This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t
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 06 15.1716 2461206.6716 12.02 10:59:26.75 +22:03:53.4
218.02830 64.10103 galactic Leo Second-epoch detections are separated by 2.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.511 Davida -0 -0 0 12.3 -0 0
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:59:26.75 +22:03:53.4: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:59:26.75 +22:03:53.4: 16.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 15.1716* 10 59 26.75 +22 03 53.4 12.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461206.6716,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260615.1716 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.06 10:46:01.30 +23:36:54.5
212.96378 61.52654 galactic LMi Second-epoch detections are separated by 2.0" and 4.1 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 | 10:46:01.30 +23:36:54.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.407+/-0.029 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:01.30 +23:36:54.5: 13.07 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:01.30 +23:36:54.5: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 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,2461206.6716,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.36 10:49:04.00 +24:49:43.5
210.76457 62.46943 galactic LMi Second-epoch detections are separated by 1.1" and 3.7 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 | 10:49:04.00 +24:49:43.5 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.319+/-0.030 (F)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:04.00 +24:49:43.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:04.00 +24:49:43.5: 13.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.30 10:51:06.49 +25:33:53.1
209.37325 63.06070 galactic LMi Second-epoch detections are separated by 1.4" and 3.9 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 | 10:51:06.49 +25:33:53.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.337+/-0.032 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:06.49 +25:33:53.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:06.49 +25:33:53.1: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 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,2461206.6716,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.36 10:49:29.16 +25:16:57.2
209.83766 62.64973 galactic LMi Second-epoch detections are separated by 1.2" and 3.5 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 | 10:49:29.16 +25:16:57.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.409+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:29.16 +25:16:57.2: 13.38 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:29.16 +25:16:57.2: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.32 10:49:59.26 +25:53:24.5
208.57373 62.86708 galactic LMi Second-epoch detections are separated by 2.1" and 3.6 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 | 10:49:59.26 +25:53:24.5 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.342+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:59.26 +25:53:24.5: 13.40 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:59.26 +25:53:24.5: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.38 10:47:34.32 +25:42:25.0
208.76755 62.30031 galactic LMi Second-epoch detections are separated by 0.9" and 3.7 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 | 10:47:34.32 +25:42:25.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.344+/-0.030 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:34.32 +25:42:25.0: 13.61 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:34.32 +25:42:25.0: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 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,2461206.6716,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.19 10:46:31.17 +25:32:47.7
209.01704 62.03871 galactic LMi Second-epoch detections are separated by 0.7" and 3.6 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 | 10:46:31.17 +25:32:47.7 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.776+/-0.028 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:31.17 +25:32:47.7: 13.47 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:31.17 +25:32:47.7: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 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,2461206.6716,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.35 10:47:42.71 +25:33:40.3
209.08815 62.30598 galactic LMi Second-epoch detections are separated by 1.1" and 3.9 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 | 10:47:42.71 +25:33:40.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.332+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:42.71 +25:33:40.3: 13.48 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:42.71 +25:33:40.3: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 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,2461206.6716,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.62 10:49:53.30 +25:43:51.8
208.90920 62.81849 galactic LMi Second-epoch detections are separated by 0.7" and 3.7 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 J162.4724+25.7308 | 10:49:53.30 +25:43:51.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.446+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:53.30 +25:43:51.8: 13.69 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:53.30 +25:43:51.8: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J162.4724+25.7308,2461206.6716,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J162.4724+25.7308 20260615.1716 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.40 10:47:54.96 +24:47:51.5
210.71773 62.20737 galactic LMi Second-epoch detections are separated by 0.7" and 3.8 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 | 10:47:54.96 +24:47:51.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.500+/-0.030 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:54.96 +24:47:51.5: 13.69 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:54.96 +24:47:51.5: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.43 10:48:17.60 +25:54:37.4
208.39366 62.49457 galactic LMi Second-epoch detections are separated by 1.1" and 3.8 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 | 10:48:17.60 +25:54:37.4 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.311+/-0.030 (F)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:17.60 +25:54:37.4: 13.68 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:17.60 +25:54:37.4: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.38 10:46:08.58 +26:06:30.5
207.80511 62.04996 galactic LMi Second-epoch detections are separated by 0.9" and 3.7 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 | 10:46:08.58 +26:06:30.5 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.772+/-0.030 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:08.58 +26:06:30.5: 13.66 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:08.58 +26:06:30.5: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.61 10:45:51.92 +25:03:31.9
209.97705 61.80302 galactic LMi Second-epoch detections are separated by 0.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 723885509034097792 | 10:45:51.96 +25:03:31.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G3 (LAMOST DR5) J-Ks=0.350+/-0.034 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:51.92 +25:03:31.9: 12.64 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:51.92 +25:03:31.9: 12.66 +/- 0.01 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
Large-amplitude variable Gaia DR2 723885509034097792,2461206.6716,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 723885509034097792 20260615.1716 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 06 15.1716 2461206.6716 12.50 10:49:09.23 +25:50:48.3
208.59952 62.67492 galactic LMi Second-epoch detections are separated by 1.6" and 3.5 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 | 10:49:09.23 +25:50:48.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.386+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:09.23 +25:50:48.3: 13.64 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:09.23 +25:50:48.3: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.60 +/- 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,2461206.6716,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.44 10:46:39.17 +25:32:40.5
209.03263 62.06796 galactic LMi Second-epoch detections are separated by 1.0" and 3.8 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 | 10:46:39.17 +25:32:40.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.488+/-0.033 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:39.17 +25:32:40.5: 13.64 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:39.17 +25:32:40.5: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.45 10:49:51.08 +25:40:38.5
209.02188 62.80112 galactic LMi Second-epoch detections are separated by 1.2" and 3.9 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 | 10:49:51.08 +25:40:38.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.548+/-0.028 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:51.08 +25:40:38.5: 13.62 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:51.08 +25:40:38.5: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 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,2461206.6716,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.54 10:47:15.31 +25:22:31.4
209.44087 62.17124 galactic LMi Second-epoch detections are separated by 0.8" and 3.6 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 | 10:47:15.31 +25:22:31.4 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.353+/-0.029 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:15.31 +25:22:31.4: 13.60 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:15.31 +25:22:31.4: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461206.6716,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.21 10:49:22.18 +25:57:22.3
208.38147 62.74079 galactic LMi Second-epoch detections are separated by 0.7" and 3.6 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 | 10:49:22.18 +25:57:22.3 (user input) | T | P | (position from user input) SpType: F4 (LAMOST DR5) J-Ks=0.267+/-0.028 (F)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:22.18 +25:57:22.3: 13.28 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:22.18 +25:57:22.3: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.19 10:48:09.20 +25:45:24.9
208.70959 62.43784 galactic LMi Second-epoch detections are separated by 1.9" and 3.9 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 | 10:48:09.20 +25:45:24.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.372+/-0.029 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:09.20 +25:45:24.9: 13.27 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:09.20 +25:45:24.9: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 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,2461206.6716,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.13 10:46:38.65 +25:03:06.4
210.06411 61.97471 galactic LMi Second-epoch detections are separated by 0.2" and 3.7 pix
The object was found in VSX 1" ASASSN-V J104638.62+250306.9
Type: SR
# Max. Min./Amp. JD0 Period
13.260 V 13.360 V 2458196.00000 235.000000000000 C-H
The object was not found in astcheck.
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:38.65 +25:03:06.4: 13.27 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:38.65 +25:03:06.4: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104638.62+250306.9,2461206.6716,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J104638.62+250306.9 20260615.1716 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.10 10:49:45.71 +25:50:01.6
208.67710 62.80766 galactic LMi Second-epoch detections are separated by 0.2" and 3.8 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 | 10:49:45.71 +25:50:01.6 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:45.71 +25:50:01.6: 13.30 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:45.71 +25:50:01.6: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.02 10:46:41.68 +25:46:50.2
208.53949 62.11823 galactic LMi Second-epoch detections are separated by 0.4" and 3.7 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 | 10:46:41.68 +25:46:50.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.404+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:41.68 +25:46:50.2: 13.26 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:41.68 +25:46:50.2: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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,2461206.6716,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.38 10:53:14.40 +25:42:53.0
209.22755 63.55977 galactic LMi Second-epoch detections are separated by 1.0" and 3.7 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 | 10:53:14.40 +25:42:53.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.388+/-0.026 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:53:14.40 +25:42:53.0: 13.25 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:53:14.40 +25:42:53.0: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.35 10:46:52.77 +23:30:19.2
213.28698 61.69112 galactic LMi Second-epoch detections are separated by 1.7" and 3.9 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 | 10:46:52.77 +23:30:19.2 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.027 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:52.77 +23:30:19.2: 13.26 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:52.77 +23:30:19.2: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.68 10:46:27.31 +25:02:43.7
210.05967 61.93149 galactic LMi Second-epoch detections are separated by 0.9" and 3.8 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 723837882141249152 | 10:46:27.37 +25:02:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.229+/-0.030 (F)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:27.31 +25:02:43.7: 12.61 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:27.31 +25:02:43.7: 12.62 +/- 0.01 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 723837882141249152,2461206.6716,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 723837882141249152 20260615.1716 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 06 15.1716 2461206.6716 12.03 10:48:11.02 +25:01:50.9
210.25228 62.31279 galactic LMi Second-epoch detections are separated by 1.5" and 3.7 pix
The object was found in VSX 1" Gaia DR3 723849328229610624
Type: ROT
# Max. Min./Amp. JD0 Period
12.860 G 12.880 G G
The object was not found in astcheck.
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:11.02 +25:01:50.9: 13.00 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:11.02 +25:01:50.9: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 723849328229610624,2461206.6716,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 723849328229610624 20260615.1716 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.20 10:45:47.79 +23:37:02.8
212.93339 61.47699 galactic LMi Second-epoch detections are separated by 1.4" and 3.5 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 | 10:45:47.79 +23:37:02.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.454+/-0.027 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:47.79 +23:37:02.8: 13.23 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:47.79 +23:37:02.8: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.93 10:46:36.02 +25:44:58.8
208.59693 62.09203 galactic LMi Second-epoch detections are separated by 1.1" and 3.6 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 | 10:46:36.02 +25:44:58.8 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.322+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:36.02 +25:44:58.8: 12.97 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:36.02 +25:44:58.8: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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,2461206.6716,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 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 06 15.1716 2461206.6716 12.28 10:47:24.01 +25:39:21.5
208.86111 62.25338 galactic LMi Second-epoch detections are separated by 1.8" and 3.6 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 | 10:47:24.01 +25:39:21.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.611+/-0.027 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:24.01 +25:39:21.5: 13.43 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:24.01 +25:39:21.5: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.37 10:46:37.58 +25:22:43.0
209.37865 62.03218 galactic LMi Second-epoch detections are separated by 0.6" and 3.8 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 | 10:46:37.58 +25:22:43.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.549+/-0.032 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:37.58 +25:22:43.0: 13.41 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:37.58 +25:22:43.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.23 10:47:34.39 +24:54:06.9
210.46559 62.15192 galactic LMi Second-epoch detections are separated by 2.1" and 3.4 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 | 10:47:34.39 +24:54:06.9 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.693+/-0.029 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:34.39 +24:54:06.9: 13.41 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:34.39 +24:54:06.9: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.37 10:47:47.86 +25:04:25.7
210.12540 62.23529 galactic LMi Second-epoch detections are separated by 1.0" and 3.6 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 723852828627554432 | 10:47:47.85 +25:04:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.361+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:47.86 +25:04:25.7: 12.27 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:47.86 +25:04:25.7: 12.30 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 723852828627554432,2461206.6716,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 723852828627554432 20260615.1716 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 06 15.1716 2461206.6716 11.29 10:48:30.45 +25:23:39.6
209.51153 62.45282 galactic LMi Second-epoch detections are separated by 0.3" and 3.7 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 J162.1271+25.3943 | 10:48:30.50 +25:23:39.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=0.701+/-0.028 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:30.45 +25:23:39.6: 12.22 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:30.45 +25:23:39.6: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 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 J162.1271+25.3943,2461206.6716,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J162.1271+25.3943 20260615.1716 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.36 10:49:16.08 +25:48:00.6
208.70895 62.69248 galactic LMi Second-epoch detections are separated by 0.7" and 3.8 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 | 10:49:16.08 +25:48:00.6 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.595+/-0.025 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:16.08 +25:48:00.6: 13.41 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:16.08 +25:48:00.6: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.31 10:45:53.78 +23:20:27.5
213.50638 61.43234 galactic LMi Second-epoch detections are separated by 1.7" and 3.9 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 | 10:45:53.78 +23:20:27.5 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:53.78 +23:20:27.5: 13.42 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:53.78 +23:20:27.5: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 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,2461206.6716,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.28 10:46:35.42 +26:07:09.5
207.81647 62.15082 galactic LMi Second-epoch detections are separated by 0.3" and 3.7 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 | 10:46:35.42 +26:07:09.5 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.034 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:35.42 +26:07:09.5: 13.39 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:35.42 +26:07:09.5: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.16 10:47:39.26 +25:46:26.7
208.63197 62.33004 galactic LMi Second-epoch detections are separated by 0.7" and 3.6 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 | 10:47:39.26 +25:46:26.7 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.605+/-0.026 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:39.26 +25:46:26.7: 13.39 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:39.26 +25:46:26.7: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.99 10:47:38.76 +24:47:53.2
210.69039 62.14744 galactic LMi Second-epoch detections are separated by 1.0" and 3.6 pix
The object was found in VSX 0" Gaia DR3 723634064468825216
Type: ROT
# Max. Min./Amp. JD0 Period
12.700 G 12.730 G K
The object was not found in astcheck.
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:38.76 +24:47:53.2: 12.98 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:38.76 +24:47:53.2: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 723634064468825216,2461206.6716,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 723634064468825216 20260615.1716 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.50 10:46:33.65 +25:28:22.9
209.17493 62.03475 galactic LMi Second-epoch detections are separated by 0.6" and 3.8 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 723924537401524352 | 10:46:33.61 +25:28:22.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.599+/-0.029 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:33.65 +25:28:22.9: 12.54 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:33.65 +25:28:22.9: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 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 723924537401524352,2461206.6716,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 723924537401524352 20260615.1716 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.49 10:47:15.21 +25:49:00.9
208.50841 62.24835 galactic LMi Second-epoch detections are separated by 1.0" and 3.6 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 723948898456251904 | 10:47:15.20 +25:49:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 (LAMOST DR5) J-Ks=0.555+/-0.028 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:15.21 +25:49:00.9: 12.51 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:15.21 +25:49:00.9: 12.50 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 723948898456251904,2461206.6716,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 723948898456251904 20260615.1716 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.45 10:46:51.44 +25:45:32.2
208.59851 62.15063 galactic LMi Second-epoch detections are separated by 0.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 723946974310903936 | 10:46:51.47 +25:45:31.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.379+/-0.027 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:51.44 +25:45:32.2: 12.48 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:51.44 +25:45:32.2: 12.48 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 723946974310903936,2461206.6716,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 723946974310903936 20260615.1716 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 06 15.1716 2461206.6716 11.52 10:48:26.39 +25:54:24.2
208.41325 62.52646 galactic LMi Second-epoch detections are separated by 0.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 729949277006073728 | 10:48:26.44 +25:54:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=0.751+/-0.028 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:26.39 +25:54:24.2: 12.48 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:26.39 +25:54:24.2: 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
Gaia DR3 729949277006073728,2461206.6716,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 729949277006073728 20260615.1716 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 06 15.1716 2461206.6716 12.18 10:46:58.39 +24:36:52.9
211.00712 61.96046 galactic LMi Second-epoch detections are separated by 0.9" and 3.6 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 | ATO J161.7459+24.6162 | 10:46:58.39 +24:36:52.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:58.39 +24:36:52.9: 13.26 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:58.39 +24:36:52.9: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J161.7459+24.6162,2461206.6716,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J161.7459+24.6162 20260615.1716 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.15 10:49:28.38 +25:45:17.5
208.82331 62.73034 galactic LMi Second-epoch detections are separated by 1.4" and 3.7 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 | 10:49:28.38 +25:45:17.5 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.330+/-0.027 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:28.38 +25:45:17.5: 13.24 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:28.38 +25:45:17.5: 13.24 +/- 0.02 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
target,2461206.6716,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.09 10:46:44.32 +25:24:34.3
209.32366 62.06276 galactic LMi Second-epoch detections are separated by 0.7" and 3.8 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 | 10:46:44.32 +25:24:34.3 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:44.32 +25:24:34.3: 13.22 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:44.32 +25:24:34.3: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.19 10:45:57.88 +25:17:15.8
209.51000 61.86847 galactic LMi Second-epoch detections are separated by 1.3" and 3.8 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 | 10:45:57.88 +25:17:15.8 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.771+/-0.030 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:57.88 +25:17:15.8: 13.24 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:57.88 +25:17:15.8: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.26 10:51:14.22 +25:33:44.1
209.38988 63.08887 galactic LMi Second-epoch detections are separated by 0.2" and 3.7 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 | 10:51:14.22 +25:33:44.1 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.286+/-0.029 (F)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:14.22 +25:33:44.1: 13.21 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:14.22 +25:33:44.1: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.11 10:46:32.10 +25:47:54.8
208.48867 62.08586 galactic LMi Second-epoch detections are separated by 1.7" and 3.5 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 | 10:46:32.10 +25:47:54.8 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.329+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:32.10 +25:47:54.8: 13.21 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:32.10 +25:47:54.8: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.19 10:48:23.26 +24:23:28.5
211.61835 62.22811 galactic LMi Second-epoch detections are separated by 0.7" and 3.8 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 | 10:48:23.26 +24:23:28.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.332+/-0.027 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:23.26 +24:23:28.5: 13.21 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:23.26 +24:23:28.5: 13.17 +/- 0.02 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,2461206.6716,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.15 10:49:41.38 +25:25:06.7
209.56459 62.71976 galactic LMi Second-epoch detections are separated by 0.7" and 3.7 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 | 10:49:41.38 +25:25:06.7 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.705+/-0.028 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:41.38 +25:25:06.7: 13.19 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:41.38 +25:25:06.7: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.51 10:46:00.17 +24:42:22.3
210.72119 61.76350 galactic LMi Second-epoch detections are separated by 0.4" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 723724052623715584 | 10:46:00.20 +24:42:22.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.560+/-0.027 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:00.17 +24:42:22.3: 12.45 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:00.17 +24:42:22.3: 12.47 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 723724052623715584,2461206.6716,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 723724052623715584 20260615.1716 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 06 15.1716 2461206.6716 12.19 10:45:49.85 +23:50:06.6
212.49358 61.53566 galactic LMi Second-epoch detections are separated by 1.7" and 3.6 pix
The object was found in VSX 0" Gaia DR3 723465010260596096
Type: ROT
# Max. Min./Amp. JD0 Period
12.850 G 12.880 G K
The object was not found in astcheck.
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:49.85 +23:50:06.6: 13.19 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:49.85 +23:50:06.6: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 723465010260596096,2461206.6716,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 723465010260596096 20260615.1716 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.13 10:49:08.43 +24:24:30.1
211.66099 62.39922 galactic LMi Second-epoch detections are separated by 1.1" and 3.5 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 | 10:49:08.43 +24:24:30.1 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.530+/-0.025 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:08.43 +24:24:30.1: 13.15 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:08.43 +24:24:30.1: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.24 10:51:55.87 +25:30:06.7
209.58235 63.23246 galactic LMi Second-epoch detections are separated by 0.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 729706834692310656 | 10:51:58.41 +25:30:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.366+/-0.030 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:55.87 +25:30:06.7: 13.14 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:55.87 +25:30:06.7: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 729706834692310656,2461206.6716,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 729706834692310656 20260615.1716 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.04 10:49:16.13 +25:57:43.4
208.36082 62.71937 galactic LMi Second-epoch detections are separated by 1.6" and 3.5 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 | 10:49:16.13 +25:57:43.4 (user input) | T | P | (position from user input) J-Ks=0.473+/-0.025 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:16.13 +25:57:43.4: 13.15 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:16.13 +25:57:43.4: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.02 10:47:14.99 +25:53:40.5
208.34363 62.26051 galactic LMi Second-epoch detections are separated by 1.5" and 3.9 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 | 10:47:14.99 +25:53:40.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.376+/-0.029 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:14.99 +25:53:40.5: 13.15 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:14.99 +25:53:40.5: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.19 10:51:37.82 +25:34:04.9
209.41149 63.17723 galactic LMi Second-epoch detections are separated by 1.1" and 3.6 pix
The object was found in VSX 1" Gaia DR3 729707904139627776
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.960 G 12.990 G F
The object was not found in astcheck.
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:37.82 +25:34:04.9: 13.13 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:37.82 +25:34:04.9: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 729707904139627776,2461206.6716,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 729707904139627776 20260615.1716 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.12 10:47:40.54 +26:05:40.3
207.95235 62.38742 galactic LMi Second-epoch detections are separated by 1.2" and 3.7 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 | 10:47:40.54 +26:05:40.3 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.763+/-0.028 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:40.54 +26:05:40.3: 13.12 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:40.54 +26:05:40.3: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 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,2461206.6716,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.35 10:47:29.18 +24:06:49.3
212.10154 61.96712 galactic LMi Second-epoch detections are separated by 1.5" and 3.6 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 | 10:47:29.18 +24:06:49.3 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.397+/-0.029 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:29.18 +24:06:49.3: 13.35 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:29.18 +24:06:49.3: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.93 10:46:03.85 +24:24:34.8
211.33981 61.71524 galactic LMi Second-epoch detections are separated by 1.2" and 3.7 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 | 10:46:03.85 +24:24:34.8 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.378+/-0.033 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:03.85 +24:24:34.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:03.85 +24:24:34.8: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 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 06 15.1716 2461206.6716 11.96 10:46:46.19 +24:29:03.2
211.25771 61.88800 galactic LMi Second-epoch detections are separated by 0.7" and 3.8 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 | 10:46:46.19 +24:29:03.2 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.598+/-0.030 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:46.19 +24:29:03.2: 12.96 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:46.19 +24:29:03.2: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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,2461206.6716,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 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 06 15.1716 2461206.6716 11.99 10:48:41.57 +24:58:47.9
210.40801 62.41611 galactic LMi Second-epoch detections are separated by 0.9" and 3.7 pix
The object was found in VSX 1" ASASSN-V J104841.59+245847.9
Type: ROT
# Max. Min./Amp. JD0 Period
13.400 g Y 0.100 g 2459401.46200 20.060000000000
The object was not found in astcheck.
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:41.57 +24:58:47.9: 12.92 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:41.57 +24:58:47.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104841.59+245847.9,2461206.6716,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J104841.59+245847.9 20260615.1716 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.93 10:47:19.18 +24:39:27.3
210.95227 62.04635 galactic LMi Second-epoch detections are separated by 0.5" and 3.6 pix
The object was found in VSX 0" ASASSN-V J104719.18+243927.5
Type: VAR
# Max. Min./Amp. JD0 Period
13.580 g Y 0.120 g 2458184.70100 19.327000000000
The object was not found in astcheck.
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:19.18 +24:39:27.3: 12.92 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:19.18 +24:39:27.3: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104719.18+243927.5,2461206.6716,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J104719.18+243927.5 20260615.1716 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 06 15.1716 2461206.6716 11.86 10:47:20.74 +23:55:45.8
212.46780 61.89432 galactic LMi Second-epoch detections are separated by 1.2" and 3.6 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 | ATO J161.8359+23.9268 | 10:47:20.74 +23:55:45.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G4 (LAMOST DR5)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:20.74 +23:55:45.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:20.74 +23:55:45.8: 12.89 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J161.8359+23.9268,2461206.6716,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J161.8359+23.9268 20260615.1716 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 06 15.1716 2461206.6716 12.36 10:47:11.27 +25:44:03.2
208.67795 62.21974 galactic LMi Second-epoch detections are separated by 1.6" and 3.8 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 | 10:47:11.27 +25:44:03.2 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.478+/-0.029 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:11.27 +25:44:03.2: 13.56 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:11.27 +25:44:03.2: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 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,2461206.6716,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.03 10:45:56.50 +25:26:17.6
209.19409 61.89100 galactic LMi Second-epoch detections are separated by 0.4" and 3.8 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 723912683291672832 | 10:45:56.50 +25:26:17.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.754+/-0.029 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:56.50 +25:26:17.6: 11.95 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:56.50 +25:26:17.6: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 723912683291672832,2461206.6716,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 723912683291672832 20260615.1716 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.88 10:48:22.28 +25:52:07.6
208.48882 62.50499 galactic LMi Second-epoch detections are separated by 1.7" and 3.9 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 | ATO J162.0892+25.8684 | 10:48:22.28 +25:52:07.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.401+/-0.030 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:22.28 +25:52:07.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:22.28 +25:52:07.6: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J162.0892+25.8684,2461206.6716,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J162.0892+25.8684 20260615.1716 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 06 15.1716 2461206.6716 11.02 10:47:11.83 +26:03:16.0
208.00055 62.27494 galactic LMi Second-epoch detections are separated by 0.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 730711307283597184 | 10:47:11.84 +26:03:15.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.399+/-0.027 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:11.83 +26:03:16.0: 11.94 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:11.83 +26:03:16.0: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 730711307283597184,2461206.6716,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 730711307283597184 20260615.1716 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.82 10:46:10.67 +25:18:41.0
209.47961 61.92021 galactic LMi Second-epoch detections are separated by 1.2" and 3.5 pix
The object was found in ASASSN-V 1" ASASSN-V J104610.73+251841.7
Type: ROT:
MeanMag 12.81 m Amp. 0.04 m Period d
The object was not found in astcheck.
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:10.67 +25:18:41.0: 12.85 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:10.67 +25:18:41.0: 12.83 +/- 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
VARIABLE_NAME,2461206.6716,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260615.1716 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 06 15.1716 2461206.6716 11.77 10:46:14.10 +24:52:20.5
210.39917 61.84861 galactic LMi Second-epoch detections are separated by 0.8" and 3.8 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 | 10:46:14.10 +24:52:20.5 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.336+/-0.030 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:14.10 +24:52:20.5: 12.84 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:14.10 +24:52:20.5: 12.81 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.44 10:46:05.65 +25:36:47.1
208.84156 61.95605 galactic LMi Second-epoch detections are separated by 1.8" and 3.9 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 723941171810227072 | 10:46:05.70 +25:36:46.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.395+/-0.032 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:05.65 +25:36:47.1: 12.43 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:05.65 +25:36:47.1: 12.43 +/- 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 723941171810227072,2461206.6716,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 723941171810227072 20260615.1716 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.16 10:48:28.43 +23:34:31.2
213.32892 62.06265 galactic LMi Second-epoch detections are separated by 1.0" and 3.9 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 | 10:48:28.43 +23:34:31.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.402+/-0.030 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:28.43 +23:34:31.2: 13.12 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:28.43 +23:34:31.2: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.12 10:48:33.01 +26:05:26.5
208.02805 62.58066 galactic LMi Second-epoch detections are separated by 1.5" and 3.6 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 | 10:48:33.01 +26:05:26.5 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.027 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:33.01 +26:05:26.5: 13.12 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:33.01 +26:05:26.5: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.40 10:46:24.47 +26:06:30.5
207.82538 62.10865 galactic LMi Second-epoch detections are separated by 0.8" and 3.8 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 730714743257433600 | 10:46:24.47 +26:06:30.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.340+/-0.030 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:24.47 +26:06:30.5: 12.41 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:24.47 +26:06:30.5: 12.40 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 730714743257433600,2461206.6716,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 730714743257433600 20260615.1716 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 06 15.1716 2461206.6716 12.21 10:46:56.79 +25:16:02.3
209.64059 62.08275 galactic LMi Second-epoch detections are separated by 0.8" and 3.7 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 | 10:46:56.79 +25:16:02.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.398+/-0.033 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:56.79 +25:16:02.3: 13.34 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:56.79 +25:16:02.3: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.43 10:50:36.65 +24:59:45.4
210.55735 62.84557 galactic LMi Second-epoch detections are separated by 1.7" and 3.5 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 | 10:50:36.65 +24:59:45.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.350+/-0.027 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:50:36.65 +24:59:45.4: 13.34 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:50:36.65 +24:59:45.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.30 10:47:22.16 +25:38:05.0
208.90346 62.24284 galactic LMi Second-epoch detections are separated by 3.7" and 4.1 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 | 10:47:22.16 +25:38:05.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.357+/-0.029 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:22.16 +25:38:05.0: 13.56 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:22.16 +25:38:05.0: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 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,2461206.6716,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.22 10:47:43.84 +25:59:38.2
208.17081 62.38345 galactic LMi Second-epoch detections are separated by 1.8" and 3.7 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 | 10:47:43.84 +25:59:38.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.244+/-0.028 (F)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:43.84 +25:59:38.2: 13.32 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:43.84 +25:59:38.2: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.14 10:51:13.67 +25:52:09.6
208.71984 63.13883 galactic LMi Second-epoch detections are separated by 0.6" and 3.6 pix
The object was found in VSX 0" Gaia DR3 729907255046050304
Type: ROT
# Max. Min./Amp. JD0 Period
12.980 G 13.000 G G
The object was not found in astcheck.
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:13.67 +25:52:09.6: 13.11 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:13.67 +25:52:09.6: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 729907255046050304,2461206.6716,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 729907255046050304 20260615.1716 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.04 10:47:17.49 +23:54:19.2
212.51150 61.87677 galactic LMi Second-epoch detections are separated by 0.5" and 3.6 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 | 10:47:17.49 +23:54:19.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.476+/-0.027 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:17.49 +23:54:19.2: 13.11 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:17.49 +23:54:19.2: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 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,2461206.6716,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.38 10:47:13.55 +25:55:57.1
208.26131 62.26146 galactic LMi Second-epoch detections are separated by 1.0" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 729957488984043648 | 10:47:13.59 +25:55:56.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.270+/-0.028 (F)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:13.55 +25:55:57.1: 12.35 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:13.55 +25:55:57.1: 12.32 +/- 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
Gaia DR3 729957488984043648,2461206.6716,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 729957488984043648 20260615.1716 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 06 15.1716 2461206.6716 11.88 10:46:35.76 +26:00:07.4
208.06455 62.13320 galactic LMi Second-epoch detections are separated by 0.7" and 3.7 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 | 10:46:35.76 +26:00:07.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.292+/-0.033 (F)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:35.76 +26:00:07.4: 13.09 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:35.76 +26:00:07.4: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 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,2461206.6716,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 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 06 15.1716 2461206.6716 11.80 10:45:50.01 +23:55:44.9
212.30191 61.55783 galactic LMi Second-epoch detections are separated by 0.6" and 3.8 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 | 10:45:50.01 +23:55:44.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.423+/-0.030 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:50.01 +23:55:44.9: 12.80 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:50.01 +23:55:44.9: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.13 10:46:44.93 +24:15:33.0
211.72166 61.83507 galactic LMi Second-epoch detections are separated by 0.2" and 3.7 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 | 10:46:44.93 +24:15:33.0 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.509+/-0.029 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:44.93 +24:15:33.0: 13.10 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:44.93 +24:15:33.0: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 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,2461206.6716,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.09 10:49:49.83 +25:37:18.3
209.13993 62.78692 galactic LMi Second-epoch detections are separated by 0.5" and 3.7 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 | 10:49:49.83 +25:37:18.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.378+/-0.028 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:49.83 +25:37:18.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:49.83 +25:37:18.3: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 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,2461206.6716,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 11.94 10:47:28.15 +26:03:31.0
208.01281 62.33591 galactic LMi Second-epoch detections are separated by 0.6" and 3.6 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 | 10:47:28.15 +26:03:31.0 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.399+/-0.029 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:28.15 +26:03:31.0: 13.07 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:28.15 +26:03:31.0: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 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,2461206.6716,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 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 06 15.1716 2461206.6716 11.79 10:47:37.79 +25:39:55.1
208.86063 62.30597 galactic LMi Second-epoch detections are separated by 0.3" and 3.7 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 | 10:47:37.79 +25:39:55.1 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.416+/-0.026 (G)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:37.79 +25:39:55.1: 12.76 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:37.79 +25:39:55.1: 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461206.6716,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 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 06 15.1716 2461206.6716 12.04 10:46:13.21 +24:21:03.9
211.47668 61.73738 galactic LMi Second-epoch detections are separated by 1.6" and 3.8 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 | 10:46:13.21 +24:21:03.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.303+/-0.035 (F)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:13.21 +24:21:03.9: 13.06 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:13.21 +24:21:03.9: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 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,2461206.6716,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.10 10:48:00.94 +23:15:34.2
213.92623 61.88369 galactic LMi Second-epoch detections are separated by 2.0" and 3.5 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 | 10:48:00.94 +23:15:34.2 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.302+/-0.027 (F)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:00.94 +23:15:34.2: 13.06 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:00.94 +23:15:34.2: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 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,2461206.6716,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1716 2461206.6716 12.14 10:48:23.67 +25:30:28.7
209.25992 62.44812 galactic LMi Second-epoch detections are separated by 1.0" and 3.6 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 | 10:48:23.67 +25:30:28.7 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.590+/-0.028 (K)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:23.67 +25:30:28.7: 13.30 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:23.67 +25:30:28.7: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6716,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260615.1716 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
First image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Last image: 2461206.67180909 15.06.2026 04:07:14.305 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4406
Objects passed selection criteria: 4370
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 2642.5
Average stars matched: 2584.25 (97.7956 %)
Memory usage VmPeak: 111020 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 14 23:39:23 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: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
First image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Last image: 2461206.67180909 15.06.2026 04:07:14.305 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 219
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 23192
Objects passed selection criteria: 23102
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 15005
Average stars matched: 14505.2 (96.6694 %)
Memory usage VmPeak: 129088 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 14 23:40:33 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.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: 2461206.67134097
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits exists and is non-empty
Saving wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits exists and is non-empty
Saving wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits'
wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits exists and is non-empty
Saving wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits to local_wcs_cache/
'wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits' -> 'local_wcs_cache/wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits'
wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits exists and is non-empty
Saving wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits to local_wcs_cache/
'wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits' -> 'local_wcs_cache/wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (1st reference image)
verification OK: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:04:39.947 +21:57:23.32 J2000 4789.000 3195.000
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The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
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# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits (1st new image)
verification OK: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:05:00.445 +21:59:02.25 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:05:00.445 +21:59:02.25
Angular distance between the image centers 0.0838 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits (2nd new image)
verification OK: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:05:00.197 +21:58:40.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:05:00.197 +21:58:40.93
Angular distance between the image centers 0.0812 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 11:05:00.445 +21:59:02.25
Second-epoch second image center 11:05:00.197 +21:58:40.93
Angular distance between the image centers 0.00600 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits &> /tmp/tmp.hCjDb4663B
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits &> /tmp/tmp.80c6WNRXu5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits &> /tmp/tmp.hPp4ti5Y61
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits &> /tmp/tmp.8TeE1f95Q8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
The reference image (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits) and catalog (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat) found
'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat' -> 'wcsmag.cat'
Read 5863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6102 to 175.2048 deg, Dec +16.0221 to +27.5014 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 157.6102 to 175.2048 deg, Dec 16.0221 to 27.5014 deg
Loaded 4338 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): 3191 out of 3323 total matches.
Matched with Tycho-2 3323 out of 5863 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.852600
a=0.000000 b=1.000000 c=22.852600
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6102 to 175.2048 deg, Dec +16.0221 to +27.5014 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 157.6102 to 175.2048 deg, Dec 16.0221 to 27.5014 deg
Loaded 4338 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): 3191 out of 3323 total matches.
Matched with Tycho-2 3323 out of 5863 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (aperture=6.1)
Read 5873 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6053 to 175.1804 deg, Dec +16.0221 to +27.5014 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 157.6053 to 175.1804 deg, Dec 16.0221 to 27.5014 deg
Loaded 4338 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): 3172 out of 3318 total matches.
Matched with Tycho-2 3318 out of 5873 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits (aperture=6.2)
____ 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: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.1 pix Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
2.6 pix fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
2.7 pix fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
2.1 pix wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.1 pix wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Limiting magnitude estimates:
15.4 mag. Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
15.4 mag. Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
12.0 mag. fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
11.9 mag. fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
All-image limiting magnitude estimate: 11.9 (SNR ) 10.0 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hCjDb4663B (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=376, passed=5863
Got 5863 stars (including 5481 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
util/solve_plate_with_UCAC5 got 5863 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits N_match=944 sigma_overall_arcsec=0.274 sigma_q1_arcsec=0.217 sigma_q2_arcsec=0.328 sigma_q3_arcsec=0.235 sigma_q4_arcsec=0.295 n_q1=218 n_q2=240 n_q3=245 n_q4=241 worst_quadrant_to_overall_ratio=1.199
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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.80c6WNRXu5 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=393, passed=5873
Got 5873 stars (including 5475 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat
util/solve_plate_with_UCAC5 got 5873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5771 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
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits N_match=943 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.277 sigma_q2_arcsec=0.404 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.301 n_q1=217 n_q2=238 n_q3=247 n_q4=241 worst_quadrant_to_overall_ratio=1.306
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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.hPp4ti5Y61 (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_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.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_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=44, passed=1177
Got 1177 stars (including 1133 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat
util/solve_plate_with_UCAC5 got 1177 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.7 to 27.2)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 1134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.7 to 27.2)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 1130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 1130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits N_match=927 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.382 sigma_q2_arcsec=0.484 sigma_q3_arcsec=0.469 sigma_q4_arcsec=0.599 n_q1=224 n_q2=384 n_q3=177 n_q4=142 worst_quadrant_to_overall_ratio=1.290
The image catalog is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits -region wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.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.8TeE1f95Q8 (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_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.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_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
Checking if the catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
WCS catalog name: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=41, passed=1094
Got 1094 stars (including 1051 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat
util/solve_plate_with_UCAC5 got 1094 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.7 to 27.2)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 1047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.7 to 27.2)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 1047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 1047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits N_match=925 sigma_overall_arcsec=0.483 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.502 sigma_q3_arcsec=0.493 sigma_q4_arcsec=0.629 n_q1=206 n_q2=396 n_q3=158 n_q4=165 worst_quadrant_to_overall_ratio=1.302
The image catalog is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits -region wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits sigma_overall=0.274 worst_q_ratio=1.199
ref2=Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits sigma_overall=0.310 worst_q_ratio=1.306
new1=fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits sigma_overall=0.464 worst_q_ratio=1.290
new2=fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits sigma_overall=0.483 worst_q_ratio=1.302
reference average sigma_overall=0.292 worst_q_ratio=1.2525
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176_astrometric_residuals.png (944 matched stars from wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177_astrometric_residuals.png (943 matched stars from wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086_astrometric_residuals.png (927 matched stars from wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087_astrometric_residuals.png (925 matched stars from wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.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_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits'
Saving fully-calibrated image wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits'
Preparing the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits exists and is non-empty
wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits exists and is non-empty
wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits exists and is non-empty
wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (1st reference image)
verification OK: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:04:39.947 +21:57:23.32 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_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits (1st new image)
verification OK: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:05:00.445 +21:59:02.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:05:00.445 +21:59:02.25
Angular distance between the image centers 0.0838 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits (2nd new image)
verification OK: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:05:00.197 +21:58:40.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:05:00.197 +21:58:40.93
Angular distance between the image centers 0.0812 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 11:05:00.445 +21:59:02.25
Second-epoch second image center 11:05:00.197 +21:58:40.93
Angular distance between the image centers 0.00600 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits &> /tmp/tmp.gg8AigToAm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits &> /tmp/tmp.WqzrbYIuDp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits &> /tmp/tmp.1pj54d60Lp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits &> /tmp/tmp.JGnZ95lQv5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
The reference image (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits) and catalog (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat) found
'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat' -> 'wcsmag.cat'
Read 31701 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6097 to 175.2801 deg, Dec +16.0221 to +27.5078 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 157.6097 to 175.2801 deg, Dec 16.0221 to 27.5078 deg
Loaded 4353 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): 3103 out of 3360 total matches.
Matched with Tycho-2 3360 out of 31701 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.749800
a=0.000000 b=1.000000 c=22.749800
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31701 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6097 to 175.2801 deg, Dec +16.0221 to +27.5078 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 157.6097 to 175.2801 deg, Dec 16.0221 to 27.5078 deg
Loaded 4353 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): 3103 out of 3360 total matches.
Matched with Tycho-2 3360 out of 31701 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (aperture=4.8)
Read 31604 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.5943 to 175.2797 deg, Dec +16.0221 to +27.5110 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 157.5943 to 175.2797 deg, Dec 16.0221 to 27.5110 deg
Loaded 4362 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): 3082 out of 3366 total matches.
Matched with Tycho-2 3366 out of 31604 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 119 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.0 pix Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
2.4 pix fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
2.4 pix fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
2.0 pix wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.0 pix wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Limiting magnitude estimates:
15.6 mag. Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
15.6 mag. Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
12.6 mag. fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
12.6 mag. fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.4 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gg8AigToAm (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1119, passed=31691
Got 31691 stars (including 30518 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
util/solve_plate_with_UCAC5 got 31691 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 31378 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
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 31379 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 31379 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits N_match=943 sigma_overall_arcsec=0.262 sigma_q1_arcsec=0.216 sigma_q2_arcsec=0.305 sigma_q3_arcsec=0.223 sigma_q4_arcsec=0.282 n_q1=220 n_q2=244 n_q3=242 n_q4=237 worst_quadrant_to_overall_ratio=1.165
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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.WqzrbYIuDp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1160, passed=31589
Got 31589 stars (including 30375 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat
util/solve_plate_with_UCAC5 got 31589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31160 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
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits N_match=944 sigma_overall_arcsec=0.308 sigma_q1_arcsec=0.276 sigma_q2_arcsec=0.374 sigma_q3_arcsec=0.255 sigma_q4_arcsec=0.308 n_q1=219 n_q2=243 n_q3=244 n_q4=238 worst_quadrant_to_overall_ratio=1.215
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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.1pj54d60Lp (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_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.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_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=151, passed=7643
Got 7643 stars (including 7479 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat
util/solve_plate_with_UCAC5 got 7643 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.2)
Done reading UCAC5 zone files...
Matched 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 7305 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.2)
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 7302 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 7302 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 914 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits N_match=914 sigma_overall_arcsec=0.465 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.498 sigma_q3_arcsec=0.453 sigma_q4_arcsec=0.539 n_q1=223 n_q2=380 n_q3=170 n_q4=141 worst_quadrant_to_overall_ratio=1.159
The image catalog is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits -region wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.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.JGnZ95lQv5 (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_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.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_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
Checking if the catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
WCS catalog name: wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=156, passed=7162
Got 7162 stars (including 6993 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat
util/solve_plate_with_UCAC5 got 7162 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.2)
Done reading UCAC5 zone files...
Matched 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 6851 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
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.2)
Done reading UCAC5 zone files...
Matched 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 6849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 6849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 915 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits N_match=915 sigma_overall_arcsec=0.475 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.492 sigma_q3_arcsec=0.506 sigma_q4_arcsec=0.531 n_q1=213 n_q2=396 n_q3=144 n_q4=162 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits -region wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.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_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.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_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-06-33_20.00sec_5.00C_LIGHT_0086.fits
Saving fully-calibrated image wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.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_2026-06-14_CI_Leo-03-Q2b1x1_233711_TTUQ2b1x1_2547304_fHwYZC5t/wcs_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087.fits
Preparing the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:59:26.75 +22:03:53.4: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:01.30 +23:36:54.5: 13.07 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:29.16 +25:16:57.2: 13.38 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:06.49 +25:33:53.1: 13.18 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:04.00 +24:49:43.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:59.26 +25:53:24.5: 13.40 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:34.32 +25:42:25.0: 13.61 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:31.17 +25:32:47.7: 13.47 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:59:26.75 +22:03:53.4: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:42.71 +25:33:40.3: 13.48 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:53.30 +25:43:51.8: 13.69 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:04.00 +24:49:43.5: 13.28 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:01.30 +23:36:54.5: 13.08 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:06.49 +25:33:53.1: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 10:49:04.00 +24:49:43.5: ref_mag=13.29 +/- 0.02 new_mean_mag=12.3527 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:01.30 +23:36:54.5: ref_mag=13.07 +/- 0.01 new_mean_mag=12.0535 delta=1.02 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:34.32 +25:42:25.0: 13.60 +/- 0.03 detection
Forced photometry filter KEPT candidate at 10:51:06.49 +25:33:53.1: ref_mag=13.22 +/- 0.02 new_mean_mag=12.3047 delta=0.91 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:59.26 +25:53:24.5: 13.38 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:29.16 +25:16:57.2: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:31.17 +25:32:47.7: 13.47 +/- 0.03 detection
Forced photometry filter KEPT candidate at 10:47:34.32 +25:42:25.0: ref_mag=13.61 +/- 0.02 new_mean_mag=12.3564 delta=1.25 (need > 0.90)
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 10:49:59.26 +25:53:24.5: ref_mag=13.39 +/- 0.02 new_mean_mag=12.3189 delta=1.07 (need > 0.90)
Forced photometry filter KEPT candidate at 10:49:29.16 +25:16:57.2: ref_mag=13.35 +/- 0.02 new_mean_mag=12.3540 delta=0.99 (need > 0.90)
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:31.17 +25:32:47.7: ref_mag=13.47 +/- 0.02 new_mean_mag=12.1277 delta=1.34 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:53.30 +25:43:51.8: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 10:49:53.30 +25:43:51.8: ref_mag=13.71 +/- 0.03 new_mean_mag=12.6043 delta=1.10 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:42.71 +25:33:40.3: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:42.71 +25:33:40.3: ref_mag=13.47 +/- 0.02 new_mean_mag=12.3382 delta=1.13 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:54.96 +24:47:51.5: 13.69 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:54.96 +24:47:51.5: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 10:47:54.96 +24:47:51.5: ref_mag=13.66 +/- 0.03 new_mean_mag=12.3808 delta=1.28 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:17.60 +25:54:37.4: 13.68 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:17.60 +25:54:37.4: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter KEPT candidate at 10:48:17.60 +25:54:37.4: ref_mag=13.65 +/- 0.03 new_mean_mag=12.4209 delta=1.23 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:08.58 +26:06:30.5: 13.66 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:51.92 +25:03:31.9: 12.64 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:09.23 +25:50:48.3: 13.64 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:39.17 +25:32:40.5: 13.64 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:08.58 +26:06:30.5: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:51.92 +25:03:31.9: 12.66 +/- 0.01 detection
Forced photometry filter KEPT candidate at 10:46:08.58 +26:06:30.5: ref_mag=13.66 +/- 0.03 new_mean_mag=12.3851 delta=1.27 (need > 0.90)
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 10:45:51.92 +25:03:31.9: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6012 delta=1.05 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:09.23 +25:50:48.3: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.02
Forced photometry filter KEPT candidate at 10:49:09.23 +25:50:48.3: ref_mag=13.60 +/- 0.02 new_mean_mag=12.4708 delta=1.13 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:39.17 +25:32:40.5: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry filter KEPT candidate at 10:46:39.17 +25:32:40.5: ref_mag=13.63 +/- 0.03 new_mean_mag=12.4460 delta=1.18 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:51.08 +25:40:38.5: 13.62 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:15.31 +25:22:31.4: 13.60 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:22.18 +25:57:22.3: 13.28 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:51.08 +25:40:38.5: 13.60 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:15.31 +25:22:31.4: 13.67 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:22.18 +25:57:22.3: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Forced photometry reference-image weighted average: 13.63 +/- 0.02
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 10:49:51.08 +25:40:38.5: ref_mag=13.61 +/- 0.02 new_mean_mag=12.4345 delta=1.17 (need > 0.90)
Forced photometry filter KEPT candidate at 10:49:22.18 +25:57:22.3: ref_mag=13.26 +/- 0.02 new_mean_mag=12.1944 delta=1.07 (need > 0.90)
Forced photometry filter KEPT candidate at 10:47:15.31 +25:22:31.4: ref_mag=13.63 +/- 0.02 new_mean_mag=12.4851 delta=1.14 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:09.20 +25:45:24.9: 13.27 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:09.20 +25:45:24.9: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 10:48:09.20 +25:45:24.9: ref_mag=13.27 +/- 0.02 new_mean_mag=12.1854 delta=1.09 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:38.65 +25:03:06.4: 13.27 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:38.65 +25:03:06.4: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:38.65 +25:03:06.4: ref_mag=13.26 +/- 0.02 new_mean_mag=12.1122 delta=1.15 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:45.71 +25:50:01.6: 13.30 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:45.71 +25:50:01.6: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 10:49:45.71 +25:50:01.6: ref_mag=13.28 +/- 0.02 new_mean_mag=12.0957 delta=1.18 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:41.68 +25:46:50.2: 13.26 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:41.68 +25:46:50.2: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:41.68 +25:46:50.2: ref_mag=13.25 +/- 0.02 new_mean_mag=12.0195 delta=1.23 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:53:14.40 +25:42:53.0: 13.25 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:52.77 +23:30:19.2: 13.26 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:53:14.40 +25:42:53.0: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 10:53:14.40 +25:42:53.0: ref_mag=13.28 +/- 0.02 new_mean_mag=12.3652 delta=0.91 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:52.77 +23:30:19.2: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:52.77 +23:30:19.2: ref_mag=13.28 +/- 0.02 new_mean_mag=12.3400 delta=0.94 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:11.02 +25:01:50.9: 13.00 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:27.31 +25:02:43.7: 12.61 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:47.79 +23:37:02.8: 13.23 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:27.31 +25:02:43.7: 12.62 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:11.02 +25:01:50.9: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry reference-image weighted average: 13.01 +/- 0.01
Forced photometry filter KEPT candidate at 10:48:11.02 +25:01:50.9: ref_mag=13.01 +/- 0.01 new_mean_mag=12.0275 delta=0.99 (need > 0.90)
Forced photometry filter KEPT candidate at 10:46:27.31 +25:02:43.7: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6626 delta=0.95 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:47.79 +23:37:02.8: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 10:45:47.79 +23:37:02.8: ref_mag=13.18 +/- 0.02 new_mean_mag=12.1972 delta=0.98 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:36.02 +25:44:58.8: 12.97 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:24.01 +25:39:21.5: 13.43 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:37.58 +25:22:43.0: 13.41 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:36.02 +25:44:58.8: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:36.02 +25:44:58.8: ref_mag=12.97 +/- 0.01 new_mean_mag=11.9176 delta=1.05 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:37.58 +25:22:43.0: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:37.58 +25:22:43.0: ref_mag=13.43 +/- 0.02 new_mean_mag=12.3444 delta=1.08 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:24.01 +25:39:21.5: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:24.01 +25:39:21.5: ref_mag=13.42 +/- 0.02 new_mean_mag=12.2620 delta=1.16 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:34.39 +24:54:06.9: 13.41 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:34.39 +24:54:06.9: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:34.39 +24:54:06.9: ref_mag=13.39 +/- 0.02 new_mean_mag=12.1628 delta=1.23 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:47.86 +25:04:25.7: 12.27 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:47.86 +25:04:25.7: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter KEPT candidate at 10:47:47.86 +25:04:25.7: ref_mag=12.28 +/- 0.01 new_mean_mag=11.3667 delta=0.92 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:30.45 +25:23:39.6: 12.22 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:30.45 +25:23:39.6: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry filter KEPT candidate at 10:48:30.45 +25:23:39.6: ref_mag=12.21 +/- 0.01 new_mean_mag=11.2824 delta=0.92 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:16.08 +25:48:00.6: 13.41 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:16.08 +25:48:00.6: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 10:49:16.08 +25:48:00.6: ref_mag=13.39 +/- 0.02 new_mean_mag=12.3582 delta=1.04 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:53.78 +23:20:27.5: 13.42 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:53.78 +23:20:27.5: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.02
Forced photometry filter KEPT candidate at 10:45:53.78 +23:20:27.5: ref_mag=13.47 +/- 0.02 new_mean_mag=12.3090 delta=1.16 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:35.42 +26:07:09.5: 13.39 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:35.42 +26:07:09.5: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:35.42 +26:07:09.5: ref_mag=13.39 +/- 0.02 new_mean_mag=12.2765 delta=1.11 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:39.26 +25:46:26.7: 13.39 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:38.76 +24:47:53.2: 12.98 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:33.65 +25:28:22.9: 12.54 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:39.26 +25:46:26.7: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:39.26 +25:46:26.7: ref_mag=13.39 +/- 0.02 new_mean_mag=12.1456 delta=1.25 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:15.21 +25:49:00.9: 12.51 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:38.76 +24:47:53.2: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 10:47:38.76 +24:47:53.2: ref_mag=12.97 +/- 0.01 new_mean_mag=11.9558 delta=1.01 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:33.65 +25:28:22.9: 12.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:33.65 +25:28:22.9: ref_mag=12.53 +/- 0.01 new_mean_mag=11.4831 delta=1.05 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:15.21 +25:49:00.9: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter KEPT candidate at 10:47:15.21 +25:49:00.9: ref_mag=12.50 +/- 0.01 new_mean_mag=11.4951 delta=1.01 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:51.44 +25:45:32.2: 12.48 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:51.44 +25:45:32.2: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:51.44 +25:45:32.2: ref_mag=12.48 +/- 0.01 new_mean_mag=11.4431 delta=1.04 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:26.39 +25:54:24.2: 12.48 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:26.39 +25:54:24.2: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter KEPT candidate at 10:48:26.39 +25:54:24.2: ref_mag=12.47 +/- 0.01 new_mean_mag=11.5082 delta=0.96 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:58.39 +24:36:52.9: 13.26 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:58.39 +24:36:52.9: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:58.39 +24:36:52.9: ref_mag=13.28 +/- 0.02 new_mean_mag=12.1705 delta=1.11 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:28.38 +25:45:17.5: 13.24 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:28.38 +25:45:17.5: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 10:49:28.38 +25:45:17.5: ref_mag=13.24 +/- 0.02 new_mean_mag=12.1513 delta=1.09 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:44.32 +25:24:34.3: 13.22 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:44.32 +25:24:34.3: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:44.32 +25:24:34.3: ref_mag=13.21 +/- 0.02 new_mean_mag=12.0734 delta=1.14 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:57.88 +25:17:15.8: 13.24 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:14.22 +25:33:44.1: 13.21 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:57.88 +25:17:15.8: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 10:45:57.88 +25:17:15.8: ref_mag=13.26 +/- 0.02 new_mean_mag=12.1447 delta=1.12 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:14.22 +25:33:44.1: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 10:51:14.22 +25:33:44.1: ref_mag=13.23 +/- 0.02 new_mean_mag=12.2177 delta=1.01 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:32.10 +25:47:54.8: 13.21 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:23.26 +24:23:28.5: 13.21 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:41.38 +25:25:06.7: 13.19 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:32.10 +25:47:54.8: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:32.10 +25:47:54.8: ref_mag=13.21 +/- 0.02 new_mean_mag=12.0912 delta=1.12 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:23.26 +24:23:28.5: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 10:48:23.26 +24:23:28.5: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1580 delta=1.03 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:41.38 +25:25:06.7: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry filter KEPT candidate at 10:49:41.38 +25:25:06.7: ref_mag=13.18 +/- 0.02 new_mean_mag=12.1596 delta=1.02 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:00.17 +24:42:22.3: 12.45 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:00.17 +24:42:22.3: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:00.17 +24:42:22.3: ref_mag=12.46 +/- 0.01 new_mean_mag=11.4947 delta=0.96 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:49.85 +23:50:06.6: 13.19 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:49.85 +23:50:06.6: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 10:45:49.85 +23:50:06.6: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1743 delta=1.00 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:08.43 +24:24:30.1: 13.15 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:08.43 +24:24:30.1: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
Forced photometry filter KEPT candidate at 10:49:08.43 +24:24:30.1: ref_mag=13.12 +/- 0.01 new_mean_mag=12.1368 delta=0.98 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:55.87 +25:30:06.7: 13.14 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:55.87 +25:30:06.7: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 10:51:55.87 +25:30:06.7: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1979 delta=0.93 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:16.13 +25:57:43.4: 13.15 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:16.13 +25:57:43.4: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 10:49:16.13 +25:57:43.4: ref_mag=13.17 +/- 0.02 new_mean_mag=12.0297 delta=1.14 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:14.99 +25:53:40.5: 13.15 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:14.99 +25:53:40.5: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:14.99 +25:53:40.5: ref_mag=13.17 +/- 0.02 new_mean_mag=12.0075 delta=1.17 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:37.82 +25:34:04.9: 13.13 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:37.82 +25:34:04.9: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 10:51:37.82 +25:34:04.9: ref_mag=13.11 +/- 0.02 new_mean_mag=12.1929 delta=0.92 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:40.54 +26:05:40.3: 13.12 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:40.54 +26:05:40.3: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:40.54 +26:05:40.3: ref_mag=13.10 +/- 0.02 new_mean_mag=12.1024 delta=1.00 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:29.18 +24:06:49.3: 13.35 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:03.85 +24:24:34.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:46.19 +24:29:03.2: 12.96 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:29.18 +24:06:49.3: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:29.18 +24:06:49.3: ref_mag=13.33 +/- 0.02 new_mean_mag=12.3342 delta=1.00 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:03.85 +24:24:34.8: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:03.85 +24:24:34.8: ref_mag=12.95 +/- 0.01 new_mean_mag=11.8955 delta=1.05 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:41.57 +24:58:47.9: 12.92 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:46.19 +24:29:03.2: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:46.19 +24:29:03.2: ref_mag=12.97 +/- 0.01 new_mean_mag=11.9625 delta=1.01 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:41.57 +24:58:47.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 10:48:41.57 +24:58:47.9: ref_mag=12.93 +/- 0.01 new_mean_mag=11.9961 delta=0.93 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:19.18 +24:39:27.3: 12.92 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:19.18 +24:39:27.3: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter KEPT candidate at 10:47:19.18 +24:39:27.3: ref_mag=12.95 +/- 0.01 new_mean_mag=11.9156 delta=1.03 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:20.74 +23:55:45.8: 12.91 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:20.74 +23:55:45.8: 12.89 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:11.27 +25:44:03.2: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 10:47:20.74 +23:55:45.8: ref_mag=12.90 +/- 0.01 new_mean_mag=11.8943 delta=1.01 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:11.27 +25:44:03.2: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:11.27 +25:44:03.2: ref_mag=13.59 +/- 0.02 new_mean_mag=12.3669 delta=1.23 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:56.50 +25:26:17.6: 11.95 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:56.50 +25:26:17.6: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Forced photometry filter KEPT candidate at 10:45:56.50 +25:26:17.6: ref_mag=11.95 +/- 0.01 new_mean_mag=11.0215 delta=0.92 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:22.28 +25:52:07.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:22.28 +25:52:07.6: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 10:48:22.28 +25:52:07.6: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8805 delta=0.98 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:11.83 +26:03:16.0: 11.94 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:11.83 +26:03:16.0: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter KEPT candidate at 10:47:11.83 +26:03:16.0: ref_mag=11.93 +/- 0.01 new_mean_mag=11.0121 delta=0.92 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:10.67 +25:18:41.0: 12.85 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:10.67 +25:18:41.0: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:10.67 +25:18:41.0: ref_mag=12.84 +/- 0.01 new_mean_mag=11.7674 delta=1.07 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:14.10 +24:52:20.5: 12.84 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:14.10 +24:52:20.5: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:14.10 +24:52:20.5: ref_mag=12.82 +/- 0.01 new_mean_mag=11.7317 delta=1.09 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:05.65 +25:36:47.1: 12.43 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:33.01 +26:05:26.5: 13.12 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:28.43 +23:34:31.2: 13.12 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:24.47 +26:06:30.5: 12.41 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:28.43 +23:34:31.2: 13.14 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:24.47 +26:06:30.5: 12.40 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:33.01 +26:05:26.5: 13.14 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:05.65 +25:36:47.1: 12.43 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:56.79 +25:16:02.3: 13.34 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:50:36.65 +24:59:45.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter KEPT candidate at 10:48:28.43 +23:34:31.2: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1585 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 10:48:33.01 +26:05:26.5: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1107 delta=1.02 (need > 0.90)
Forced photometry filter KEPT candidate at 10:46:05.65 +25:36:47.1: ref_mag=12.43 +/- 0.01 new_mean_mag=11.4157 delta=1.01 (need > 0.90)
Forced photometry filter KEPT candidate at 10:46:24.47 +26:06:30.5: ref_mag=12.41 +/- 0.01 new_mean_mag=11.3987 delta=1.01 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:41.13 +24:30:54.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:50:36.65 +24:59:45.4: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 10:50:36.65 +24:59:45.4: ref_mag=13.37 +/- 0.02 new_mean_mag=12.4199 delta=0.95 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:56.79 +25:16:02.3: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:56.79 +25:16:02.3: ref_mag=13.36 +/- 0.02 new_mean_mag=12.2001 delta=1.16 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:41.13 +24:30:54.5: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 10:45:41.13 +24:30:54.5: ref_mag=12.96 +/- 0.02 new_mean_mag=11.9965 delta=0.96 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:22.16 +25:38:05.0: 13.56 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:22.16 +25:38:05.0: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:22.16 +25:38:05.0: ref_mag=13.60 +/- 0.02 new_mean_mag=12.3516 delta=1.25 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:43.84 +25:59:38.2: 13.32 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:43.84 +25:59:38.2: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:43.84 +25:59:38.2: ref_mag=13.30 +/- 0.02 new_mean_mag=12.2263 delta=1.08 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:13.67 +25:52:09.6: 13.11 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:13.67 +25:52:09.6: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 10:51:13.67 +25:52:09.6: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1531 delta=0.99 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:17.49 +23:54:19.2: 13.11 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:17.49 +23:54:19.2: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Forced photometry filter KEPT candidate at 10:47:17.49 +23:54:19.2: ref_mag=13.10 +/- 0.01 new_mean_mag=12.0280 delta=1.08 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:13.55 +25:55:57.1: 12.35 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:13.55 +25:55:57.1: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 10:47:13.55 +25:55:57.1: ref_mag=12.34 +/- 0.01 new_mean_mag=11.3646 delta=0.97 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:35.76 +26:00:07.4: 13.09 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:45:50.01 +23:55:44.9: 12.80 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:44.93 +24:15:33.0: 13.10 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:35.76 +26:00:07.4: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 10:46:35.76 +26:00:07.4: ref_mag=13.11 +/- 0.02 new_mean_mag=11.8481 delta=1.26 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:45:50.01 +23:55:44.9: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 10:45:50.01 +23:55:44.9: ref_mag=12.80 +/- 0.01 new_mean_mag=11.7730 delta=1.03 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:44.93 +24:15:33.0: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:44.93 +24:15:33.0: ref_mag=13.08 +/- 0.01 new_mean_mag=12.1309 delta=0.95 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:49:49.83 +25:37:18.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:28.15 +26:03:31.0: 13.07 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:49:49.83 +25:37:18.3: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter KEPT candidate at 10:49:49.83 +25:37:18.3: ref_mag=13.07 +/- 0.01 new_mean_mag=12.0456 delta=1.02 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:28.15 +26:03:31.0: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 10:47:28.15 +26:03:31.0: ref_mag=13.10 +/- 0.02 new_mean_mag=11.9248 delta=1.18 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:37.79 +25:39:55.1: 12.76 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:13.21 +24:21:03.9: 13.06 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:37.79 +25:39:55.1: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 10:47:37.79 +25:39:55.1: ref_mag=12.76 +/- 0.01 new_mean_mag=11.7907 delta=0.97 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:13.21 +24:21:03.9: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:13.21 +24:21:03.9: ref_mag=13.06 +/- 0.01 new_mean_mag=12.0183 delta=1.04 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:00.94 +23:15:34.2: 13.06 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:00.94 +23:15:34.2: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Forced photometry filter KEPT candidate at 10:48:00.94 +23:15:34.2: ref_mag=13.06 +/- 0.01 new_mean_mag=12.1040 delta=0.96 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:48:23.67 +25:30:28.7: 13.30 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:48:23.67 +25:30:28.7: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 10:48:23.67 +25:30:28.7: ref_mag=13.29 +/- 0.02 new_mean_mag=12.1513 delta=1.13 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out50051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51911.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 124s
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: 45s
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Considering the candidate 51723_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51723_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 51725_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51725_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 51729_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51729_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 51733_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51733_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 51741_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51741_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 51760_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51760_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 51765_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51765_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 51791_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51791_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 51801_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51801_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 51815_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51815_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 51832_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51832_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 10:56:23.20 +22:21:28.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 51848_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51848_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 51857_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51857_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 51870_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51870_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 51871_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51871_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 51875_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51875_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 10:55:27.60 +24:43:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51890_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51890_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 51892_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51892_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 51911_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 51911_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 51940_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51940_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 51941_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51941_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 51954_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 51954_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 11558_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 11558_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 07716_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07716_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05390_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05390_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 06273_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 06273_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04491_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04491_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05109_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05109_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05564_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05564_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05497_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05497_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04977_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04977_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07814_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07814_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04485_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04485_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03922_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 03922_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07085_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07085_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04657_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04657_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05583_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05583_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05135_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05135_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06055_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 06055_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04308_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04308_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04930_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04930_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07086_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07086_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04668_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04668_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04896_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04896_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 04910_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04910_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 11913_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 11913_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07110_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07110_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07111_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07111_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11573_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 11573_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04998_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04998_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05227_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05227_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06063_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 06063_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07521_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07521_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06970_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 06970_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05962_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05962_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04788_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04788_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12471_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 12471_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03859_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 03859_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04893_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04893_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07809_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07809_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05781_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05781_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04778_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04778_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04943_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04943_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04445_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04445_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08385_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 08385_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04918_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04918_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05972_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05972_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 06345_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 06345_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 05396_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05396_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 04862_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04862_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 09056_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 09056_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 05872_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05872_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 08106_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 08106_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 10869_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 10869_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 08969_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 08969_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 05555_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05555_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 04293_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04293_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 04567_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04567_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 05357_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05357_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 03914_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 03914_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 09909_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 09909_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 09061_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 09061_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 08825_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 08825_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 07250_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07250_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 08246_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 08246_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 10520_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 10520_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 05030_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05030_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 05881_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05881_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 04594_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04594_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 04024_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04024_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 06272_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 06272_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 07645_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07645_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 05355_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05355_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 11637_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 11637_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 03904_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 03904_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
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Considering the candidate 03886_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 03886_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06390_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 06390_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07157_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 07157_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50051_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 50051_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 10:45:41.13 +24:30:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.388 723714530680514432 161.42139554519 +24.51503266956 12.7786 12.2471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05307_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05307_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04243_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04243_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04514_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04514_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10608_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 10608_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04419_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04419_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04233_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04233_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10559_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 10559_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09466_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 09466_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05259_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05259_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04035_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 04035_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05511_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 05511_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 10:48:41.06 +25:32:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05200_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05200_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09227_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 09227_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12697_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 12697_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05647_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
Preparing report for the candidate 05647_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30613_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 30613_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 11:02:19.80 +20:10:49.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11241_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 11241_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 11:15:12.01 +23:05:42.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22238_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 22238_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 11:14:06.57 +20:31:23.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07283_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 07283_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 10:55:36.92 +24:44:56.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27144_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087
The candidate 27144_fd_Leo-03-Q2b1x1_2026-06-14_23-07-14_20.00sec_4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 11:30:28.73 +18:24:37.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 173s
Prepared the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:46:35.42 +26:07:09.5
10:46:24.47 +26:06:30.5
10:48:33.01 +26:05:26.5
10:47:40.54 +26:05:40.3
10:46:08.58 +26:06:30.5
10:47:11.83 +26:03:16.0
10:47:28.15 +26:03:31.0
10:46:35.76 +26:00:07.4
10:47:43.84 +25:59:38.2
10:49:16.13 +25:57:43.4
10:49:22.18 +25:57:22.3
10:47:13.55 +25:55:57.1
10:48:26.39 +25:54:24.2
10:48:17.60 +25:54:37.4
10:49:59.26 +25:53:24.5
10:51:13.67 +25:52:09.6
10:47:14.99 +25:53:40.5
10:48:22.28 +25:52:07.6
10:49:09.23 +25:50:48.3
10:49:45.71 +25:50:01.6
10:47:15.21 +25:49:00.9
10:49:16.08 +25:48:00.6
10:46:32.10 +25:47:54.8
10:47:39.26 +25:46:26.7
10:46:41.68 +25:46:50.2
10:53:14.40 +25:42:53.0
10:49:28.38 +25:45:17.5
10:48:09.20 +25:45:24.9
10:46:51.44 +25:45:32.2
10:49:53.30 +25:43:51.8
10:46:36.02 +25:44:58.8
10:47:11.27 +25:44:03.2
10:47:34.32 +25:42:25.0
10:49:51.08 +25:40:38.5
10:47:37.79 +25:39:55.1
10:47:24.01 +25:39:21.5
10:49:49.83 +25:37:18.3
10:47:22.16 +25:38:05.0
10:46:05.65 +25:36:47.1
10:51:37.82 +25:34:04.9
10:51:06.49 +25:33:53.1
10:51:14.22 +25:33:44.1
10:47:42.71 +25:33:40.3
10:51:55.87 +25:30:06.7
10:46:31.17 +25:32:47.7
10:46:39.17 +25:32:40.5
10:48:23.67 +25:30:28.7
10:46:33.65 +25:28:22.9
10:49:41.38 +25:25:06.7
10:45:56.50 +25:26:17.6
10:48:30.45 +25:23:39.6
10:46:44.32 +25:24:34.3
10:47:15.31 +25:22:31.4
10:46:37.58 +25:22:43.0
10:46:10.67 +25:18:41.0
10:49:29.16 +25:16:57.2
10:45:57.88 +25:17:15.8
10:46:56.79 +25:16:02.3
10:47:47.86 +25:04:25.7
10:45:51.92 +25:03:31.9
10:46:38.65 +25:03:06.4
10:46:27.31 +25:02:43.7
10:48:11.02 +25:01:50.9
10:50:36.65 +24:59:45.4
10:48:41.57 +24:58:47.9
10:47:34.39 +24:54:06.9
10:46:14.10 +24:52:20.5
10:49:04.00 +24:49:43.5
10:47:38.76 +24:47:53.2
10:47:54.96 +24:47:51.5
10:46:00.17 +24:42:22.3
10:47:19.18 +24:39:27.3
10:46:58.39 +24:36:52.9
10:46:46.19 +24:29:03.2
10:49:08.43 +24:24:30.1
10:48:23.26 +24:23:28.5
10:46:03.85 +24:24:34.8
10:46:13.21 +24:21:03.9
10:46:44.93 +24:15:33.0
10:47:29.18 +24:06:49.3
10:47:20.74 +23:55:45.8
10:45:50.01 +23:55:44.9
10:47:17.49 +23:54:19.2
10:45:49.85 +23:50:06.6
10:46:01.30 +23:36:54.5
10:45:47.79 +23:37:02.8
10:48:28.43 +23:34:31.2
10:46:52.77 +23:30:19.2
10:45:53.78 +23:20:27.5
10:48:00.94 +23:15:34.2
10:59:26.75 +22:03:53.4
########### Completed Leo-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
10:59:26.75 +22:03:53.4
10:46:01.30 +23:36:54.5
10:49:04.00 +24:49:43.5
10:51:06.49 +25:33:53.1
10:49:29.16 +25:16:57.2
10:49:59.26 +25:53:24.5
10:47:34.32 +25:42:25.0
10:46:31.17 +25:32:47.7
10:47:42.71 +25:33:40.3
10:49:53.30 +25:43:51.8
10:47:54.96 +24:47:51.5
10:48:17.60 +25:54:37.4
10:46:08.58 +26:06:30.5
10:45:51.92 +25:03:31.9
10:49:09.23 +25:50:48.3
10:46:39.17 +25:32:40.5
10:49:51.08 +25:40:38.5
10:47:15.31 +25:22:31.4
10:49:22.18 +25:57:22.3
10:48:09.20 +25:45:24.9
10:46:38.65 +25:03:06.4
10:49:45.71 +25:50:01.6
10:46:41.68 +25:46:50.2
10:53:14.40 +25:42:53.0
10:46:52.77 +23:30:19.2
10:46:27.31 +25:02:43.7
10:48:11.02 +25:01:50.9
10:45:47.79 +23:37:02.8
10:46:36.02 +25:44:58.8
10:47:24.01 +25:39:21.5
10:46:37.58 +25:22:43.0
10:47:34.39 +24:54:06.9
10:47:47.86 +25:04:25.7
10:48:30.45 +25:23:39.6
10:49:16.08 +25:48:00.6
10:45:53.78 +23:20:27.5
10:46:35.42 +26:07:09.5
10:47:39.26 +25:46:26.7
10:47:38.76 +24:47:53.2
10:46:33.65 +25:28:22.9
10:47:15.21 +25:49:00.9
10:46:51.44 +25:45:32.2
10:48:26.39 +25:54:24.2
10:46:58.39 +24:36:52.9
10:49:28.38 +25:45:17.5
10:46:44.32 +25:24:34.3
10:45:57.88 +25:17:15.8
10:51:14.22 +25:33:44.1
10:46:32.10 +25:47:54.8
10:48:23.26 +24:23:28.5
10:49:41.38 +25:25:06.7
10:46:00.17 +24:42:22.3
10:45:49.85 +23:50:06.6
10:49:08.43 +24:24:30.1
10:51:55.87 +25:30:06.7
10:49:16.13 +25:57:43.4
10:47:14.99 +25:53:40.5
10:51:37.82 +25:34:04.9
10:47:40.54 +26:05:40.3
10:47:29.18 +24:06:49.3
10:46:03.85 +24:24:34.8
10:46:46.19 +24:29:03.2
10:48:41.57 +24:58:47.9
10:47:19.18 +24:39:27.3
10:47:20.74 +23:55:45.8
10:47:11.27 +25:44:03.2
10:45:56.50 +25:26:17.6
10:48:22.28 +25:52:07.6
10:47:11.83 +26:03:16.0
10:46:10.67 +25:18:41.0
10:46:14.10 +24:52:20.5
10:46:05.65 +25:36:47.1
10:48:28.43 +23:34:31.2
10:48:33.01 +26:05:26.5
10:46:24.47 +26:06:30.5
10:46:56.79 +25:16:02.3
10:50:36.65 +24:59:45.4
10:47:22.16 +25:38:05.0
10:47:43.84 +25:59:38.2
10:51:13.67 +25:52:09.6
10:47:17.49 +23:54:19.2
10:47:13.55 +25:55:57.1
10:46:35.76 +26:00:07.4
10:45:50.01 +23:55:44.9
10:46:44.93 +24:15:33.0
10:49:49.83 +25:37:18.3
10:47:28.15 +26:03:31.0
10:47:37.79 +25:39:55.1
10:46:13.21 +24:21:03.9
10:48:00.94 +23:15:34.2
10:48:23.67 +25:30:28.7
###################################################################################
10:59:26.75 +22:03:53.4 -- asteroid (will NOT add it to exclusion list)
10:46:01.30 +23:36:54.5 -- not an asteroid (will add it to exclusion list)
10:49:04.00 +24:49:43.5 -- not an asteroid (will add it to exclusion list)
10:51:06.49 +25:33:53.1 -- not an asteroid (will add it to exclusion list)
10:49:29.16 +25:16:57.2 -- not an asteroid (will add it to exclusion list)
10:49:59.26 +25:53:24.5 -- not an asteroid (will add it to exclusion list)
10:47:34.32 +25:42:25.0 -- not an asteroid (will add it to exclusion list)
10:46:31.17 +25:32:47.7 -- not an asteroid (will add it to exclusion list)
10:47:42.71 +25:33:40.3 -- not an asteroid (will add it to exclusion list)
10:49:53.30 +25:43:51.8 -- not an asteroid (will add it to exclusion list)
10:47:54.96 +24:47:51.5 -- not an asteroid (will add it to exclusion list)
10:48:17.60 +25:54:37.4 -- not an asteroid (will add it to exclusion list)
10:46:08.58 +26:06:30.5 -- not an asteroid (will add it to exclusion list)
10:45:51.92 +25:03:31.9 -- not an asteroid (will add it to exclusion list)
10:49:09.23 +25:50:48.3 -- not an asteroid (will add it to exclusion list)
10:46:39.17 +25:32:40.5 -- not an asteroid (will add it to exclusion list)
10:49:51.08 +25:40:38.5 -- not an asteroid (will add it to exclusion list)
10:47:15.31 +25:22:31.4 -- not an asteroid (will add it to exclusion list)
10:49:22.18 +25:57:22.3 -- not an asteroid (will add it to exclusion list)
10:48:09.20 +25:45:24.9 -- not an asteroid (will add it to exclusion list)
10:46:38.65 +25:03:06.4 -- not an asteroid (will add it to exclusion list)
10:49:45.71 +25:50:01.6 -- not an asteroid (will add it to exclusion list)
10:46:41.68 +25:46:50.2 -- not an asteroid (will add it to exclusion list)
10:53:14.40 +25:42:53.0 -- not an asteroid (will add it to exclusion list)
10:46:52.77 +23:30:19.2 -- not an asteroid (will add it to exclusion list)
10:46:27.31 +25:02:43.7 -- not an asteroid (will add it to exclusion list)
10:48:11.02 +25:01:50.9 -- not an asteroid (will add it to exclusion list)
10:45:47.79 +23:37:02.8 -- not an asteroid (will add it to exclusion list)
10:46:36.02 +25:44:58.8 -- not an asteroid (will add it to exclusion list)
10:47:24.01 +25:39:21.5 -- not an asteroid (will add it to exclusion list)
10:46:37.58 +25:22:43.0 -- not an asteroid (will add it to exclusion list)
10:47:34.39 +24:54:06.9 -- not an asteroid (will add it to exclusion list)
10:47:47.86 +25:04:25.7 -- not an asteroid (will add it to exclusion list)
10:48:30.45 +25:23:39.6 -- not an asteroid (will add it to exclusion list)
10:49:16.08 +25:48:00.6 -- not an asteroid (will add it to exclusion list)
10:45:53.78 +23:20:27.5 -- not an asteroid (will add it to exclusion list)
10:46:35.42 +26:07:09.5 -- not an asteroid (will add it to exclusion list)
10:47:39.26 +25:46:26.7 -- not an asteroid (will add it to exclusion list)
10:47:38.76 +24:47:53.2 -- not an asteroid (will add it to exclusion list)
10:46:33.65 +25:28:22.9 -- not an asteroid (will add it to exclusion list)
10:47:15.21 +25:49:00.9 -- not an asteroid (will add it to exclusion list)
10:46:51.44 +25:45:32.2 -- not an asteroid (will add it to exclusion list)
10:48:26.39 +25:54:24.2 -- not an asteroid (will add it to exclusion list)
10:46:58.39 +24:36:52.9 -- not an asteroid (will add it to exclusion list)
10:49:28.38 +25:45:17.5 -- not an asteroid (will add it to exclusion list)
10:46:44.32 +25:24:34.3 -- not an asteroid (will add it to exclusion list)
10:45:57.88 +25:17:15.8 -- not an asteroid (will add it to exclusion list)
10:51:14.22 +25:33:44.1 -- not an asteroid (will add it to exclusion list)
10:46:32.10 +25:47:54.8 -- not an asteroid (will add it to exclusion list)
10:48:23.26 +24:23:28.5 -- not an asteroid (will add it to exclusion list)
10:49:41.38 +25:25:06.7 -- not an asteroid (will add it to exclusion list)
10:46:00.17 +24:42:22.3 -- not an asteroid (will add it to exclusion list)
10:45:49.85 +23:50:06.6 -- not an asteroid (will add it to exclusion list)
10:49:08.43 +24:24:30.1 -- not an asteroid (will add it to exclusion list)
10:51:55.87 +25:30:06.7 -- not an asteroid (will add it to exclusion list)
10:49:16.13 +25:57:43.4 -- not an asteroid (will add it to exclusion list)
10:47:14.99 +25:53:40.5 -- not an asteroid (will add it to exclusion list)
10:51:37.82 +25:34:04.9 -- not an asteroid (will add it to exclusion list)
10:47:40.54 +26:05:40.3 -- not an asteroid (will add it to exclusion list)
10:47:29.18 +24:06:49.3 -- not an asteroid (will add it to exclusion list)
10:46:03.85 +24:24:34.8 -- not an asteroid (will add it to exclusion list)
10:46:46.19 +24:29:03.2 -- not an asteroid (will add it to exclusion list)
10:48:41.57 +24:58:47.9 -- not an asteroid (will add it to exclusion list)
10:47:19.18 +24:39:27.3 -- not an asteroid (will add it to exclusion list)
10:47:20.74 +23:55:45.8 -- not an asteroid (will add it to exclusion list)
10:47:11.27 +25:44:03.2 -- not an asteroid (will add it to exclusion list)
10:45:56.50 +25:26:17.6 -- not an asteroid (will add it to exclusion list)
10:48:22.28 +25:52:07.6 -- not an asteroid (will add it to exclusion list)
10:47:11.83 +26:03:16.0 -- not an asteroid (will add it to exclusion list)
10:46:10.67 +25:18:41.0 -- not an asteroid (will add it to exclusion list)
10:46:14.10 +24:52:20.5 -- not an asteroid (will add it to exclusion list)
10:46:05.65 +25:36:47.1 -- not an asteroid (will add it to exclusion list)
10:48:28.43 +23:34:31.2 -- not an asteroid (will add it to exclusion list)
10:48:33.01 +26:05:26.5 -- not an asteroid (will add it to exclusion list)
10:46:24.47 +26:06:30.5 -- not an asteroid (will add it to exclusion list)
10:46:56.79 +25:16:02.3 -- not an asteroid (will add it to exclusion list)
10:50:36.65 +24:59:45.4 -- not an asteroid (will add it to exclusion list)
10:47:22.16 +25:38:05.0 -- not an asteroid (will add it to exclusion list)
10:47:43.84 +25:59:38.2 -- not an asteroid (will add it to exclusion list)
10:51:13.67 +25:52:09.6 -- not an asteroid (will add it to exclusion list)
10:47:17.49 +23:54:19.2 -- not an asteroid (will add it to exclusion list)
10:47:13.55 +25:55:57.1 -- not an asteroid (will add it to exclusion list)
10:46:35.76 +26:00:07.4 -- not an asteroid (will add it to exclusion list)
10:45:50.01 +23:55:44.9 -- not an asteroid (will add it to exclusion list)
10:46:44.93 +24:15:33.0 -- not an asteroid (will add it to exclusion list)
10:49:49.83 +25:37:18.3 -- not an asteroid (will add it to exclusion list)
10:47:28.15 +26:03:31.0 -- not an asteroid (will add it to exclusion list)
10:47:37.79 +25:39:55.1 -- not an asteroid (will add it to exclusion list)
10:46:13.21 +24:21:03.9 -- not an asteroid (will add it to exclusion list)
10:48:00.94 +23:15:34.2 -- not an asteroid (will add it to exclusion list)
10:48:23.67 +25:30:28.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
10:45:47.79 +23:37:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:49.85 +23:50:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:50.01 +23:55:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:51.92 +25:03:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:53.78 +23:20:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:56.50 +25:26:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:45:57.88 +25:17:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:00.17 +24:42:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:01.30 +23:36:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:03.85 +24:24:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:05.65 +25:36:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:08.58 +26:06:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:10.67 +25:18:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:13.21 +24:21:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:14.10 +24:52:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:24.47 +26:06:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:27.31 +25:02:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:31.17 +25:32:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:32.10 +25:47:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:33.65 +25:28:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:35.42 +26:07:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:35.76 +26:00:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:36.02 +25:44:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:37.58 +25:22:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:38.65 +25:03:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:39.17 +25:32:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:41.68 +25:46:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:44.32 +25:24:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:44.93 +24:15:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:46.19 +24:29:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:51.44 +25:45:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:52.77 +23:30:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:56.79 +25:16:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:46:58.39 +24:36:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:11.27 +25:44:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:11.83 +26:03:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:13.55 +25:55:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:14.99 +25:53:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:15.21 +25:49:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:15.31 +25:22:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:17.49 +23:54:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:19.18 +24:39:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:20.74 +23:55:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:22.16 +25:38:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:24.01 +25:39:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:28.15 +26:03:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:29.18 +24:06:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:34.32 +25:42:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:34.39 +24:54:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:37.79 +25:39:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:38.76 +24:47:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:39.26 +25:46:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:40.54 +26:05:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:42.71 +25:33:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:43.84 +25:59:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:47.86 +25:04:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:54.96 +24:47:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:00.94 +23:15:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:09.20 +25:45:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:11.02 +25:01:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:17.60 +25:54:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:22.28 +25:52:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:23.26 +24:23:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:23.67 +25:30:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:26.39 +25:54:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:28.43 +23:34:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:30.45 +25:23:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:33.01 +26:05:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:48:41.57 +24:58:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:04.00 +24:49:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:08.43 +24:24:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:09.23 +25:50:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:16.08 +25:48:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:16.13 +25:57:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:22.18 +25:57:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:28.38 +25:45:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:29.16 +25:16:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:41.38 +25:25:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:45.71 +25:50:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:49.83 +25:37:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:51.08 +25:40:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:53.30 +25:43:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:49:59.26 +25:53:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:50:36.65 +24:59:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:51:06.49 +25:33:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:51:13.67 +25:52:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:51:14.22 +25:33:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:51:37.82 +25:34:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:51:55.87 +25:30:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:53:14.40 +25:42:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
10:45:47.79 +23:37:02.8 -- not a known variable star
10:45:49.85 +23:50:06.6 -- a known variable star
10:45:50.01 +23:55:44.9 -- not a known variable star
10:45:51.92 +25:03:31.9 -- not a known variable star
10:45:53.78 +23:20:27.5 -- not a known variable star
10:45:56.50 +25:26:17.6 -- not a known variable star
10:45:57.88 +25:17:15.8 -- not a known variable star
10:46:00.17 +24:42:22.3 -- not a known variable star
10:46:01.30 +23:36:54.5 -- not a known variable star
10:46:03.85 +24:24:34.8 -- not a known variable star
10:46:05.65 +25:36:47.1 -- not a known variable star
10:46:08.58 +26:06:30.5 -- not a known variable star
10:46:10.67 +25:18:41.0 -- a known variable star
10:46:13.21 +24:21:03.9 -- not a known variable star
10:46:14.10 +24:52:20.5 -- not a known variable star
10:46:24.47 +26:06:30.5 -- not a known variable star
10:46:27.31 +25:02:43.7 -- not a known variable star
10:46:31.17 +25:32:47.7 -- not a known variable star
10:46:32.10 +25:47:54.8 -- not a known variable star
10:46:33.65 +25:28:22.9 -- not a known variable star
10:46:35.42 +26:07:09.5 -- not a known variable star
10:46:35.76 +26:00:07.4 -- not a known variable star
10:46:36.02 +25:44:58.8 -- not a known variable star
10:46:37.58 +25:22:43.0 -- not a known variable star
10:46:38.65 +25:03:06.4 -- a known variable star
10:46:39.17 +25:32:40.5 -- not a known variable star
10:46:41.68 +25:46:50.2 -- not a known variable star
10:46:44.32 +25:24:34.3 -- not a known variable star
10:46:44.93 +24:15:33.0 -- not a known variable star
10:46:46.19 +24:29:03.2 -- not a known variable star
10:46:51.44 +25:45:32.2 -- not a known variable star
10:46:52.77 +23:30:19.2 -- not a known variable star
10:46:56.79 +25:16:02.3 -- not a known variable star
10:46:58.39 +24:36:52.9 -- not a known variable star
10:47:11.27 +25:44:03.2 -- not a known variable star
10:47:11.83 +26:03:16.0 -- not a known variable star
10:47:13.55 +25:55:57.1 -- not a known variable star
10:47:14.99 +25:53:40.5 -- not a known variable star
10:47:15.21 +25:49:00.9 -- not a known variable star
10:47:15.31 +25:22:31.4 -- not a known variable star
10:47:17.49 +23:54:19.2 -- not a known variable star
10:47:19.18 +24:39:27.3 -- a known variable star
10:47:20.74 +23:55:45.8 -- not a known variable star
10:47:22.16 +25:38:05.0 -- not a known variable star
10:47:24.01 +25:39:21.5 -- not a known variable star
10:47:28.15 +26:03:31.0 -- not a known variable star
10:47:29.18 +24:06:49.3 -- not a known variable star
10:47:34.32 +25:42:25.0 -- not a known variable star
10:47:34.39 +24:54:06.9 -- not a known variable star
10:47:37.79 +25:39:55.1 -- not a known variable star
10:47:38.76 +24:47:53.2 -- a known variable star
10:47:39.26 +25:46:26.7 -- not a known variable star
10:47:40.54 +26:05:40.3 -- not a known variable star
10:47:42.71 +25:33:40.3 -- not a known variable star
10:47:43.84 +25:59:38.2 -- not a known variable star
10:47:47.86 +25:04:25.7 -- not a known variable star
10:47:54.96 +24:47:51.5 -- not a known variable star
10:48:00.94 +23:15:34.2 -- not a known variable star
10:48:09.20 +25:45:24.9 -- not a known variable star
10:48:11.02 +25:01:50.9 -- a known variable star
10:48:17.60 +25:54:37.4 -- not a known variable star
10:48:22.28 +25:52:07.6 -- not a known variable star
10:48:23.26 +24:23:28.5 -- not a known variable star
10:48:23.67 +25:30:28.7 -- not a known variable star
10:48:26.39 +25:54:24.2 -- not a known variable star
10:48:28.43 +23:34:31.2 -- not a known variable star
10:48:30.45 +25:23:39.6 -- not a known variable star
10:48:33.01 +26:05:26.5 -- not a known variable star
10:48:41.57 +24:58:47.9 -- a known variable star
10:49:04.00 +24:49:43.5 -- not a known variable star
10:49:08.43 +24:24:30.1 -- not a known variable star
10:49:09.23 +25:50:48.3 -- not a known variable star
10:49:16.08 +25:48:00.6 -- not a known variable star
10:49:16.13 +25:57:43.4 -- not a known variable star
10:49:22.18 +25:57:22.3 -- not a known variable star
10:49:28.38 +25:45:17.5 -- not a known variable star
10:49:29.16 +25:16:57.2 -- not a known variable star
10:49:41.38 +25:25:06.7 -- not a known variable star
10:49:45.71 +25:50:01.6 -- not a known variable star
10:49:49.83 +25:37:18.3 -- not a known variable star
10:49:51.08 +25:40:38.5 -- not a known variable star
10:49:53.30 +25:43:51.8 -- not a known variable star
10:49:59.26 +25:53:24.5 -- not a known variable star
10:50:36.65 +24:59:45.4 -- not a known variable star
10:51:06.49 +25:33:53.1 -- not a known variable star
10:51:13.67 +25:52:09.6 -- a known variable star
10:51:14.22 +25:33:44.1 -- not a known variable star
10:51:37.82 +25:34:04.9 -- a known variable star
10:51:55.87 +25:30:06.7 -- not a known variable star
10:53:14.40 +25:42:53.0 -- not a known variable star
Found 81 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
90 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 90 (excluding asteroids and hot pixels, 81 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)2461206.67134097 -observatory V36
07:19:32.01 +23:18:07.5 Mercury (0.5mag)
08:17:26.42 +21:46:30.5 Venus (-4.0mag)
03:09:56.93 +17:13:16.6 Mars (1.3mag)
07:54:20.11 +21:16:14.8 Jupiter (-1.8mag)
00:51:14.76 +02:58:43.0 Saturn (0.8mag)
04:01:50.83 +20:30:08.9 Uranus (5.8mag)
00:16:30.35 +00:18:46.5 Neptune (7.8mag)
20:32:56.05 -23:07:15.1 Pluto (14.5mag)
05:32:17.81 +27:11:32.2 Moon (99.9mag)
-rw-r--r-- 1 apache apache 361 Jun 14 23:39 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461206.67134097:
07:54:18.85 +21:16:20.7 Io (6.2mag)
07:54:18.03 +21:16:23.4 Europa (6.3mag)
07:54:05.06 +21:17:01.1 Ganymede (5.6mag)
07:53:54.57 +21:17:36.5 Callisto (6.9mag)
07:54:12.48 +20:53:17.4 Himalia (15.6mag)
07:54:19.67 +21:16:16.4 Thebe (16.5mag)
07:54:00.33 +21:05:45.5 Elara (17.6mag)
07:56:51.70 +21:24:07.8 Pasiphae (17.8mag)
08:00:36.24 +21:18:30.8 Carme (18.9mag)
00:51:26.78 +02:58:40.8 Titan (8.6mag)
00:51:19.69 +02:58:36.3 Rhea (9.9mag)
00:51:39.22 +03:01:15.6 Iapetus (11.3mag)
00:51:30.14 +02:58:32.1 Hyperion (14.6mag)
00:51:48.36 +02:59:38.8 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 14 23:39 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461206.67134097:
17:28:23.58 -35:36:06.7 JWST
18:56:27.63 +19:31:34.2 Chandra
08:25:15.81 -46:00:42.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 14 23:39 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461206.67134097 -observatory V36
18:38:25.03 -33:08:27.4 13.6mag P/2010 H2 (Vales)
06:00:23.07 -68:00:35.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:51:38.39 +32:03:41.6 17.5mag C/2017 K2 (PANSTARRS)
17:11:56.83 +15:39:29.6 17.8mag C/2021 G2 (ATLAS)
22:20:31.79 -43:49:35.8 16.3mag P/2021 N1 (ZTF)
23:10:49.28 +31:50:23.8 17.2mag C/2022 E2 (ATLAS)
05:42:34.07 +27:00:18.8 16.5mag C/2022 N2 (PANSTARRS)
09:34:53.17 +30:49:45.1 16.7mag C/2022 QE78 (ATLAS)
08:54:23.46 +04:14:36.2 17.7mag C/2022 R6 (PANSTARRS)
18:23:37.43 +21:41:35.6 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:17:00.78 -11:02:00.4 17.6mag P/2023 B1 (PANSTARRS)
22:11:26.79 +66:55:41.4 17.8mag C/2023 H5 (Lemmon)
17:29:01.46 -07:23:33.2 13.7mag C/2023 R1 (PANSTARRS)
13:16:36.79 +81:22:31.4 18.0mag C/2023 X2 (Lemmon)
07:20:22.36 +64:33:29.7 17.7mag C/2024 A1 (ATLAS)
06:57:42.89 +28:25:11.0 13.9mag C/2024 E1 (Wierzchos)
15:31:58.22 +14:05:18.8 17.4mag C/2024 G6 (ATLAS)
20:07:55.28 +33:10:25.7 13.9mag C/2024 J3 (ATLAS)
04:25:00.84 -15:22:08.5 16.0mag C/2024 T5 (ATLAS)
06:12:22.96 +33:17:23.0 17.9mag C/2025 J1 (Borisov)
11:32:34.53 +52:19:51.5 17.7mag C/2025 L1 (ATLAS)
06:52:49.83 -11:11:57.9 14.7mag C/2025 R3 (PANSTARRS)
09:30:08.73 +23:13:31.8 17.9mag C/2025 V2 (Rankin)
12:39:47.56 +04:38:12.2 17.1mag C/2025 Y1 (ATLAS)
18:00:07.58 +76:31:28.4 17.8mag C/2026 A2 (Bok)
02:12:21.14 +43:53:20.7 16.2mag C/2026 B2 (Sun-Gao)
11:13:09.03 -01:26:06.0 16.6mag A/2026 E1
20:36:13.88 -09:13:39.4 8.4mag 10P/Tempel
11:03:50.01 -01:05:20.9 16.0mag 29P/Schwassmann-Wachmann
03:22:29.03 +26:33:42.1 17.7mag 47P/Ashbrook-Jackson
09:14:51.56 +21:44:50.0 16.9mag 63P/Wild
00:32:40.25 -05:57:08.0 15.6mag 65P/Gunn
07:06:06.79 +34:00:54.9 17.1mag 76P/West-Kohoutek-Ikemura
03:26:05.71 +18:03:31.7 13.8mag 78P/Gehrels
01:35:33.58 +06:18:43.4 15.7mag 88P/Howell
05:17:04.55 +30:43:26.6 15.3mag 93P/Lovas
03:03:02.10 +28:40:55.7 17.4mag 114P/Wiseman-Skiff
07:07:17.33 +32:43:58.0 15.5mag 123P/West-Hartley
10:02:24.85 +11:39:47.0 16.6mag 124P/Mrkos
04:10:33.16 +19:41:27.6 16.3mag 128P/Shoemaker-Holt
04:47:24.50 +19:21:56.6 17.8mag 131P/Mueller
06:27:15.27 +17:44:57.8 15.5mag 141P/Machholz
06:30:21.11 +17:53:34.6 15.5mag 141P-A/Machholz
05:28:29.74 +16:56:55.4 12.4mag 141P-D/Machholz
03:02:29.45 -23:46:15.5 16.6mag 161P/Hartley-IRAS
04:04:47.00 +26:29:39.9 15.0mag 162P/SidingSpring
19:35:08.25 +03:54:37.1 16.5mag 169P/NEAT
00:37:00.22 +03:47:24.4 17.8mag 220P/McNaught
16:47:04.98 -08:12:20.5 16.5mag 235P/LINEAR
07:50:21.84 +35:09:30.2 17.6mag 240P/NEAT
00:50:45.67 +00:32:53.4 16.2mag 260P/McNaught
04:23:28.25 +33:41:22.0 17.5mag 295P/LINEAR
00:31:44.64 -01:36:09.9 17.8mag 320P/McNaught
15:12:19.67 +07:48:45.6 17.5mag 391P/Kowalski
08:12:47.76 +20:33:21.2 17.9mag 450P/LONEOS
07:11:20.72 +41:11:29.8 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 14 23:39 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.18 +22:02:03.40 AT2026lxf 2026-05-8.07 13.94
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:26:28.11 -72:31:19.50 2026-06-11 17.05
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:26:28.11 -72:31:19.50 2026-06-11 17.05
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.68 -22:39:32.70 ASASSN-26cm 2026-04-4.27 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
-rw-r--r-- 1 apache apache 5.6K Jun 14 23:39 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
-rw-r--r-- 1 apache apache 189K Jun 14 23:39 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:49:19.289 -10:17:13.45 AT 2026ome 2026-06-06.42 19.9
15:05:48.011 -29:45:37.21 AT 2026omd 2026-06-06.50 20.04
20:30:10.926 -29:56:07.53 AT 2026omc 2026-06-07.64 18.81
19:50:57.124 -53:24:23.12 AT 2026omb 2026-06-06.67 20.17
23:28:37.442 -43:16:54.75 AT 2026oma 2026-06-06.73 19.64
11:48:30.394 -39:49:36.11 AT 2026olz 2026-06-06.77 19.237
13:56:31.281 +70:50:34.89 AT 2026oly 2026-06-06.35 19.395
12:22:49.169 -21:19:33.91 AT 2026olx 2026-06-07.30 18.696
22:49:46.803 -26:24:12.60 SN 2026olw 2026-06-07.58 18.251
10:47:10.687 -70:44:55.20 AT 2026olv 2026-06-06.81 18.37
11:06:55.086 +37:19:50.72 AT 2026olu 2026-06-01.30 18.692
14:54:40.331 -10:41:24.18 SN 2026olt 2026-06-04.43 18.588
10:58:43.462 +36:47:26.62 AT 2026ols 2026-06-04.90 18.501
08:45:48.069 -64:46:34.13 AT 2026olr 2026-06-06.71 18.616
10:02:19.987 -84:42:35.43 AT 2026olq 2026-06-06.80 18.714
22:35:38.444 -55:59:06.00 SN 2026olp 2026-05-30.09 18.424
21:02:06.402 +85:28:22.07 AT 2026olo 2026-06-07.10 18.987
18:52:00.191 +72:19:28.04 AT 2026oln 2026-06-07.07 18.528
23:35:46.181 -42:09:54.16 AT 2026olm 2026-06-07.13 18.697
12:34:21.767 -10:29:46.08 AT 2026oll 2026-06-05.82 19.393
-rw-r--r-- 1 apache apache 30K Jun 14 23:39 tns_transients_list.txt
