36:41.64 +70:42:55.2: ref_mag=12.52 +/- 0.01 new_mean_mag=11.5199 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:41:13.28 +70:44:47.5: 12.47 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:41:13.28 +70:44:47.5: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter KEPT candidate at 10:41:13.28 +70:44:47.5: ref_mag=12.46 +/- 0.01 new_mean_mag=11.5550 delta=0.91 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:30:13.32 +70:21:37.9: 12.45 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:30:13.32 +70:21:37.9: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter KEPT candidate at 10:30:13.32 +70:21:37.9: ref_mag=12.43 +/- 0.01 new_mean_mag=11.4826 delta=0.95 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:28:49.29 +70:32:55.4: 12.46 +/- 0.02 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:28:49.29 +70:32:55.4: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter KEPT candidate at 10:28:49.29 +70:32:55.4: ref_mag=12.45 +/- 0.01 new_mean_mag=11.5098 delta=0.94 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:50:18.11 +74:57:24.4: 12.46 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:50:18.11 +74:57:24.4: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter KEPT candidate at 11:50:18.11 +74:57:24.4: ref_mag=12.42 +/- 0.01 new_mean_mag=11.4645 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:11:24.29 +74:05:25.7: 12.41 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:11:24.29 +74:05:25.7: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter KEPT candidate at 11:11:24.29 +74:05:25.7: ref_mag=12.43 +/- 0.01 new_mean_mag=11.5157 delta=0.91 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:41:45.75 +74:48:46.1: 12.40 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:41:45.75 +74:48:46.1: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter KEPT candidate at 11:41:45.75 +74:48:46.1: ref_mag=12.40 +/- 0.01 new_mean_mag=11.4799 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:39:30.16 +71:01:11.2: 12.39 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:39:30.16 +71:01:11.2: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter KEPT candidate at 10:39:30.16 +71:01:11.2: ref_mag=12.38 +/- 0.01 new_mean_mag=11.4150 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:42:33.99 +72:31:21.6: 12.38 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:42:33.99 +72:31:21.6: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 10:42:33.99 +72:31:21.6: ref_mag=12.35 +/- 0.01 new_mean_mag=11.4266 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:09:18.68 +73:48:38.4: 12.37 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:09:18.68 +73:48:38.4: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 11:09:18.68 +73:48:38.4: ref_mag=12.36 +/- 0.01 new_mean_mag=11.3979 delta=0.96 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:45:40.72 +74:50:57.2: 12.36 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:45:40.72 +74:50:57.2: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 11:45:40.72 +74:50:57.2: ref_mag=12.34 +/- 0.01 new_mean_mag=11.3368 delta=1.00 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:04:46.84 +73:53:22.1: 12.31 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:04:46.84 +73:53:22.1: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter KEPT candidate at 11:04:46.84 +73:53:22.1: ref_mag=12.29 +/- 0.01 new_mean_mag=11.3597 delta=0.93 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 11:01:45.12 +73:30:27.1: 12.31 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 11:01:45.12 +73:30:27.1: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter KEPT candidate at 11:01:45.12 +73:30:27.1: ref_mag=12.31 +/- 0.01 new_mean_mag=11.3917 delta=0.92 (need > 0.90)
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-11_01-10-16_20.00sec_-14.90C_LIGHT_0294.fits at 10:45:07.86 +71:15:10.9: 12.28 +/- 0.01 detection
Forced photometry on wcs_Dra-03-Q1b1x1_2026-02-22_00-20-43_20.00sec_-15.00C_LIGHT_0266.fits at 10:45:07.86 +71:15:10.9: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter KEPT candidate at 10:45:07.86 +71:15:10.9: ref_mag=12.28 +/- 0.01 new_mean_mag=11.3065 delta=0.97 (need > 0.90)
Adding exclusion_list_local.txt__out24938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38794.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 1488s
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: 41s
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Considering the candidate 53343_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53343_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (30.3") between the two second-epoch detections
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Considering the candidate 53409_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53409_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 53429_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53429_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 53468_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53468_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (32.4") between the two second-epoch detections
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Considering the candidate 53538_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53538_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
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Considering the candidate 53559_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53559_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (30.1") between the two second-epoch detections
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Considering the candidate 53572_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53572_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
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Considering the candidate 53589_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53589_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (28.1") between the two second-epoch detections
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Considering the candidate 53647_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53647_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (31.6") between the two second-epoch detections
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Considering the candidate 53658_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53658_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 53691_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53691_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 53704_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53704_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (29.3") between the two second-epoch detections
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Considering the candidate 53708_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53708_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 53711_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53711_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (30.1") between the two second-epoch detections
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Considering the candidate 53750_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 53750_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 25200_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25200_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25367_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25367_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 35824_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 35824_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27857_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27857_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 32345_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 32345_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27144_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27144_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36269_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36269_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 32124_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 32124_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 29460_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 29460_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25871_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25871_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 37049_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 37049_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 32258_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 32258_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 26454_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 26454_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 26757_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 26757_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 33424_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 33424_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36663_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36663_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36357_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36357_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25448_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25448_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25040_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25040_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25998_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25998_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 37740_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 37740_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36197_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36197_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 32827_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 32827_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36642_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36642_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 26249_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 26249_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25781_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25781_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36571_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36571_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 35696_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 35696_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25747_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25747_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 33179_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 33179_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36665_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36665_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25044_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25044_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 32006_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 32006_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 33462_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 33462_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27984_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27984_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 33499_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 33499_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 37781_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 37781_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36512_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36512_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 24938_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 24938_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 34650_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 34650_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 33721_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 33721_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 26199_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 26199_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36220_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36220_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 31857_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 31857_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 26710_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 26710_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 34584_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 34584_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27228_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27228_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 34518_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 34518_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25608_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25608_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36396_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36396_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27375_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27375_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 34312_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 34312_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 33743_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 33743_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 35430_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 35430_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
**** FOUND 10:55:41.56 +71:52:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27323_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27323_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 26622_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 26622_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25759_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25759_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36903_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36903_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 26052_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 26052_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 34477_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 34477_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27128_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27128_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25091_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25091_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25487_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25487_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 38794_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 38794_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 35650_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 35650_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27173_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27173_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 37273_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 37273_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 28073_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 28073_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25690_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25690_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 29413_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 29413_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27085_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27085_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 37103_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 37103_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27896_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 27896_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
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Considering the candidate 26110_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 26110_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36809_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36809_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 37408_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 37408_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36995_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36995_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27995_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27995_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25397_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25397_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25783_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25783_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25421_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25421_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36201_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36201_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 27985_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 27985_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 26620_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 26620_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25571_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25571_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 25853_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 25853_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 26963_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 26963_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 36209_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
Preparing report for the candidate 36209_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
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Considering the candidate 23249_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 23249_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
**** FOUND 10:44:38.51 +68:46:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18099_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 18099_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
**** FOUND 11:31:24.51 +69:19:50.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 01192_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 01192_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
**** FOUND 12:55:28.51 +65:26:17.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 05341_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197
The candidate 05341_fd_Dra-03-Q1b1x1_2026-08-22_05-44-19_20.00sec_-0.00C_LIGHTs_0197 did not pass the final checks
**** FOUND 12:59:54.35 +66:35:50.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 1535s
Prepared the HTML report for the field Dra-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:16:27.27 +74:26:14.2
11:07:02.60 +74:09:48.8
11:05:13.12 +74:06:33.7
11:44:31.90 +74:56:58.0
11:13:18.23 +74:17:12.3
12:02:08.84 +75:06:19.5
11:50:18.11 +74:57:24.4
11:41:45.75 +74:48:46.1
10:56:08.27 +73:43:28.2
11:42:27.92 +74:49:23.4
11:45:40.72 +74:50:57.2
11:01:36.82 +73:51:31.3
11:14:10.03 +74:11:06.8
11:09:57.31 +74:03:33.8
11:17:57.01 +74:15:39.7
11:45:06.71 +74:47:17.8
11:11:24.29 +74:05:25.7
11:04:46.84 +73:53:22.1
11:23:18.84 +74:21:21.2
10:54:06.74 +73:30:44.3
11:35:21.99 +74:33:45.8
11:18:14.07 +74:10:41.0
11:16:03.56 +74:05:55.2
11:01:53.90 +73:41:26.1
11:18:50.50 +74:05:56.2
11:09:18.68 +73:48:38.4
10:49:11.50 +73:10:04.3
11:06:15.04 +73:42:08.5
11:54:31.97 +74:40:38.4
11:01:45.12 +73:30:27.1
10:28:59.44 +72:13:20.8
10:49:57.77 +73:04:30.1
10:42:06.71 +72:46:22.3
10:35:33.10 +72:29:38.0
10:59:51.51 +73:23:14.2
11:00:44.88 +73:23:18.8
11:01:59.65 +73:25:09.6
10:34:33.19 +72:15:53.7
11:02:20.79 +73:13:41.9
10:42:33.99 +72:31:21.6
10:28:49.29 +70:32:55.4
10:35:49.91 +70:42:30.3
10:42:33.78 +70:43:57.8
10:30:54.79 +70:10:04.2
10:36:41.59 +70:59:34.0
11:10:00.32 +73:22:27.1
10:36:42.10 +72:02:37.6
10:32:11.85 +71:56:13.6
10:59:59.12 +72:59:36.3
10:36:07.44 +71:55:42.1
10:37:18.65 +71:52:48.2
10:43:23.73 +72:04:55.8
10:52:21.02 +72:23:00.6
10:51:31.75 +72:15:40.3
10:48:06.07 +72:09:58.2
10:44:40.02 +72:01:47.8
10:26:54.12 +71:00:24.8
10:45:00.33 +71:48:07.1
10:41:32.89 +71:37:57.6
10:44:24.84 +71:44:51.1
10:41:27.49 +71:34:59.2
10:53:32.36 +71:47:36.6
10:33:58.40 +70:54:59.8
10:27:00.45 +70:34:02.8
10:33:39.84 +70:46:24.1
10:39:30.16 +71:01:11.2
10:45:07.86 +71:15:10.9
10:45:13.29 +71:15:41.7
10:32:20.40 +70:40:47.3
10:39:59.67 +71:01:29.4
10:39:33.57 +70:59:24.8
10:34:03.16 +70:40:57.7
10:35:32.06 +70:44:33.3
10:34:10.40 +70:39:15.6
10:42:54.25 +71:03:22.5
10:30:02.92 +70:27:27.4
10:36:41.64 +70:42:55.2
10:41:03.16 +70:49:14.5
10:30:13.32 +70:21:37.9
10:37:24.65 +70:40:42.7
10:36:10.46 +70:36:52.7
10:35:58.67 +70:32:47.9
10:41:13.28 +70:44:47.5
10:36:41.43 +70:21:59.0
10:37:30.27 +70:26:34.2
10:31:19.89 +69:49:23.9
########### Completed Dra-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
11:13:18.23 +74:17:12.3
12:02:08.84 +75:06:19.5
10:27:00.45 +70:34:02.8
10:34:33.19 +72:15:53.7
10:59:59.12 +72:59:36.3
10:42:06.71 +72:46:22.3
10:32:20.40 +70:40:47.3
10:36:42.10 +72:02:37.6
10:30:54.79 +70:10:04.2
11:23:18.84 +74:21:21.2
10:37:24.65 +70:40:42.7
10:32:11.85 +71:56:13.6
11:18:50.50 +74:05:56.2
11:54:31.97 +74:40:38.4
10:43:23.73 +72:04:55.8
10:42:54.25 +71:03:22.5
10:39:59.67 +71:01:29.4
10:56:08.27 +73:43:28.2
11:07:02.60 +74:09:48.8
10:54:06.74 +73:30:44.3
10:36:41.43 +70:21:59.0
10:33:39.84 +70:46:24.1
10:36:07.44 +71:55:42.1
10:34:10.40 +70:39:15.6
11:01:53.90 +73:41:26.1
11:45:06.71 +74:47:17.8
10:35:32.06 +70:44:33.3
10:33:58.40 +70:54:59.8
11:09:57.31 +74:03:33.8
10:37:18.65 +71:52:48.2
10:30:02.92 +70:27:27.4
11:05:13.12 +74:06:33.7
11:10:00.32 +73:22:27.1
10:52:21.02 +72:23:00.6
11:02:20.79 +73:13:41.9
10:51:31.75 +72:15:40.3
10:37:30.27 +70:26:34.2
10:34:03.16 +70:40:57.7
11:16:27.27 +74:26:14.2
10:41:27.49 +71:34:59.2
10:48:06.07 +72:09:58.2
11:16:03.56 +74:05:55.2
10:45:13.29 +71:15:41.7
10:36:41.59 +70:59:34.0
11:06:15.04 +73:42:08.5
10:44:24.84 +71:44:51.1
10:59:51.51 +73:23:14.2
10:41:32.89 +71:37:57.6
11:01:36.82 +73:51:31.3
10:39:33.57 +70:59:24.8
11:01:59.65 +73:25:09.6
10:26:54.12 +71:00:24.8
10:44:40.02 +72:01:47.8
11:00:44.88 +73:23:18.8
10:49:11.50 +73:10:04.3
11:17:57.01 +74:15:39.7
10:41:03.16 +70:49:14.5
11:35:21.99 +74:33:45.8
10:45:00.33 +71:48:07.1
10:49:57.77 +73:04:30.1
11:44:31.90 +74:56:58.0
11:42:27.92 +74:49:23.4
10:31:19.89 +69:49:23.9
10:53:32.36 +71:47:36.6
10:35:33.10 +72:29:38.0
10:35:58.67 +70:32:47.9
10:35:49.91 +70:42:30.3
11:14:10.03 +74:11:06.8
10:42:33.78 +70:43:57.8
10:28:59.44 +72:13:20.8
10:36:10.46 +70:36:52.7
11:18:14.07 +74:10:41.0
10:36:41.64 +70:42:55.2
10:41:13.28 +70:44:47.5
10:30:13.32 +70:21:37.9
10:28:49.29 +70:32:55.4
11:50:18.11 +74:57:24.4
11:11:24.29 +74:05:25.7
11:41:45.75 +74:48:46.1
10:39:30.16 +71:01:11.2
10:42:33.99 +72:31:21.6
11:09:18.68 +73:48:38.4
11:45:40.72 +74:50:57.2
11:04:46.84 +73:53:22.1
11:01:45.12 +73:30:27.1
10:45:07.86 +71:15:10.9
###################################################################################
11:13:18.23 +74:17:12.3 -- not an asteroid (will add it to exclusion list)
12:02:08.84 +75:06:19.5 -- not an asteroid (will add it to exclusion list)
10:27:00.45 +70:34:02.8 -- not an asteroid (will add it to exclusion list)
10:34:33.19 +72:15:53.7 -- not an asteroid (will add it to exclusion list)
10:59:59.12 +72:59:36.3 -- not an asteroid (will add it to exclusion list)
10:42:06.71 +72:46:22.3 -- not an asteroid (will add it to exclusion list)
10:32:20.40 +70:40:47.3 -- not an asteroid (will add it to exclusion list)
10:36:42.10 +72:02:37.6 -- not an asteroid (will add it to exclusion list)
10:30:54.79 +70:10:04.2 -- not an asteroid (will add it to exclusion list)
11:23:18.84 +74:21:21.2 -- not an asteroid (will add it to exclusion list)
10:37:24.65 +70:40:42.7 -- not an asteroid (will add it to exclusion list)
10:32:11.85 +71:56:13.6 -- not an asteroid (will add it to exclusion list)
11:18:50.50 +74:05:56.2 -- not an asteroid (will add it to exclusion list)
11:54:31.97 +74:40:38.4 -- not an asteroid (will add it to exclusion list)
10:43:23.73 +72:04:55.8 -- not an asteroid (will add it to exclusion list)
10:42:54.25 +71:03:22.5 -- not an asteroid (will add it to exclusion list)
10:39:59.67 +71:01:29.4 -- not an asteroid (will add it to exclusion list)
10:56:08.27 +73:43:28.2 -- not an asteroid (will add it to exclusion list)
11:07:02.60 +74:09:48.8 -- not an asteroid (will add it to exclusion list)
10:54:06.74 +73:30:44.3 -- not an asteroid (will add it to exclusion list)
10:36:41.43 +70:21:59.0 -- not an asteroid (will add it to exclusion list)
10:33:39.84 +70:46:24.1 -- not an asteroid (will add it to exclusion list)
10:36:07.44 +71:55:42.1 -- not an asteroid (will add it to exclusion list)
10:34:10.40 +70:39:15.6 -- not an asteroid (will add it to exclusion list)
11:01:53.90 +73:41:26.1 -- not an asteroid (will add it to exclusion list)
11:45:06.71 +74:47:17.8 -- not an asteroid (will add it to exclusion list)
10:35:32.06 +70:44:33.3 -- not an asteroid (will add it to exclusion list)
10:33:58.40 +70:54:59.8 -- not an asteroid (will add it to exclusion list)
11:09:57.31 +74:03:33.8 -- not an asteroid (will add it to exclusion list)
10:37:18.65 +71:52:48.2 -- not an asteroid (will add it to exclusion list)
10:30:02.92 +70:27:27.4 -- not an asteroid (will add it to exclusion list)
11:05:13.12 +74:06:33.7 -- not an asteroid (will add it to exclusion list)
11:10:00.32 +73:22:27.1 -- not an asteroid (will add it to exclusion list)
10:52:21.02 +72:23:00.6 -- not an asteroid (will add it to exclusion list)
11:02:20.79 +73:13:41.9 -- not an asteroid (will add it to exclusion list)
10:51:31.75 +72:15:40.3 -- not an asteroid (will add it to exclusion list)
10:37:30.27 +70:26:34.2 -- not an asteroid (will add it to exclusion list)
10:34:03.16 +70:40:57.7 -- not an asteroid (will add it to exclusion list)
11:16:27.27 +74:26:14.2 -- not an asteroid (will add it to exclusion list)
10:41:27.49 +71:34:59.2 -- not an asteroid (will add it to exclusion list)
10:48:06.07 +72:09:58.2 -- not an asteroid (will add it to exclusion list)
11:16:03.56 +74:05:55.2 -- not an asteroid (will add it to exclusion list)
10:45:13.29 +71:15:41.7 -- not an asteroid (will add it to exclusion list)
10:36:41.59 +70:59:34.0 -- not an asteroid (will add it to exclusion list)
11:06:15.04 +73:42:08.5 -- not an asteroid (will add it to exclusion list)
10:44:24.84 +71:44:51.1 -- not an asteroid (will add it to exclusion list)
10:59:51.51 +73:23:14.2 -- not an asteroid (will add it to exclusion list)
10:41:32.89 +71:37:57.6 -- not an asteroid (will add it to exclusion list)
11:01:36.82 +73:51:31.3 -- not an asteroid (will add it to exclusion list)
10:39:33.57 +70:59:24.8 -- not an asteroid (will add it to exclusion list)
11:01:59.65 +73:25:09.6 -- not an asteroid (will add it to exclusion list)
10:26:54.12 +71:00:24.8 -- not an asteroid (will add it to exclusion list)
10:44:40.02 +72:01:47.8 -- not an asteroid (will add it to exclusion list)
11:00:44.88 +73:23:18.8 -- not an asteroid (will add it to exclusion list)
10:49:11.50 +73:10:04.3 -- not an asteroid (will add it to exclusion list)
11:17:57.01 +74:15:39.7 -- not an asteroid (will add it to exclusion list)
10:41:03.16 +70:49:14.5 -- not an asteroid (will add it to exclusion list)
11:35:21.99 +74:33:45.8 -- not an asteroid (will add it to exclusion list)
10:45:00.33 +71:48:07.1 -- not an asteroid (will add it to exclusion list)
10:49:57.77 +73:04:30.1 -- not an asteroid (will add it to exclusion list)
11:44:31.90 +74:56:58.0 -- not an asteroid (will add it to exclusion list)
11:42:27.92 +74:49:23.4 -- not an asteroid (will add it to exclusion list)
10:31:19.89 +69:49:23.9 -- not an asteroid (will add it to exclusion list)
10:53:32.36 +71:47:36.6 -- not an asteroid (will add it to exclusion list)
10:35:33.10 +72:29:38.0 -- not an asteroid (will add it to exclusion list)
10:35:58.67 +70:32:47.9 -- not an asteroid (will add it to exclusion list)
10:35:49.91 +70:42:30.3 -- not an asteroid (will add it to exclusion list)
11:14:10.03 +74:11:06.8 -- not an asteroid (will add it to exclusion list)
10:42:33.78 +70:43:57.8 -- not an asteroid (will add it to exclusion list)
10:28:59.44 +72:13:20.8 -- not an asteroid (will add it to exclusion list)
10:36:10.46 +70:36:52.7 -- not an asteroid (will add it to exclusion list)
11:18:14.07 +74:10:41.0 -- not an asteroid (will add it to exclusion list)
10:36:41.64 +70:42:55.2 -- not an asteroid (will add it to exclusion list)
10:41:13.28 +70:44:47.5 -- not an asteroid (will add it to exclusion list)
10:30:13.32 +70:21:37.9 -- not an asteroid (will add it to exclusion list)
10:28:49.29 +70:32:55.4 -- not an asteroid (will add it to exclusion list)
11:50:18.11 +74:57:24.4 -- not an asteroid (will add it to exclusion list)
11:11:24.29 +74:05:25.7 -- not an asteroid (will add it to exclusion list)
11:41:45.75 +74:48:46.1 -- not an asteroid (will add it to exclusion list)
10:39:30.16 +71:01:11.2 -- not an asteroid (will add it to exclusion list)
10:42:33.99 +72:31:21.6 -- not an asteroid (will add it to exclusion list)
11:09:18.68 +73:48:38.4 -- not an asteroid (will add it to exclusion list)
11:45:40.72 +74:50:57.2 -- not an asteroid (will add it to exclusion list)
11:04:46.84 +73:53:22.1 -- not an asteroid (will add it to exclusion list)
11:01:45.12 +73:30:27.1 -- not an asteroid (will add it to exclusion list)
10:45:07.86 +71:15:10.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
10:26:54.12 +71:00:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:27:00.45 +70:34:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:28:49.29 +70:32:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:28:59.44 +72:13:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:30:02.92 +70:27:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:30:13.32 +70:21:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:30:54.79 +70:10:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:31:19.89 +69:49:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:32:11.85 +71:56:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:32:20.40 +70:40:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:33:39.84 +70:46:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:33:58.40 +70:54:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:34:03.16 +70:40:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:34:10.40 +70:39:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:34:33.19 +72:15:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:35:32.06 +70:44:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:35:33.10 +72:29:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:35:49.91 +70:42:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:35:58.67 +70:32:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:07.44 +71:55:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:10.46 +70:36:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:41.43 +70:21:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:41.59 +70:59:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:41.64 +70:42:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:36:42.10 +72:02:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:37:18.65 +71:52:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:37:24.65 +70:40:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:37:30.27 +70:26:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:39:30.16 +71:01:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:39:33.57 +70:59:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:39:59.67 +71:01:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:41:03.16 +70:49:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:41:13.28 +70:44:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:41:27.49 +71:34:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:41:32.89 +71:37:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:42:06.71 +72:46:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:42:33.78 +70:43:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:42:33.99 +72:31:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:42:54.25 +71:03:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:43:23.73 +72:04:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:44:24.84 +71:44:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:44:40.02 +72:01:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:00.33 +71:48:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:07.86 +71:15:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:13.29 +71:15:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:06.07 +72:09:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:11.50 +73:10:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:57.77 +73:04:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:51:31.75 +72:15:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:52:21.02 +72:23:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:53:32.36 +71:47:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:54:06.74 +73:30:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:56:08.27 +73:43:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:59:51.51 +73:23:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:59:59.12 +72:59:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:00:44.88 +73:23:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:01:36.82 +73:51:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:01:45.12 +73:30:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:01:53.90 +73:41:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:01:59.65 +73:25:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
11:02:20.79 +73:13:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
11:04:46.84 +73:53:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:05:13.12 +74:06:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:06:15.04 +73:42:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
11:07:02.60 +74:09:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:09:18.68 +73:48:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:09:57.31 +74:03:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:10:00.32 +73:22:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:11:24.29 +74:05:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:13:18.23 +74:17:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
11:14:10.03 +74:11:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:03.56 +74:05:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:16:27.27 +74:26:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:17:57.01 +74:15:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:14.07 +74:10:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:18:50.50 +74:05:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:23:18.84 +74:21:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:35:21.99 +74:33:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:41:45.75 +74:48:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
11:42:27.92 +74:49:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:44:31.90 +74:56:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
11:45:06.71 +74:47:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
11:45:40.72 +74:50:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
11:50:18.11 +74:57:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
11:54:31.97 +74:40:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:02:08.84 +75:06:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
10:26:54.12 +71:00:24.8 -- not a known variable star
10:27:00.45 +70:34:02.8 -- not a known variable star
10:28:49.29 +70:32:55.4 -- not a known variable star
10:28:59.44 +72:13:20.8 -- not a known variable star
10:30:02.92 +70:27:27.4 -- a known variable star
10:30:13.32 +70:21:37.9 -- not a known variable star
10:30:54.79 +70:10:04.2 -- not a known variable star
10:31:19.89 +69:49:23.9 -- a known variable star
10:32:11.85 +71:56:13.6 -- not a known variable star
10:32:20.40 +70:40:47.3 -- not a known variable star
10:33:39.84 +70:46:24.1 -- not a known variable star
10:33:58.40 +70:54:59.8 -- not a known variable star
10:34:03.16 +70:40:57.7 -- not a known variable star
10:34:10.40 +70:39:15.6 -- not a known variable star
10:34:33.19 +72:15:53.7 -- not a known variable star
10:35:32.06 +70:44:33.3 -- not a known variable star
10:35:33.10 +72:29:38.0 -- not a known variable star
10:35:49.91 +70:42:30.3 -- not a known variable star
10:35:58.67 +70:32:47.9 -- not a known variable star
10:36:07.44 +71:55:42.1 -- not a known variable star
10:36:10.46 +70:36:52.7 -- not a known variable star
10:36:41.43 +70:21:59.0 -- not a known variable star
10:36:41.59 +70:59:34.0 -- not a known variable star
10:36:41.64 +70:42:55.2 -- not a known variable star
10:36:42.10 +72:02:37.6 -- not a known variable star
10:37:18.65 +71:52:48.2 -- not a known variable star
10:37:24.65 +70:40:42.7 -- not a known variable star
10:37:30.27 +70:26:34.2 -- not a known variable star
10:39:30.16 +71:01:11.2 -- not a known variable star
10:39:33.57 +70:59:24.8 -- not a known variable star
10:39:59.67 +71:01:29.4 -- not a known variable star
10:41:03.16 +70:49:14.5 -- not a known variable star
10:41:13.28 +70:44:47.5 -- not a known variable star
10:41:27.49 +71:34:59.2 -- not a known variable star
10:41:32.89 +71:37:57.6 -- not a known variable star
10:42:06.71 +72:46:22.3 -- not a known variable star
10:42:33.78 +70:43:57.8 -- not a known variable star
10:42:33.99 +72:31:21.6 -- not a known variable star
10:42:54.25 +71:03:22.5 -- a known variable star
10:43:23.73 +72:04:55.8 -- not a known variable star
10:44:24.84 +71:44:51.1 -- not a known variable star
10:44:40.02 +72:01:47.8 -- not a known variable star
10:45:00.33 +71:48:07.1 -- not a known variable star
10:45:07.86 +71:15:10.9 -- not a known variable star
10:45:13.29 +71:15:41.7 -- not a known variable star
10:48:06.07 +72:09:58.2 -- not a known variable star
10:49:11.50 +73:10:04.3 -- not a known variable star
10:49:57.77 +73:04:30.1 -- not a known variable star
10:51:31.75 +72:15:40.3 -- not a known variable star
10:52:21.02 +72:23:00.6 -- not a known variable star
10:53:32.36 +71:47:36.6 -- not a known variable star
10:54:06.74 +73:30:44.3 -- not a known variable star
10:56:08.27 +73:43:28.2 -- not a known variable star
10:59:51.51 +73:23:14.2 -- not a known variable star
10:59:59.12 +72:59:36.3 -- a known variable star
11:00:44.88 +73:23:18.8 -- not a known variable star
11:01:36.82 +73:51:31.3 -- not a known variable star
11:01:45.12 +73:30:27.1 -- not a known variable star
11:01:53.90 +73:41:26.1 -- not a known variable star
11:01:59.65 +73:25:09.6 -- not a known variable star
11:02:20.79 +73:13:41.9 -- not a known variable star
11:04:46.84 +73:53:22.1 -- not a known variable star
11:05:13.12 +74:06:33.7 -- not a known variable star
11:06:15.04 +73:42:08.5 -- not a known variable star
11:07:02.60 +74:09:48.8 -- a known variable star
11:09:18.68 +73:48:38.4 -- not a known variable star
11:09:57.31 +74:03:33.8 -- not a known variable star
11:10:00.32 +73:22:27.1 -- not a known variable star
11:11:24.29 +74:05:25.7 -- not a known variable star
11:13:18.23 +74:17:12.3 -- not a known variable star
11:14:10.03 +74:11:06.8 -- not a known variable star
11:16:03.56 +74:05:55.2 -- not a known variable star
11:16:27.27 +74:26:14.2 -- not a known variable star
11:17:57.01 +74:15:39.7 -- not a known variable star
11:18:14.07 +74:10:41.0 -- not a known variable star
11:18:50.50 +74:05:56.2 -- not a known variable star
11:23:18.84 +74:21:21.2 -- a known variable star
11:35:21.99 +74:33:45.8 -- not a known variable star
11:41:45.75 +74:48:46.1 -- not a known variable star
11:42:27.92 +74:49:23.4 -- not a known variable star
11:44:31.90 +74:56:58.0 -- a known variable star
11:45:06.71 +74:47:17.8 -- not a known variable star
11:45:40.72 +74:50:57.2 -- not a known variable star
11:50:18.11 +74:57:24.4 -- not a known variable star
11:54:31.97 +74:40:38.4 -- not a known variable star
12:02:08.84 +75:06:19.5 -- not a known variable star
Found 79 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
86 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 86 (excluding asteroids and hot pixels, 79 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461274.94694641 -observatory V36
09:45:56.39 +15:15:31.0 Mercury (-1.7mag)
12:50:30.21 -07:49:06.7 Venus (-4.5mag)
06:30:07.57 +23:38:53.9 Mars (1.3mag)
08:55:34.79 +17:52:45.3 Jupiter (-1.8mag)
00:54:48.37 +03:01:25.8 Saturn (0.5mag)
04:13:02.63 +21:00:20.3 Uranus (5.7mag)
00:15:07.57 +00:06:13.5 Neptune (7.7mag)
20:26:50.14 -23:35:13.8 Pluto (14.5mag)
17:32:29.42 -28:19:52.0 Moon (-11.0mag)
-rw-r--r-- 1 apache apache 363 Aug 22 05:49 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461274.94694641:
08:55:36.50 +17:52:37.3 Io (6.1mag)
08:55:43.33 +17:52:06.5 Europa (6.3mag)
08:55:51.28 +17:51:29.9 Ganymede (5.6mag)
08:55:16.02 +17:54:13.6 Callisto (6.9mag)
08:53:03.04 +18:00:49.0 Himalia (15.7mag)
08:55:32.78 +17:52:54.9 Thebe (16.6mag)
08:52:42.30 +17:56:40.3 Elara (17.7mag)
08:59:42.34 +17:25:58.4 Pasiphae (17.9mag)
08:57:47.52 +18:06:21.7 Carme (19.0mag)
00:54:44.31 +03:01:51.1 Titan (8.4mag)
00:54:52.85 +03:01:18.3 Rhea (9.7mag)
00:55:23.85 +03:03:07.6 Iapetus (11.1mag)
00:54:55.84 +03:01:43.1 Hyperion (14.4mag)
00:53:53.03 +02:52:50.5 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 22 05:50 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461274.94694641:
20:12:14.71 -13:57:51.1 JWST
17:44:13.02 +32:42:54.1 Chandra
12:12:50.22 -61:51:36.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 22 05:49 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461274.94694641 -observatory V36
03:28:20.18 +18:26:50.5 17.5mag P/1996 R2 (Lagerkvist)
17:59:54.75 -34:28:29.7 14.2mag P/2010 H2 (Vales)
07:06:35.00 -69:29:40.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:13:09.71 +33:18:34.9 17.7mag C/2017 K2 (PANSTARRS)
04:21:18.98 +42:25:55.1 17.5mag P/2021 N1 (ZTF)
22:26:39.23 +30:22:10.3 17.4mag C/2022 E2 (ATLAS)
06:56:59.58 +26:16:54.7 16.8mag C/2022 N2 (PANSTARRS)
10:34:47.54 +27:50:53.8 17.0mag C/2022 QE78 (ATLAS)
09:38:21.80 +05:17:58.7 18.0mag C/2022 R6 (PANSTARRS)
15:15:41.49 -12:52:56.1 18.0mag P/2023 B1 (PANSTARRS)
20:53:20.02 +64:03:21.9 18.0mag C/2023 H5 (Lemmon)
15:36:25.64 -14:14:28.1 14.6mag C/2023 R1 (PANSTARRS)
08:23:21.11 +32:01:02.0 15.5mag C/2024 E1 (Wierzchos)
15:05:42.17 +15:30:12.9 17.8mag C/2024 G6 (ATLAS)
18:46:45.90 +43:29:22.7 13.7mag C/2024 J3 (ATLAS)
20:49:16.37 +49:41:20.1 17.5mag C/2024 R4 (PANSTARRS)
05:25:49.45 -12:53:58.3 15.3mag C/2024 T5 (ATLAS)
07:04:39.52 +21:35:27.0 17.9mag C/2025 J1 (Borisov)
10:53:24.23 +19:57:05.6 17.1mag C/2025 V2 (Rankin)
13:07:27.60 +01:20:51.3 16.9mag C/2025 Y1 (ATLAS)
16:10:36.56 +76:16:42.0 16.5mag C/2026 A2 (Bok)
03:09:55.31 +46:21:00.2 17.3mag C/2026 B2 (Sun-Gao)
11:58:56.04 +09:56:09.7 17.4mag A/2026 E1
22:12:28.64 -32:19:34.8 7.1mag 10P/Tempel
11:37:46.76 -04:19:36.4 16.3mag 29P/Schwassmann-Wachmann
11:36:35.65 -00:00:18.0 17.4mag 63P/Wild
00:51:35.77 -06:06:27.3 15.4mag 65P/Gunn
06:06:58.34 +20:14:20.1 13.7mag 78P/Gehrels
20:25:45.68 -25:00:26.2 17.5mag 84P/Giclas
03:12:02.78 +14:32:28.7 16.9mag 88P/Howell
08:30:42.86 +25:34:21.1 16.4mag 93P/Lovas
04:47:50.29 +22:26:54.2 17.2mag 112P/Urata-Niijima
06:42:50.92 +28:16:55.4 16.1mag 114P/Wiseman-Skiff
09:51:51.47 +24:04:37.9 14.9mag 123P/West-Hartley
12:12:42.40 -15:38:17.7 17.3mag 124P/Mrkos
05:56:52.44 +21:01:40.3 16.0mag 128P/Shoemaker-Holt
06:52:05.55 +18:05:42.9 17.9mag 131P/Mueller
23:59:35.47 +03:05:50.9 17.4mag 139P/Vaisala-Oterma
03:09:30.44 -18:37:23.3 12.8mag 161P/Hartley-IRAS
08:03:54.17 +38:07:17.5 16.1mag 162P/Siding Spring
11:03:15.09 +29:48:30.9 12.2mag 169P/NEAT
03:06:18.18 +09:23:30.0 17.6mag 220P/McNaught
20:16:19.69 -51:47:52.3 18.0mag 259P/Garradd
04:03:31.39 +30:51:46.4 15.3mag 260P/McNaught
07:47:33.72 +37:04:57.3 17.3mag 295P/LINEAR
15:16:13.86 +01:32:41.1 17.8mag 391P/Kowalski
09:13:47.73 +17:39:48.0 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.3K Aug 22 05:49 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
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
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
-rw-r--r-- 1 apache apache 5.7K Aug 22 05:49 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
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
-rw-r--r-- 1 apache apache 190K Aug 22 05:49 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:27:30.457 +02:47:32.36 AT 2026xfu 2026-01-14.53 21.69
17:59:19.284 +29:24:54.02 AT 2026xft 2026-07-18.43 20.84
19:54:12.936 -24:01:35.76 AT 2026xfs 2026-05-17.56 19.77
08:44:08.771 +29:07:45.05 AT 2026xfr 2026-01-14.38 20.4
23:28:59.311 -21:41:17.71 AT 2026xfq 2026-07-19.57 21.15
20:34:55.430 -31:12:10.98 AT 2026xfp 2026-07-14.44 20
13:01:30.092 +38:12:35.50 AT 2026xfo 2026-06-23.28 20.85
23:22:05.758 +18:57:29.94 AT 2026xfn 2026-07-25.52 21.28
10:13:35.246 -20:37:42.73 AT 2026xfm 2026-01-27.58 21
21:57:25.287 +03:48:20.98 AT 2026xfl 2026-07-16.55 21.68
14:26:07.382 +33:39:52.18 AT 2026xfk 2026-06-13.34 20.9
02:09:31.559 -03:10:04.80 AT 2026xfj 2026-01-17.24 21.98
20:17:01.562 -20:06:27.94 AT 2026xfi 2026-05-20.56 20.93
21:08:09.912 -21:12:24.85 AT 2026xfh 2026-06-19.58 20.9
20:08:20.135 -25:53:36.34 AT 2026xfg 2026-07-19.45 20.74
14:51:25.078 +41:07:07.07 AT 2026xff 2026-06-13.34 21.62
22:33:15.210 +12:04:33.49 AT 2026xfe 2026-06-21.53 20.23
13:52:05.795 +29:21:47.19 AT 2026xfd 2026-04-24.32 20.92
13:30:27.613 +10:38:39.93 AT 2026xfc 2026-04-20.32 21.07
13:40:18.442 +39:30:10.71 AT 2026xfb 2026-05-24.29 20.6
-rw-r--r-- 1 apache apache 87K Aug 22 05:49 tns_transients_list.txt
