This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb
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 08.1390 2461199.6390 12.31 09:21:18.01 +22:06:36.5
206.87630 42.31312 galactic Cnc Second-epoch detections are separated by 1.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:18.01 +22:06:36.5 (user input) | T | P | (position from user input) J-Ks=0.346+/-0.033 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:18.01 +22:06:36.5: 13.20 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:18.01 +22:06:36.5: 13.19 +/- 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,2461199.6390,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.34 09:25:08.90 +23:34:04.1
205.31048 43.57696 galactic Leo Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:25:08.90 +23:34:04.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.356+/-0.033 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:25:08.90 +23:34:04.1: 13.22 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:25:08.90 +23:34:04.1: 13.26 +/- 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!
TCP 2026 06 08.1390* 09 25 08.90 +23 34 04.1 12.3 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
target,2461199.6390,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 08.1390 2461199.6390 11.65 09:22:16.53 +22:50:27.0
206.01614 42.74073 galactic Leo Second-epoch detections are separated by 0.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 639059080304533376 | 09:22:16.55 +22:50:27.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.329+/-0.029 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:16.53 +22:50:27.0: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:16.53 +22:50:27.0: 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!
TCP 2026 06 08.1390* 09 22 16.53 +22 50 27.0 11.7 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
Gaia DR3 639059080304533376,2461199.6390,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 639059080304533376 20260608.1390 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 12.05 09:22:26.41 +22:52:05.1
205.99524 42.78485 galactic Leo Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J140.6080+22.8686 | 09:22:26.41 +22:52:05.1 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.287+/-0.031 (F)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:26.41 +22:52:05.1: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:26.41 +22:52:05.1: 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!
TCP 2026 06 08.1390* 09 22 26.41 +22 52 05.1 12.1 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
ATO J140.6080+22.8686,2461199.6390,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J140.6080+22.8686 20260608.1390 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 08.1390 2461199.6390 11.78 09:22:57.92 +22:59:15.7
205.88539 42.93467 galactic Leo Second-epoch detections are separated by 0.4" and 6.3 pix
The object was found in VSX 1" Gaia DR3 639067807678059520
Type: ROT
# Max. Min./Amp. JD0 Period
12.530 G 12.550 G G
The object was not found in astcheck.
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:57.92 +22:59:15.7: 12.74 +/- 0.01 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:57.92 +22:59:15.7: 12.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 22 57.92 +22 59 15.7 11.8 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
Gaia DR3 639067807678059520,2461199.6390,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 639067807678059520 20260608.1390 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 12.12 09:24:56.57 +23:55:05.5
204.82699 43.62592 galactic Leo Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:24:56.57 +23:55:05.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.605+/-0.026 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:24:56.57 +23:55:05.5: 13.06 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:24:56.57 +23:55:05.5: 13.09 +/- 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!
TCP 2026 06 08.1390* 09 24 56.57 +23 55 05.5 12.1 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
target,2461199.6390,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.15 09:21:58.36 +22:23:51.3
206.56588 42.54623 galactic Cnc Second-epoch detections are separated by 0.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:58.36 +22:23:51.3 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.031 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:58.36 +22:23:51.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:58.36 +22:23:51.3: 13.08 +/- 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,2461199.6390,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.08 09:21:57.81 +22:32:22.0
206.38071 42.58536 galactic Cnc Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:57.81 +22:32:22.0 (user input) | T | P | (position from user input) J-Ks=0.549+/-0.027 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:57.81 +22:32:22.0: 13.04 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:57.81 +22:32:22.0: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 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,2461199.6390,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 11.99 09:22:35.73 +23:24:59.2
205.29045 42.97257 galactic Leo Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:22:35.73 +23:24:59.2 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.493+/-0.030 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:35.73 +23:24:59.2: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:35.73 +23:24:59.2: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 22 35.73 +23 24 59.2 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
target,2461199.6390,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.02 09:24:14.14 +23:37:38.6
205.15321 43.39190 galactic Leo Second-epoch detections are separated by 0.9" and 6.4 pix
The object was found in VSX10" Gaia DR3 639216993367008128
Type: ROT
# Max. Min./Amp. JD0 Period
12.290 G 12.320 G M
The object was not found in astcheck.
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:24:14.14 +23:37:38.6: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:24:14.14 +23:37:38.6: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 24 14.14 +23 37 38.6 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
Gaia DR3 639216993367008128,2461199.6390,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 639216993367008128 20260608.1390 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 08.1390 2461199.6390 12.07 09:23:15.59 +23:05:38.9
205.77177 43.02960 galactic Leo Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:23:15.59 +23:05:38.9 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.354+/-0.030 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:15.59 +23:05:38.9: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:15.59 +23:05:38.9: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 23 15.59 +23 05 38.9 12.1 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
target,2461199.6390,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 08.1390 2461199.6390 12.06 09:26:10.86 +23:59:23.3
204.83533 43.91767 galactic Leo Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:26:10.86 +23:59:23.3 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.288+/-0.028 (F)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:26:10.86 +23:59:23.3: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:26:10.86 +23:59:23.3: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 26 10.86 +23 59 23.3 12.1 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
target,2461199.6390,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.52 09:23:32.57 +23:08:57.3
205.72424 43.10748 galactic Leo Second-epoch detections are separated by 1.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:23:32.57 +23:08:57.3 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.033 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:32.57 +23:08:57.3: 13.55 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:32.57 +23:08:57.3: 13.66 +/- 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!
TCP 2026 06 08.1390* 09 23 32.57 +23 08 57.3 12.5 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
target,2461199.6390,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 12.52CV 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 08.1390 2461199.6390 12.38 09:23:04.02 +23:41:41.1
204.96447 43.15260 galactic Leo Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:23:04.02 +23:41:41.1 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.486+/-0.032 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:04.02 +23:41:41.1: 13.34 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:04.02 +23:41:41.1: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 23 04.02 +23 41 41.1 12.4 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
target,2461199.6390,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.48 09:25:32.87 +23:41:50.8
205.17223 43.70012 galactic Leo Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:25:32.87 +23:41:50.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.586+/-0.031 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:25:32.87 +23:41:50.8: 13.51 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:25:32.87 +23:41:50.8: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 25 32.87 +23 41 50.8 12.5 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
target,2461199.6390,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 12.32 09:23:56.82 +23:22:18.5
205.46629 43.25837 galactic Leo Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:23:56.82 +23:22:18.5 (user input) | T | P | (position from user input) J-Ks=0.313+/-0.033 (F)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:56.82 +23:22:18.5: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:56.82 +23:22:18.5: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 23 56.82 +23 22 18.5 12.3 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
target,2461199.6390,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.32 09:27:10.04 +24:30:49.5
204.21220 44.27092 galactic Leo Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:27:10.04 +24:30:49.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.668+/-0.033 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:27:10.04 +24:30:49.5: 13.29 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:27:10.04 +24:30:49.5: 13.25 +/- 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!
TCP 2026 06 08.1390* 09 27 10.04 +24 30 49.5 12.3 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
target,2461199.6390,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.18 09:21:57.30 +22:25:02.5
206.53858 42.54808 galactic Cnc Second-epoch detections are separated by 0.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:57.30 +22:25:02.5 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.030 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:57.30 +22:25:02.5: 13.29 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:57.30 +22:25:02.5: 13.23 +/- 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,2461199.6390,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.32 09:27:56.39 +24:58:52.5
203.64041 44.55815 galactic Leo Second-epoch detections are separated by 1.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:27:56.39 +24:58:52.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.499+/-0.028 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:27:56.39 +24:58:52.5: 13.27 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:27:56.39 +24:58:52.5: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 27 56.39 +24 58 52.5 12.3 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
target,2461199.6390,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 11.91 09:22:02.31 +22:39:26.8
206.23396 42.63594 galactic Cnc Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:22:02.31 +22:39:26.8 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.028 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:02.31 +22:39:26.8: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:02.31 +22:39:26.8: 12.91 +/- 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
target,2461199.6390,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 11.94 08:59:41.69 +22:13:38.2
204.76478 37.57859 galactic Cnc Second-epoch detections are separated by 2.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:59:41.69 +22:13:38.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.498+/-0.031 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:59:41.69 +22:13:38.2: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:59:41.69 +22:13:38.2: 12.87 +/- 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
target,2461199.6390,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 11.99 09:24:36.41 +24:09:57.0
204.46906 43.61747 galactic Leo Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:24:36.41 +24:09:57.0 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.602+/-0.030 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:24:36.41 +24:09:57.0: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:24:36.41 +24:09:57.0: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 24 36.41 +24 09 57.0 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
target,2461199.6390,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 11.56 09:21:52.52 +22:38:34.5
206.23816 42.59571 galactic Cnc Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 639029251756023040 | 09:21:52.53 +22:38:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.592+/-0.028 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:52.52 +22:38:34.5: 12.52 +/- 0.01 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:52.52 +22:38:34.5: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 639029251756023040,2461199.6390,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 639029251756023040 20260608.1390 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 12.39 09:23:22.11 +23:14:51.2
205.57965 43.09637 galactic Leo Second-epoch detections are separated by 1.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:23:22.11 +23:14:51.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.556+/-0.030 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:22.11 +23:14:51.2: 13.79 +/- 0.04 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:22.11 +23:14:51.2: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 23 22.11 +23 14 51.2 12.4 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
target,2461199.6390,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 12.48 09:22:27.60 +23:09:52.8
205.60897 42.87279 galactic Leo Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:22:27.60 +23:09:52.8 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.348+/-0.031 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:27.60 +23:09:52.8: 13.59 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:27.60 +23:09:52.8: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 22 27.60 +23 09 52.8 12.5 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
target,2461199.6390,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 12.18 09:22:28.57 +22:42:23.3
206.20946 42.74672 galactic Leo Second-epoch detections are separated by 1.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:22:28.57 +22:42:23.3 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.346+/-0.029 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:28.57 +22:42:23.3: 13.18 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:28.57 +22:42:23.3: 13.20 +/- 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!
TCP 2026 06 08.1390* 09 22 28.57 +22 42 23.3 12.2 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
target,2461199.6390,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.33 09:23:10.43 +23:17:42.6
205.50004 43.06662 galactic Leo Second-epoch detections are separated by 1.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J140.7937+23.2950 | 09:23:10.43 +23:17:42.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.297+/-0.031 (F)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:10.43 +23:17:42.6: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:10.43 +23:17:42.6: 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!
TCP 2026 06 08.1390* 09 23 10.43 +23 17 42.6 12.3 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
ATO J140.7937+23.2950,2461199.6390,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J140.7937+23.2950 20260608.1390 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 12.16 09:22:47.48 +23:13:19.9
205.56254 42.96195 galactic Leo Second-epoch detections are separated by 0.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:22:47.48 +23:13:19.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.272+/-0.030 (F)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:47.48 +23:13:19.9: 13.16 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:47.48 +23:13:19.9: 13.12 +/- 0.02 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!
TCP 2026 06 08.1390* 09 22 47.48 +23 13 19.9 12.2 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
target,2461199.6390,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.12 09:22:41.43 +23:07:49.9
205.67394 42.91411 galactic Leo Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:22:41.43 +23:07:49.9 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.359+/-0.031 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:41.43 +23:07:49.9: 13.16 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:41.43 +23:07:49.9: 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!
TCP 2026 06 08.1390* 09 22 41.43 +23 07 49.9 12.1 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
target,2461199.6390,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.18 09:18:29.84 +21:07:01.5
207.88120 41.39101 galactic Cnc Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:18:29.84 +21:07:01.5 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.029 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:18:29.84 +21:07:01.5: 13.14 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:18:29.84 +21:07:01.5: 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
target,2461199.6390,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.39 09:21:32.83 +22:17:58.4
206.65405 42.42350 galactic Cnc Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:32.83 +22:17:58.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.396+/-0.027 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:32.83 +22:17:58.4: 13.37 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:32.83 +22:17:58.4: 13.35 +/- 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,2461199.6390,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 12.41 09:26:14.91 +24:16:27.1
204.45965 44.00707 galactic Leo Second-epoch detections are separated by 0.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:26:14.91 +24:16:27.1 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.274+/-0.030 (F)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:26:14.91 +24:16:27.1: 13.37 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:26:14.91 +24:16:27.1: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 08.1390* 09 26 14.91 +24 16 27.1 12.4 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
target,2461199.6390,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 12.15 09:24:05.13 +23:28:38.9
205.33869 43.31793 galactic Leo Second-epoch detections are separated by 2.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:24:05.13 +23:28:38.9 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.608+/-0.028 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:24:05.13 +23:28:38.9: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:24:05.13 +23:28:38.9: 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!
TCP 2026 06 08.1390* 09 24 05.13 +23 28 38.9 12.2 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
target,2461199.6390,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.27 09:22:04.90 +22:26:16.5
206.52343 42.58206 galactic Cnc Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:22:04.90 +22:26:16.5 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.030 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:04.90 +22:26:16.5: 13.37 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:04.90 +22:26:16.5: 13.35 +/- 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,2461199.6390,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1390 2461199.6390 12.10 09:22:05.42 +23:09:58.0
205.57468 42.79162 galactic Cnc Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:22:05.42 +23:09:58.0 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.028 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:05.42 +23:09:58.0: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:05.42 +23:09:58.0: 13.13 +/- 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
target,2461199.6390,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.06 09:23:03.68 +23:25:55.3
205.31021 43.07959 galactic Leo Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:23:03.68 +23:25:55.3 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.648+/-0.028 (K)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:03.68 +23:25:55.3: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:03.68 +23:25:55.3: 13.05 +/- 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!
TCP 2026 06 08.1390* 09 23 03.68 +23 25 55.3 12.1 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
target,2461199.6390,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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 08.1390 2461199.6390 12.13 09:18:18.33 +20:49:35.9
208.22981 41.25751 galactic Cnc Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:18:18.33 +20:49:35.9 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.353+/-0.031 (G)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:18:18.33 +20:49:35.9: 13.09 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:18:18.33 +20:49:35.9: 13.11 +/- 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,2461199.6390,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1390 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
First image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Last image: 2461199.63930743 08.06.2026 03:20:26.162 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 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): 8554
Objects passed selection criteria: 8486
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 4958.25
Average stars matched: 4825.25 (97.3176 %)
Memory usage VmPeak: 114352 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 7 22:48:34 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: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
First image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Last image: 2461199.63930743 08.06.2026 03:20:26.162 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 41
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 10 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): 46899
Objects passed selection criteria: 46710
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: 29103
Average stars matched: 28080.2 (96.4858 %)
Memory usage VmPeak: 148488 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 7 22:50:25 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.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: 2461199.63879346
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits exists and is non-empty
Saving wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits'
wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits exists and is non-empty
Saving wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits'
wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits'
wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (1st reference image)
verification OK: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:50.749 +22:00:00.30 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_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits (1st new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
Image size: 941.5'x626.6' 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: 09:14:01.839 +22:00:17.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:13:50.749 +22:00:00.30
Second-epoch image center 09:14:01.839 +22:00:17.41
Angular distance between the image centers 0.0431 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits (2nd new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
Image size: 941.5'x626.6' 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: 09:14:00.269 +22:00:48.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:13:50.749 +22:00:00.30
Second-epoch image center 09:14:00.269 +22:00:48.79
Angular distance between the image centers 0.0392 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 09:14:01.839 +22:00:17.41
Second-epoch second image center 09:14:00.269 +22:00:48.79
Angular distance between the image centers 0.01062 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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits &> /tmp/tmp.5DphiZoLWV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits &> /tmp/tmp.q5nKdAimIz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits &> /tmp/tmp.h5Mg6hdjMw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits &> /tmp/tmp.zpI6TbifV2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat
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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat
The reference image (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits) and catalog (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat) found
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat' -> 'wcsmag.cat'
Read 9058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4948 to 147.0574 deg, Dec +16.3332 to +27.3468 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 129.4948 to 147.0574 deg, Dec 16.3332 to 27.3468 deg
Loaded 6004 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): 4516 out of 4805 total matches.
Matched with Tycho-2 4805 out of 9058 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.920350
a=0.000000 b=1.000000 c=22.920350
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4948 to 147.0574 deg, Dec +16.3332 to +27.3468 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 129.4948 to 147.0574 deg, Dec 16.3332 to 27.3468 deg
Loaded 6004 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): 4516 out of 4805 total matches.
Matched with Tycho-2 4805 out of 9058 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits:
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (aperture=6.3)
Read 9037 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4948 to 147.0612 deg, Dec +16.3333 to +27.3527 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 129.4948 to 147.0612 deg, Dec 16.3333 to 27.3527 deg
Loaded 6007 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): 4487 out of 4795 total matches.
Matched with Tycho-2 4795 out of 9037 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits:
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.2 pix Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
2.1 pix fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
2.0 pix fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
2.2 pix wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.2 pix wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Limiting magnitude estimates:
15.4 mag. Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
15.4 mag. Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
12.4 mag. fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
12.2 mag. fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 9.9 (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.5DphiZoLWV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=691, passed=9058
Got 9058 stars (including 8360 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat
util/solve_plate_with_UCAC5 got 9058 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits N_match=957 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.455 sigma_q2_arcsec=0.400 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.337 n_q1=266 n_q2=204 n_q3=249 n_q4=238 worst_quadrant_to_overall_ratio=1.194
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.q5nKdAimIz (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=724, passed=9037
Got 9037 stars (including 8310 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat
util/solve_plate_with_UCAC5 got 9037 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 8949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 8948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 8948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits N_match=958 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.483 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.392 sigma_q4_arcsec=0.345 n_q1=262 n_q2=201 n_q3=256 n_q4=239 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.h5Mg6hdjMw (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_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.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_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=35, passed=963
Got 963 stars (including 927 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat
util/solve_plate_with_UCAC5 got 963 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.2)
Done reading UCAC5 zone files...
Matched 861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 861 matched stars entering correct_measured_positions(), 822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 861 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.2)
Done reading UCAC5 zone files...
Matched 862 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 862 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 862 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 862 stars left (next iteration limit 947)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits N_match=862 sigma_overall_arcsec=0.325 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.468 sigma_q3_arcsec=0.309 sigma_q4_arcsec=0.336 n_q1=317 n_q2=128 n_q3=264 n_q4=153 worst_quadrant_to_overall_ratio=1.439
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zpI6TbifV2 (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_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.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_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=42, passed=887
Got 887 stars (including 844 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat
util/solve_plate_with_UCAC5 got 887 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.2)
Done reading UCAC5 zone files...
Matched 782 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 782 matched stars entering correct_measured_positions(), 751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 782 matched stars entering correct_measured_positions(), 845 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.2)
Done reading UCAC5 zone files...
Matched 782 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 782 matched stars entering correct_measured_positions(), 844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 782 matched stars entering correct_measured_positions(), 844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 782 stars left (next iteration limit 860)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits N_match=782 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.491 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.302 n_q1=315 n_q2=140 n_q3=213 n_q4=114 worst_quadrant_to_overall_ratio=1.408
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat.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=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits sigma_overall=0.381 worst_q_ratio=1.194
ref2=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits sigma_overall=0.407 worst_q_ratio=1.185
new1=fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits sigma_overall=0.325 worst_q_ratio=1.439
new2=fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits sigma_overall=0.349 worst_q_ratio=1.408
reference average sigma_overall=0.394 worst_q_ratio=1.1895
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037_astrometric_residuals.png (see messages above)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits'
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20490_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
The candidate 20490_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037 did not pass the final checks
**** FOUND 09:43:25.56 +19:51:39.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits exists and is non-empty
wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (1st reference image)
verification OK: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:50.749 +22:00:00.30 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_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits (1st new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
Image size: 941.5'x626.6' 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: 09:14:01.839 +22:00:17.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:13:50.749 +22:00:00.30
Second-epoch image center 09:14:01.839 +22:00:17.41
Angular distance between the image centers 0.0431 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits (2nd new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
Image size: 941.5'x626.6' 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: 09:14:00.269 +22:00:48.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:13:50.749 +22:00:00.30
Second-epoch image center 09:14:00.269 +22:00:48.79
Angular distance between the image centers 0.0392 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 09:14:01.839 +22:00:17.41
Second-epoch second image center 09:14:00.269 +22:00:48.79
Angular distance between the image centers 0.01062 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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits &> /tmp/tmp.ns79zthSin
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits &> /tmp/tmp.2SvklkCiKq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits &> /tmp/tmp.R0nxvQfGTl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits &> /tmp/tmp.0PCWz3E8q4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat
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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat
The reference image (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits) and catalog (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat) found
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat' -> 'wcsmag.cat'
Read 50507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4949 to 147.0725 deg, Dec +16.3332 to +27.3504 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 129.4949 to 147.0725 deg, Dec 16.3332 to 27.3504 deg
Loaded 6013 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): 4206 out of 4845 total matches.
Matched with Tycho-2 4845 out of 50507 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.814650
a=0.000000 b=1.000000 c=22.814650
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 50507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4949 to 147.0725 deg, Dec +16.3332 to +27.3504 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 129.4949 to 147.0725 deg, Dec 16.3332 to 27.3504 deg
Loaded 6013 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): 4206 out of 4845 total matches.
Matched with Tycho-2 4845 out of 50507 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits:
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (aperture=5.0)
Read 50709 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4922 to 147.0612 deg, Dec +16.3288 to +27.3568 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 129.4922 to 147.0612 deg, Dec 16.3288 to 27.3568 deg
Loaded 6019 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): 4180 out of 4844 total matches.
Matched with Tycho-2 4844 out of 50709 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits:
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 41 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.0 pix Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
1.9 pix fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
1.8 pix fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
2.0 pix wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.0 pix wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Limiting magnitude estimates:
15.5 mag. Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
15.5 mag. Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
12.8 mag. fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
12.7 mag. fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 12.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ns79zthSin (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=2848, passed=50482
Got 50482 stars (including 47533 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat
util/solve_plate_with_UCAC5 got 50482 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 50087 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 50084 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 50083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits N_match=953 sigma_overall_arcsec=0.385 sigma_q1_arcsec=0.440 sigma_q2_arcsec=0.394 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.354 n_q1=260 n_q2=193 n_q3=256 n_q4=244 worst_quadrant_to_overall_ratio=1.144
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2SvklkCiKq (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=2904, passed=50680
Got 50680 stars (including 47694 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat
util/solve_plate_with_UCAC5 got 50680 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 50198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 50198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 50198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits N_match=957 sigma_overall_arcsec=0.416 sigma_q1_arcsec=0.470 sigma_q2_arcsec=0.403 sigma_q3_arcsec=0.394 sigma_q4_arcsec=0.376 n_q1=259 n_q2=193 n_q3=261 n_q4=244 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.R0nxvQfGTl (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_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.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_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=115, passed=8211
Got 8211 stars (including 8081 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat
util/solve_plate_with_UCAC5 got 8211 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.2 to 27.5)
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: 928 matched stars entering correct_measured_positions(), 889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 7785 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.2 to 27.5)
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: 928 matched stars entering correct_measured_positions(), 7784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 7784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits N_match=928 sigma_overall_arcsec=0.307 sigma_q1_arcsec=0.289 sigma_q2_arcsec=0.436 sigma_q3_arcsec=0.289 sigma_q4_arcsec=0.312 n_q1=362 n_q2=138 n_q3=275 n_q4=153 worst_quadrant_to_overall_ratio=1.422
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0PCWz3E8q4 (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_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.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_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=103, passed=7856
Got 7856 stars (including 7734 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat
util/solve_plate_with_UCAC5 got 7856 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 7502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 7500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 7500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits N_match=926 sigma_overall_arcsec=0.351 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.504 sigma_q3_arcsec=0.334 sigma_q4_arcsec=0.278 n_q1=381 n_q2=172 n_q3=243 n_q4=130 worst_quadrant_to_overall_ratio=1.436
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits.cat.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_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.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_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-19-41_20.00sec_-0.00C_LIGHTs_0036.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.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_2026-06-07_CI_Cnc-03-Q1b1x1_224245_TTUQ1b1x1_346189_aynpDvrb/wcs_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037.fits
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:57.81 +22:32:22.0: 13.04 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:25:08.90 +23:34:04.1: 13.22 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:26.41 +22:52:05.1: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:57.92 +22:59:15.7: 12.74 +/- 0.01 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:58.36 +22:23:51.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:16.53 +22:50:27.0: 12.60 +/- 0.01 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:18.01 +22:06:36.5: 13.20 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:24:56.57 +23:55:05.5: 13.06 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:24:14.14 +23:37:38.6: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:35.73 +23:24:59.2: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:24:56.57 +23:55:05.5: 13.09 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:58.36 +22:23:51.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:25:08.90 +23:34:04.1: 13.26 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:16.53 +22:50:27.0: 12.62 +/- 0.01 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:57.92 +22:59:15.7: 12.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry filter KEPT candidate at 09:24:56.57 +23:55:05.5: ref_mag=13.07 +/- 0.01 new_mean_mag=12.1277 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 09:21:58.36 +22:23:51.3: ref_mag=13.06 +/- 0.01 new_mean_mag=12.1488 delta=0.91 (need > 0.90)
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 09:25:08.90 +23:34:04.1: ref_mag=13.24 +/- 0.02 new_mean_mag=12.2706 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 09:22:57.92 +22:59:15.7: ref_mag=12.75 +/- 0.01 new_mean_mag=11.7680 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 09:22:16.53 +22:50:27.0: ref_mag=12.61 +/- 0.01 new_mean_mag=11.6393 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:57.81 +22:32:22.0: 13.06 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:26.41 +22:52:05.1: 13.05 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:18.01 +22:06:36.5: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry reference-image weighted average: 13.05 +/- 0.01
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 09:22:26.41 +22:52:05.1: ref_mag=13.07 +/- 0.01 new_mean_mag=12.0410 delta=1.03 (need > 0.90)
Forced photometry filter KEPT candidate at 09:21:57.81 +22:32:22.0: ref_mag=13.05 +/- 0.01 new_mean_mag=12.0497 delta=1.00 (need > 0.90)
Forced photometry filter KEPT candidate at 09:21:18.01 +22:06:36.5: ref_mag=13.19 +/- 0.02 new_mean_mag=12.2817 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:24:14.14 +23:37:38.6: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 09:24:14.14 +23:37:38.6: ref_mag=13.06 +/- 0.02 new_mean_mag=12.0165 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:35.73 +23:24:59.2: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 09:22:35.73 +23:24:59.2: ref_mag=13.02 +/- 0.01 new_mean_mag=11.9864 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:15.59 +23:05:38.9: 13.03 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:15.59 +23:05:38.9: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter KEPT candidate at 09:23:15.59 +23:05:38.9: ref_mag=13.03 +/- 0.01 new_mean_mag=12.0525 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:26:10.86 +23:59:23.3: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:26:10.86 +23:59:23.3: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.01
Forced photometry filter KEPT candidate at 09:26:10.86 +23:59:23.3: ref_mag=13.02 +/- 0.01 new_mean_mag=12.0469 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:32.57 +23:08:57.3: 13.55 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:04.02 +23:41:41.1: 13.34 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:04.02 +23:41:41.1: 13.35 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:32.57 +23:08:57.3: 13.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.02
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 09:23:04.02 +23:41:41.1: ref_mag=13.34 +/- 0.02 new_mean_mag=12.3727 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 09:23:32.57 +23:08:57.3: ref_mag=13.60 +/- 0.02 new_mean_mag=12.5146 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:25:32.87 +23:41:50.8: 13.51 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:56.82 +23:22:18.5: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:25:32.87 +23:41:50.8: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Forced photometry filter KEPT candidate at 09:25:32.87 +23:41:50.8: ref_mag=13.53 +/- 0.02 new_mean_mag=12.4840 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:56.82 +23:22:18.5: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Forced photometry filter KEPT candidate at 09:23:56.82 +23:22:18.5: ref_mag=13.35 +/- 0.02 new_mean_mag=12.2835 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:27:10.04 +24:30:49.5: 13.29 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:27:10.04 +24:30:49.5: 13.25 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:57.30 +22:25:02.5: 13.29 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:27:56.39 +24:58:52.5: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 09:27:10.04 +24:30:49.5: ref_mag=13.27 +/- 0.02 new_mean_mag=12.3110 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:27:56.39 +24:58:52.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:57.30 +22:25:02.5: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 09:27:56.39 +24:58:52.5: ref_mag=13.29 +/- 0.02 new_mean_mag=12.3266 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 09:21:57.30 +22:25:02.5: ref_mag=13.26 +/- 0.02 new_mean_mag=12.1818 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:02.31 +22:39:26.8: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:02.31 +22:39:26.8: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 09:22:02.31 +22:39:26.8: ref_mag=12.93 +/- 0.01 new_mean_mag=11.8899 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:59:41.69 +22:13:38.2: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:59:41.69 +22:13:38.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 08:59:41.69 +22:13:38.2: ref_mag=12.90 +/- 0.01 new_mean_mag=11.9200 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:24:36.41 +24:09:57.0: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:24:36.41 +24:09:57.0: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter KEPT candidate at 09:24:36.41 +24:09:57.0: ref_mag=12.92 +/- 0.01 new_mean_mag=11.9541 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:52.52 +22:38:34.5: 12.52 +/- 0.01 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:52.52 +22:38:34.5: 12.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter KEPT candidate at 09:21:52.52 +22:38:34.5: ref_mag=12.52 +/- 0.01 new_mean_mag=11.5522 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:22.11 +23:14:51.2: 13.79 +/- 0.04 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:22.11 +23:14:51.2: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 09:23:22.11 +23:14:51.2: ref_mag=13.77 +/- 0.03 new_mean_mag=12.3798 delta=1.39 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:27.60 +23:09:52.8: 13.59 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:27.60 +23:09:52.8: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Forced photometry filter KEPT candidate at 09:22:27.60 +23:09:52.8: ref_mag=13.62 +/- 0.02 new_mean_mag=12.4656 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:28.57 +22:42:23.3: 13.18 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:10.43 +23:17:42.6: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:28.57 +22:42:23.3: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 09:22:28.57 +22:42:23.3: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1621 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:47.48 +23:13:19.9: 13.16 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:41.43 +23:07:49.9: 13.16 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:18:29.84 +21:07:01.5: 13.14 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:10.43 +23:17:42.6: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 09:23:10.43 +23:17:42.6: ref_mag=13.39 +/- 0.02 new_mean_mag=12.3379 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:47.48 +23:13:19.9: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 09:22:47.48 +23:13:19.9: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1458 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:18:29.84 +21:07:01.5: 13.12 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:41.43 +23:07:49.9: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 09:18:29.84 +21:07:01.5: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1661 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter KEPT candidate at 09:22:41.43 +23:07:49.9: ref_mag=13.17 +/- 0.02 new_mean_mag=12.1216 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:25:28.33 +24:29:56.1: 12.97 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:25:28.33 +24:29:56.1: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter REJECTED candidate at 09:25:28.33 +24:29:56.1: ref_mag=12.97 +/- 0.01 new_mean_mag=12.1444 delta=0.83 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:32.83 +22:17:58.4: 13.37 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:32.83 +22:17:58.4: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 09:21:32.83 +22:17:58.4: ref_mag=13.36 +/- 0.02 new_mean_mag=12.3805 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:26:14.91 +24:16:27.1: 13.37 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:26:14.91 +24:16:27.1: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 09:26:14.91 +24:16:27.1: ref_mag=13.40 +/- 0.02 new_mean_mag=12.4141 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:24:05.13 +23:28:38.9: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:24:05.13 +23:28:38.9: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Forced photometry filter KEPT candidate at 09:24:05.13 +23:28:38.9: ref_mag=13.10 +/- 0.01 new_mean_mag=12.1633 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:04.90 +22:26:16.5: 13.37 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:22:05.42 +23:09:58.0: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:04.90 +22:26:16.5: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 09:22:04.90 +22:26:16.5: ref_mag=13.36 +/- 0.02 new_mean_mag=12.2704 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:23:03.68 +23:25:55.3: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:22:05.42 +23:09:58.0: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 09:22:05.42 +23:09:58.0: ref_mag=13.11 +/- 0.02 new_mean_mag=12.0940 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:23:03.68 +23:25:55.3: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Forced photometry filter KEPT candidate at 09:23:03.68 +23:25:55.3: ref_mag=13.08 +/- 0.01 new_mean_mag=12.0627 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:18:18.33 +20:49:35.9: 13.09 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:18:18.33 +20:49:35.9: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Forced photometry filter KEPT candidate at 09:18:18.33 +20:49:35.9: ref_mag=13.10 +/- 0.01 new_mean_mag=12.0810 delta=1.02 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_local.txt__out19463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50215.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 63s
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: 19s
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Considering the candidate 64177_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
The candidate 64177_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037 did not pass the final checks
**** FOUND 09:13:35.56 +26:26:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64505_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
The candidate 64505_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037 did not pass the final checks
**** FOUND 09:42:15.79 +24:29:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25749_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 25749_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 50215_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 50215_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 29309_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 29309_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 29473_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 29473_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 30038_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 30038_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 48226_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 48226_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 27092_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 27092_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 27814_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 27814_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 35184_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 35184_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 49872_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 49872_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 30556_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 30556_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 49120_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 49120_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 36523_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 36523_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 49641_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 49641_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 49562_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 49562_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 35414_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 35414_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 14155_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
The candidate 14155_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037 did not pass the final checks
**** FOUND 09:43:25.54 +19:51:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45849_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 45849_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 27215_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 27215_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 43777_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 43777_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 28420_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 28420_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 27292_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 27292_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 47516_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 47516_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 28357_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 28357_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 35884_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 35884_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 36389_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 36389_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 28692_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 28692_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 35829_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 35829_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 36137_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 36137_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 36550_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 36550_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 20869_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 20869_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 45977_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
The candidate 45977_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037 did not pass the final checks
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Considering the candidate 26670_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 26670_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 46902_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 46902_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 34884_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 34884_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 27343_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 27343_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 36149_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 36149_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 35076_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 35076_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
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Considering the candidate 19463_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
Preparing report for the candidate 19463_fd_Cnc-03-Q1b1x1_2026-06-07_22-20-26_20.00sec_0.00C_LIGHTs_0037
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 84s
Prepared the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:18:18.33 +20:49:35.9
09:18:29.84 +21:07:01.5
09:21:18.01 +22:06:36.5
09:21:32.83 +22:17:58.4
09:21:58.36 +22:23:51.3
09:21:57.30 +22:25:02.5
08:59:41.69 +22:13:38.2
09:22:04.90 +22:26:16.5
09:21:57.81 +22:32:22.0
09:21:52.52 +22:38:34.5
09:22:02.31 +22:39:26.8
09:22:28.57 +22:42:23.3
09:22:16.53 +22:50:27.0
09:22:26.41 +22:52:05.1
09:22:57.92 +22:59:15.7
09:23:15.59 +23:05:38.9
09:24:05.13 +23:28:38.9
09:23:03.68 +23:25:55.3
09:22:35.73 +23:24:59.2
09:23:56.82 +23:22:18.5
09:23:10.43 +23:17:42.6
09:23:22.11 +23:14:51.2
09:22:47.48 +23:13:19.9
09:22:05.42 +23:09:58.0
09:22:27.60 +23:09:52.8
09:23:32.57 +23:08:57.3
09:22:41.43 +23:07:49.9
09:27:56.39 +24:58:52.5
09:27:10.04 +24:30:49.5
09:26:14.91 +24:16:27.1
09:24:36.41 +24:09:57.0
09:24:56.57 +23:55:05.5
09:26:10.86 +23:59:23.3
09:25:32.87 +23:41:50.8
09:23:04.02 +23:41:41.1
09:24:14.14 +23:37:38.6
09:25:08.90 +23:34:04.1
########### Completed Cnc-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
09:21:18.01 +22:06:36.5
09:25:08.90 +23:34:04.1
09:22:16.53 +22:50:27.0
09:22:26.41 +22:52:05.1
09:22:57.92 +22:59:15.7
09:24:56.57 +23:55:05.5
09:21:58.36 +22:23:51.3
09:21:57.81 +22:32:22.0
09:22:35.73 +23:24:59.2
09:24:14.14 +23:37:38.6
09:23:15.59 +23:05:38.9
09:26:10.86 +23:59:23.3
09:23:32.57 +23:08:57.3
09:23:04.02 +23:41:41.1
09:25:32.87 +23:41:50.8
09:23:56.82 +23:22:18.5
09:27:10.04 +24:30:49.5
09:21:57.30 +22:25:02.5
09:27:56.39 +24:58:52.5
09:22:02.31 +22:39:26.8
08:59:41.69 +22:13:38.2
09:24:36.41 +24:09:57.0
09:21:52.52 +22:38:34.5
09:23:22.11 +23:14:51.2
09:22:27.60 +23:09:52.8
09:22:28.57 +22:42:23.3
09:23:10.43 +23:17:42.6
09:22:47.48 +23:13:19.9
09:22:41.43 +23:07:49.9
09:18:29.84 +21:07:01.5
09:21:32.83 +22:17:58.4
09:26:14.91 +24:16:27.1
09:24:05.13 +23:28:38.9
09:22:04.90 +22:26:16.5
09:22:05.42 +23:09:58.0
09:23:03.68 +23:25:55.3
09:18:18.33 +20:49:35.9
###################################################################################
09:21:18.01 +22:06:36.5 -- not an asteroid (will add it to exclusion list)
09:25:08.90 +23:34:04.1 -- not an asteroid (will add it to exclusion list)
09:22:16.53 +22:50:27.0 -- not an asteroid (will add it to exclusion list)
09:22:26.41 +22:52:05.1 -- not an asteroid (will add it to exclusion list)
09:22:57.92 +22:59:15.7 -- not an asteroid (will add it to exclusion list)
09:24:56.57 +23:55:05.5 -- not an asteroid (will add it to exclusion list)
09:21:58.36 +22:23:51.3 -- not an asteroid (will add it to exclusion list)
09:21:57.81 +22:32:22.0 -- not an asteroid (will add it to exclusion list)
09:22:35.73 +23:24:59.2 -- not an asteroid (will add it to exclusion list)
09:24:14.14 +23:37:38.6 -- not an asteroid (will add it to exclusion list)
09:23:15.59 +23:05:38.9 -- not an asteroid (will add it to exclusion list)
09:26:10.86 +23:59:23.3 -- not an asteroid (will add it to exclusion list)
09:23:32.57 +23:08:57.3 -- not an asteroid (will add it to exclusion list)
09:23:04.02 +23:41:41.1 -- not an asteroid (will add it to exclusion list)
09:25:32.87 +23:41:50.8 -- not an asteroid (will add it to exclusion list)
09:23:56.82 +23:22:18.5 -- not an asteroid (will add it to exclusion list)
09:27:10.04 +24:30:49.5 -- not an asteroid (will add it to exclusion list)
09:21:57.30 +22:25:02.5 -- not an asteroid (will add it to exclusion list)
09:27:56.39 +24:58:52.5 -- not an asteroid (will add it to exclusion list)
09:22:02.31 +22:39:26.8 -- not an asteroid (will add it to exclusion list)
08:59:41.69 +22:13:38.2 -- not an asteroid (will add it to exclusion list)
09:24:36.41 +24:09:57.0 -- not an asteroid (will add it to exclusion list)
09:21:52.52 +22:38:34.5 -- not an asteroid (will add it to exclusion list)
09:23:22.11 +23:14:51.2 -- not an asteroid (will add it to exclusion list)
09:22:27.60 +23:09:52.8 -- not an asteroid (will add it to exclusion list)
09:22:28.57 +22:42:23.3 -- not an asteroid (will add it to exclusion list)
09:23:10.43 +23:17:42.6 -- not an asteroid (will add it to exclusion list)
09:22:47.48 +23:13:19.9 -- not an asteroid (will add it to exclusion list)
09:22:41.43 +23:07:49.9 -- not an asteroid (will add it to exclusion list)
09:18:29.84 +21:07:01.5 -- not an asteroid (will add it to exclusion list)
09:21:32.83 +22:17:58.4 -- not an asteroid (will add it to exclusion list)
09:26:14.91 +24:16:27.1 -- not an asteroid (will add it to exclusion list)
09:24:05.13 +23:28:38.9 -- not an asteroid (will add it to exclusion list)
09:22:04.90 +22:26:16.5 -- not an asteroid (will add it to exclusion list)
09:22:05.42 +23:09:58.0 -- not an asteroid (will add it to exclusion list)
09:23:03.68 +23:25:55.3 -- not an asteroid (will add it to exclusion list)
09:18:18.33 +20:49:35.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
08:59:41.69 +22:13:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:18:18.33 +20:49:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:18:29.84 +21:07:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:18.01 +22:06:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:32.83 +22:17:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:52.52 +22:38:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:57.30 +22:25:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:57.81 +22:32:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:58.36 +22:23:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:02.31 +22:39:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:04.90 +22:26:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:05.42 +23:09:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:16.53 +22:50:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:26.41 +22:52:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:27.60 +23:09:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:28.57 +22:42:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:35.73 +23:24:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:41.43 +23:07:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:47.48 +23:13:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:57.92 +22:59:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:23:03.68 +23:25:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:23:04.02 +23:41:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:23:10.43 +23:17:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:23:15.59 +23:05:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:23:22.11 +23:14:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:23:32.57 +23:08:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:23:56.82 +23:22:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:24:05.13 +23:28:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:24:14.14 +23:37:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:24:36.41 +24:09:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:24:56.57 +23:55:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:25:08.90 +23:34:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:25:32.87 +23:41:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:26:10.86 +23:59:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:26:14.91 +24:16:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:27:10.04 +24:30:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:27:56.39 +24:58:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
08:59:41.69 +22:13:38.2 -- not a known variable star
09:18:18.33 +20:49:35.9 -- not a known variable star
09:18:29.84 +21:07:01.5 -- not a known variable star
09:21:18.01 +22:06:36.5 -- not a known variable star
09:21:32.83 +22:17:58.4 -- not a known variable star
09:21:52.52 +22:38:34.5 -- not a known variable star
09:21:57.30 +22:25:02.5 -- not a known variable star
09:21:57.81 +22:32:22.0 -- not a known variable star
09:21:58.36 +22:23:51.3 -- not a known variable star
09:22:02.31 +22:39:26.8 -- not a known variable star
09:22:04.90 +22:26:16.5 -- not a known variable star
09:22:05.42 +23:09:58.0 -- not a known variable star
09:22:16.53 +22:50:27.0 -- not a known variable star
09:22:26.41 +22:52:05.1 -- not a known variable star
09:22:27.60 +23:09:52.8 -- not a known variable star
09:22:28.57 +22:42:23.3 -- not a known variable star
09:22:35.73 +23:24:59.2 -- not a known variable star
09:22:41.43 +23:07:49.9 -- not a known variable star
09:22:47.48 +23:13:19.9 -- not a known variable star
09:22:57.92 +22:59:15.7 -- a known variable star
09:23:03.68 +23:25:55.3 -- not a known variable star
09:23:04.02 +23:41:41.1 -- not a known variable star
09:23:10.43 +23:17:42.6 -- not a known variable star
09:23:15.59 +23:05:38.9 -- not a known variable star
09:23:22.11 +23:14:51.2 -- not a known variable star
09:23:32.57 +23:08:57.3 -- not a known variable star
09:23:56.82 +23:22:18.5 -- not a known variable star
09:24:05.13 +23:28:38.9 -- not a known variable star
09:24:14.14 +23:37:38.6 -- a known variable star
09:24:36.41 +24:09:57.0 -- not a known variable star
09:24:56.57 +23:55:05.5 -- not a known variable star
09:25:08.90 +23:34:04.1 -- not a known variable star
09:25:32.87 +23:41:50.8 -- not a known variable star
09:26:10.86 +23:59:23.3 -- not a known variable star
09:26:14.91 +24:16:27.1 -- not a known variable star
09:27:10.04 +24:30:49.5 -- not a known variable star
09:27:56.39 +24:58:52.5 -- not a known variable star
Found 35 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
37 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
08:59:41.69 +22:13:38.2
09:18:18.33 +20:49:35.9
09:18:29.84 +21:07:01.5
09:21:18.01 +22:06:36.5
09:21:32.83 +22:17:58.4
09:21:52.52 +22:38:34.5
09:21:57.30 +22:25:02.5
09:21:57.81 +22:32:22.0
09:21:58.36 +22:23:51.3
09:22:02.31 +22:39:26.8
09:22:04.90 +22:26:16.5
09:22:05.42 +23:09:58.0
09:22:16.53 +22:50:27.0
09:22:26.41 +22:52:05.1
09:22:27.60 +23:09:52.8
09:22:28.57 +22:42:23.3
09:22:35.73 +23:24:59.2
09:22:41.43 +23:07:49.9
09:22:47.48 +23:13:19.9
09:22:57.92 +22:59:15.7
09:23:03.68 +23:25:55.3
09:23:04.02 +23:41:41.1
09:23:10.43 +23:17:42.6
09:23:15.59 +23:05:38.9
09:23:22.11 +23:14:51.2
09:23:32.57 +23:08:57.3
09:23:56.82 +23:22:18.5
09:24:05.13 +23:28:38.9
09:24:14.14 +23:37:38.6
09:24:36.41 +24:09:57.0
09:24:56.57 +23:55:05.5
09:25:08.90 +23:34:04.1
09:25:32.87 +23:41:50.8
09:26:10.86 +23:59:23.3
09:26:14.91 +24:16:27.1
09:27:10.04 +24:30:49.5
09:27:56.39 +24:58:52.5
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461199.63879346 -observatory V36
06:43:24.95 +25:00:40.1 Mercury (0.1mag)
07:42:35.16 +23:23:24.0 Venus (-4.0mag)
02:49:27.23 +15:42:07.5 Mars (1.3mag)
07:48:23.60 +21:31:33.9 Jupiter (-1.9mag)
00:49:21.53 +02:48:35.9 Saturn (0.9mag)
04:00:11.65 +20:25:25.6 Uranus (5.8mag)
00:16:08.34 +00:16:47.3 Neptune (7.8mag)
20:33:21.57 -23:04:31.6 Pluto (14.5mag)
23:00:14.41 -05:57:19.7 Moon (-10.5mag)
-rw-r--r-- 1 apache apache 362 Jun 7 22:48 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461199.63879346:
07:48:23.40 +21:31:36.7 Io (6.0mag)
07:48:22.95 +21:31:38.1 Europa (6.2mag)
07:48:07.75 +21:32:20.9 Ganymede (5.6mag)
07:48:42.66 +21:30:32.6 Callisto (6.7mag)
07:48:41.14 +21:07:51.4 Himalia (15.6mag)
07:48:27.77 +21:31:21.4 Thebe (16.5mag)
07:48:40.67 +21:23:19.3 Elara (17.5mag)
07:50:34.12 +21:43:17.5 Pasiphae (17.7mag)
07:54:58.82 +21:33:16.1 Carme (18.9mag)
00:49:12.00 +02:48:35.2 Titan (8.7mag)
00:49:18.68 +02:48:49.4 Rhea (9.9mag)
00:49:53.83 +02:50:45.0 Iapetus (11.3mag)
00:49:17.33 +02:48:13.1 Hyperion (14.7mag)
00:50:03.86 +02:50:32.9 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 7 22:48 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461199.63879346:
17:26:49.46 -35:13:37.8 JWST
14:16:49.42 +57:52:54.1 Chandra
18:18:55.95 -30:54:41.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 7 22:48 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461199.63879346 -observatory V36
18:43:32.97 -32:38:59.6 13.6mag P/2010 H2 (Vales)
05:53:24.95 -68:03:52.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:49:02.32 +31:58:02.4 17.5mag C/2017 K2 (PANSTARRS)
17:14:45.30 +15:20:56.9 17.8mag C/2021 G2 (ATLAS)
21:11:46.09 -49:30:53.0 16.9mag P/2021 N1 (ZTF)
23:12:38.74 +31:35:23.7 17.2mag C/2022 E2 (ATLAS)
05:33:58.42 +26:58:30.8 16.5mag C/2022 N2 (PANSTARRS)
09:29:41.27 +31:05:04.7 16.6mag C/2022 QE78 (ATLAS)
08:50:30.97 +03:55:45.4 17.7mag C/2022 R6 (PANSTARRS)
18:28:15.53 +21:36:04.6 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:19:23.62 -11:00:30.8 17.6mag P/2023 B1 (PANSTARRS)
22:14:27.00 +66:31:30.5 17.7mag C/2023 H5 (Lemmon)
17:46:31.54 -06:41:01.7 13.7mag C/2023 R1 (PANSTARRS)
13:18:07.72 +83:00:21.9 17.9mag C/2023 X2 (Lemmon)
07:10:20.21 +64:18:26.3 17.7mag C/2024 A1 (ATLAS)
06:47:11.17 +27:49:45.8 13.6mag C/2024 E1 (Wierzchos)
15:37:19.99 +13:31:17.5 17.4mag C/2024 G6 (ATLAS)
20:13:04.98 +31:07:07.4 14.0mag C/2024 J3 (ATLAS)
04:17:58.18 -15:57:21.4 16.0mag C/2024 T5 (ATLAS)
06:05:51.53 +34:30:04.6 17.9mag C/2025 J1 (Borisov)
11:34:56.01 +52:45:08.7 17.4mag C/2025 L1 (ATLAS)
06:44:52.43 -10:52:02.3 14.1mag C/2025 R3 (PANSTARRS)
09:24:06.97 +23:20:26.8 17.9mag C/2025 V2 (Rankin)
12:39:42.19 +04:41:28.5 17.2mag C/2025 Y1 (ATLAS)
18:12:58.58 +75:07:12.5 17.9mag C/2026 A2 (Bok)
02:00:34.02 +43:24:40.7 16.1mag C/2026 B2 (Sun-Gao)
11:11:18.09 -03:45:10.9 16.5mag A/2026 E1
20:23:32.93 -08:33:55.7 8.7mag 10P/Tempel
11:01:59.55 -00:58:01.9 16.0mag 29P/Schwassmann-Wachmann
03:11:38.02 +25:38:17.7 17.7mag 47P/Ashbrook-Jackson
08:59:51.66 +23:47:06.6 16.9mag 63P/Wild
00:26:52.71 -06:22:15.9 15.7mag 65P/Gunn
06:43:15.51 +33:25:28.2 16.9mag 76P/West-Kohoutek-Ikemura
03:09:02.71 +17:12:34.4 13.8mag 78P/Gehrels
01:20:38.18 +04:50:13.8 15.6mag 88P/Howell
04:54:27.58 +30:17:56.1 15.2mag 93P/Lovas
02:42:47.49 +27:37:01.7 17.6mag 114P/Wiseman-Skiff
06:50:24.84 +33:02:25.2 15.6mag 123P/West-Hartley
09:50:04.94 +14:39:41.4 16.5mag 124P/Mrkos
03:58:56.56 +19:14:48.3 16.4mag 128P/Shoemaker-Holt
04:33:27.10 +19:04:55.1 17.7mag 131P/Mueller
05:58:04.23 +18:40:18.7 14.6mag 141P/Machholz
06:00:42.31 +17:40:20.7 14.6mag 141P-A/Machholz
04:53:48.46 +16:09:57.8 11.6mag 141P-D/Machholz
02:57:38.26 -24:42:26.5 16.8mag 161P/Hartley-IRAS
03:41:21.74 +23:47:14.0 14.9mag 162P/SidingSpring
19:36:38.39 +01:42:46.3 16.9mag 169P/NEAT
00:18:11.05 +02:27:15.9 17.9mag 220P/McNaught
16:52:13.64 -08:28:42.7 16.4mag 235P/LINEAR
07:34:31.82 +35:29:39.7 17.5mag 240P/NEAT
00:32:12.16 -02:29:34.1 16.4mag 260P/McNaught
04:04:04.31 +32:28:15.3 17.6mag 295P/LINEAR
23:51:53.23 -09:46:54.6 17.6mag 320P/McNaught
15:15:15.85 +08:06:06.2 17.4mag 391P/Kowalski
08:07:05.54 +20:44:55.9 17.9mag 450P/LONEOS
06:59:52.87 +41:42:02.1 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 7 22:48 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
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
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
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 2026-04-9.29 13.32
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 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
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
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 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
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
-rw-r--r-- 1 apache apache 5.6K Jun 7 22:48 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 7 22:48 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:39:35.110 +15:17:58.28 AT 2026nsc 2026-05-09.80 20.76
16:42:48.680 +20:27:18.30 AT 2026nsb 2026-05-09.80 20.54
13:34:03.440 +31:37:31.73 AT 2026nsa 2026-05-07.80 21.26
13:50:28.150 +02:34:54.72 AT 2026nrz 2026-05-22.72 21.54
13:43:59.750 +03:47:21.63 AT 2026nry 2026-05-22.69 22.05
13:17:26.150 -01:26:00.12 AT 2026nrx 2026-05-21.64 21.7
00:35:20.216 -08:28:38.64 AT 2026nrw 2026-05-19.42 18.74
23:50:43.016 -01:09:12.25 AT 2026nrv 2026-05-23.48 19.5028
22:36:47.715 +37:31:34.81 AT 2026nru 2026-05-22.43 19.4626
23:58:04.247 +20:56:44.66 AT 2026nrt 2026-05-23.48 20.1237
16:08:58.229 +36:53:23.76 AT 2026nrs 2026-05-21.36 20.3819
19:44:04.734 +84:44:44.91 SN 2026nrr 2026-05-25.47 17.808
21:42:24.388 -20:21:08.51 SN 2026nrq 2026-05-25.56 18.623
22:03:20.669 -84:55:27.45 AT 2026nrp 2026-05-22.30 19.244
23:07:53.376 -39:04:26.84 AT 2026nro 2026-05-22.38 19.567
00:40:07.848 -39:10:21.32 AT 2026nrn 2026-05-12.41 18.737
23:05:28.381 -21:25:50.28 AT 2026nrm 2026-05-25.58 18.887
19:27:28.750 -48:42:52.35 AT 2026nrl 2026-05-22.24 19.107
12:33:38.422 +12:02:05.88 AT 2026nrk 2026-05-25.29 21.322
12:32:27.199 +02:39:54.51 AT 2026nrj 2026-05-25.29 21.0728
-rw-r--r-- 1 apache apache 30K Jun 7 22:48 tns_transients_list.txt
