This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.40 21:37:38.20 +60:41:33.5
101.30812 6.23873 galactic Cep Second-epoch detections are separated by 0.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:38.20 +60:41:33.5 (user input) | T | P | (position from user input) J-Ks=0.226+/-0.036 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:37:38.20 +60:41:33.5: 13.49 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:37:38.20 +60:41:33.5: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3909 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.00 21:34:41.78 +60:44:30.0
101.07411 6.51728 galactic Cep Second-epoch detections are separated by 1.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2215793041262149120 | 21:34:41.90 +60:44:30.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.154+/-0.039 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:41.78 +60:44:30.0: 12.81 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:41.78 +60:44:30.0: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2215793041262149120,2461239.8909,12.00,0.05,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 2215793041262149120 20260718.3909 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.25 21:35:35.39 +60:51:21.1
101.23265 6.52758 galactic Cep Second-epoch detections are separated by 3.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:35.39 +60:51:21.1 (user input) | T | P | (position from user input) J-Ks=0.499+/-0.033 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:35:35.39 +60:51:21.1: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:35:35.39 +60:51:21.1: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,12.25,0.05,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 20260718.3909 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 11.86 21:37:02.75 +60:39:04.7
101.22625 6.25661 galactic Cep Second-epoch detections are separated by 0.9" and 5.3 pix
The object was found in VSX19" Gaia DR3 2215774285146323072
Type: E
# Max. Min./Amp. JD0 Period
13.950 G 14.000 G 1.118100000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:37:02.75 +60:39:04.7: 12.75 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:37:02.75 +60:39:04.7: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2215774285146323072,2461239.8909,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2215774285146323072 20260718.3909 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.41 21:37:13.38 +60:31:37.4
101.15857 6.14991 galactic Cep Second-epoch detections are separated by 1.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:37:13.38 +60:31:37.4 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.036 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:37:13.38 +60:31:37.4: 13.45 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:37:13.38 +60:31:37.4: 13.69 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,12.41,0.05,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 20260718.3909 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.12 21:34:34.25 +60:32:23.2
100.92497 6.37931 galactic Cep Second-epoch detections are separated by 0.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:34.25 +60:32:23.2 (user input) | T | P | (position from user input) J-Ks=0.264+/-0.035 (F)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:34.25 +60:32:23.2: 13.00 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:34.25 +60:32:23.2: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,12.12,0.05,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 20260718.3909 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.22 21:34:26.58 +60:47:37.7
101.08683 6.57657 galactic Cep Second-epoch detections are separated by 0.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:26.58 +60:47:37.7 (user input) | T | P | (position from user input) J-Ks=0.754+/-0.033 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:26.58 +60:47:37.7: 13.25 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:26.58 +60:47:37.7: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3909 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.45 21:35:47.32 +60:32:38.4
101.03879 6.28113 galactic Cep Second-epoch detections are separated by 1.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:47.32 +60:32:38.4 (user input) | T | P | (position from user input) J-Ks=0.916+/-0.033 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:35:47.32 +60:32:38.4: 13.61 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:35:47.32 +60:32:38.4: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3909 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 11.99 21:36:00.31 +60:50:32.9
101.26110 6.48356 galactic Cep Second-epoch detections are separated by 1.9" and 5.7 pix
The object was found in VSX22" ZTF J213602.80+605020.8
Type: RS
# Max. Min./Amp. JD0 Period
19.002 r Y 0.155 r 2458247.98460 3.691047200000
ATTENTION: measured mag 11.99 is 6.9 mag brighter than the VSX record maximum brightness 18.85 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:00.31 +60:50:32.9: 12.97 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:00.31 +60:50:32.9: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J213602.80+605020.8,2461239.8909,11.99,0.05,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
ZTF J213602.80+605020.8 20260718.3909 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 07 18.3909 2461239.8909 12.44 21:36:03.66 +60:35:45.0
101.09882 6.29684 galactic Cep Second-epoch detections are separated by 1.5" and 5.5 pix
The object was found in VSX 3" Gaia DR3 2215773048195662592
Type: L
# Max. Min./Amp. JD0 Period
18.140 G 18.380 G
ATTENTION: measured mag 12.44 is 5.7 mag brighter than the VSX record maximum brightness 18.14 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:03.66 +60:35:45.0: 13.56 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:03.66 +60:35:45.0: 13.84 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2215773048195662592,2461239.8909,12.44,0.05,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 2215773048195662592 20260718.3909 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 11.99 19:49:36.85 +66:34:23.1
98.87735 19.24074 galactic Dra Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:49:36.85 +66:34:23.1 (user input) | T | P | (position from user input) J-Ks=0.581+/-0.031 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 19:49:36.85 +66:34:23.1: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 19:49:36.85 +66:34:23.1: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461239.8909,11.99,0.05,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 20260718.3909 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 07 18.3909 2461239.8909 11.90 21:36:52.34 +60:40:02.8
101.22132 6.28284 galactic Cep Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:52.34 +60:40:02.8 (user input) | T | P | (position from user input) J-Ks=0.742+/-0.034 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:52.34 +60:40:02.8: 12.92 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:52.34 +60:40:02.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 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,2461239.8909,11.90,0.05,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 20260718.3909 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 11.63 21:37:12.25 +60:28:04.8
101.11699 6.10768 galactic Cep Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J324.2973+60.4678 | 21:37:12.25 +60:28:04.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:37:12.25 +60:28:04.8: 12.57 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:37:12.25 +60:28:04.8: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J324.2973+60.4678,2461239.8909,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J324.2973+60.4678 20260718.3909 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.37 21:34:15.56 +60:46:07.1
101.05307 6.57331 galactic Cep Second-epoch detections are separated by 1.5" and 5.4 pix
The object was found in VSX22" Gaia DR3 2191774901250929024
Type: ROT
# Max. Min./Amp. JD0 Period
15.820 G 15.860 G K
ATTENTION: measured mag 12.37 is 3.5 mag brighter than the VSX record maximum brightness 15.82 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:15.56 +60:46:07.1: 13.36 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:15.56 +60:46:07.1: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2191774901250929024,2461239.8909,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2191774901250929024 20260718.3909 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 11.98 21:36:43.40 +60:31:26.3
101.11069 6.18891 galactic Cep Second-epoch detections are separated by 0.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:43.40 +60:31:26.3 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.031 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:43.40 +60:31:26.3: 12.92 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:43.40 +60:31:26.3: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 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,2461239.8909,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3909 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.26 21:36:59.36 +60:44:27.6
101.28171 6.32770 galactic Cep Second-epoch detections are separated by 0.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:59.36 +60:44:27.6 (user input) | T | P | (position from user input) J-Ks=1.082+/-0.031 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:59.36 +60:44:27.6: 13.42 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:59.36 +60:44:27.6: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3909 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.41 21:34:15.90 +60:51:08.8
101.11088 6.63435 galactic Cep Second-epoch detections are separated by 0.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2215841488493245056 | 21:34:15.90 +60:51:08.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.719+/-0.037 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:15.90 +60:51:08.8: 13.38 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:15.90 +60:51:08.8: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2215841488493245056,2461239.8909,12.41,0.05,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
Large-amplitude variable Gaia DR2 2215841488493245056 20260718.3909 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 11.99 21:36:22.56 +60:35:17.6
101.12240 6.26516 galactic Cep Second-epoch detections are separated by 0.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:22.56 +60:35:17.6 (user input) | T | P | (position from user input) J-Ks=0.456+/-0.042 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:22.56 +60:35:17.6: 12.89 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:22.56 +60:35:17.6: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.00 +/- 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,2461239.8909,11.99,0.05,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 20260718.3909 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 07 18.3909 2461239.8909 12.07 19:49:31.98 +66:29:17.7
98.79188 19.21339 galactic Dra Second-epoch detections are separated by 2.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:49:31.98 +66:29:17.7 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.030 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 19:49:31.98 +66:29:17.7: 13.16 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 19:49:31.98 +66:29:17.7: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 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,2461239.8909,12.07,0.05,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 20260718.3909 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 07 18.3909 2461239.8909 12.36 21:35:49.93 +60:46:14.0
101.19660 6.44472 galactic Cep Second-epoch detections are separated by 2.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:35:49.93 +60:46:14.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:35:49.93 +60:46:14.0: 13.39 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:35:49.93 +60:46:14.0: 13.69 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3909 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 11.96 21:34:40.73 +60:41:50.7
101.04233 6.48620 galactic Cep Second-epoch detections are separated by 0.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:40.73 +60:41:50.7 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.035 (G)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:40.73 +60:41:50.7: 12.84 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:40.73 +60:41:50.7: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3909 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.06 21:34:15.38 +60:50:19.3
101.10069 6.62497 galactic Cep Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:34:15.38 +60:50:19.3 (user input) | T | P | (position from user input) J-Ks=0.761+/-0.036 (K)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:15.38 +60:50:19.3: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:15.38 +60:50:19.3: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,12.06,0.05,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 20260718.3909 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.3909 2461239.8909 12.22 21:36:35.16 +61:00:56.7
101.43110 6.56404 galactic Cep Second-epoch detections are separated by 2.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 21:36:35.16 +61:00:56.7 (user input) | T | P | (position from user input) J-Ks=1.061+/-0.034 (M)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:35.16 +61:00:56.7: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:35.16 +61:00:56.7: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.8909,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.3909 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461201.88816286 10.06.2026 09:18:47.271 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
First image: 2461201.88816286 10.06.2026 09:18:47.271 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
Last image: 2461239.89127184 18.07.2026 09:23:15.887 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.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.: -7.58
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: 74 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): 19855
Objects passed selection criteria: 19763
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: 12291.2
Average stars matched: 11380 (92.5862 %)
Memory usage VmPeak: 128056 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 05:32:02 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: 2461201.88816286 10.06.2026 09:18:47.271 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
First image: 2461201.88816286 10.06.2026 09:18:47.271 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
Last image: 2461239.89127184 18.07.2026 09:23:15.887 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 77
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 93 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): 125128
Objects passed selection criteria: 124722
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 83046
Average stars matched: 78090.8 (94.0331 %)
Memory usage VmPeak: 2092088 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 05:39:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
SExtractor catalog cache: saved Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.cat to cache
SExtractor catalog cache: saved Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.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/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.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: 2461239.89058000
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits exists and is non-empty
Saving wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits to local_wcs_cache/
'wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits' -> 'local_wcs_cache/wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits'
wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits exists and is non-empty
Saving wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits to local_wcs_cache/
'wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits' -> 'local_wcs_cache/wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits'
wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits exists and is non-empty
Saving wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits to local_wcs_cache/
'wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits' -> 'local_wcs_cache/wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits'
wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits exists and is non-empty
Saving wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits to local_wcs_cache/
'wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits' -> 'local_wcs_cache/wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits (1st reference image)
verification OK: wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 20:34:14.356 +61:58:30.49 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits (1st new image)
verification OK: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
Image size: 941.1'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: 20:34:40.940 +61:55:35.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:34:14.356 +61:58:30.49
Second-epoch image center 20:34:40.940 +61:55:35.46
Angular distance between the image centers 0.0713 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits (2nd new image)
verification OK: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
Image size: 941.1'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: 20:34:38.629 +61:56:06.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:34:14.356 +61:58:30.49
Second-epoch image center 20:34:38.629 +61:56:06.79
Angular distance between the image centers 0.0621 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 20:34:40.940 +61:55:35.46
Second-epoch second image center 20:34:38.629 +61:56:06.79
Angular distance between the image centers 0.00981 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits &> /tmp/tmp.os2wLkAqnb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits &> /tmp/tmp.PKKsHjKGE6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits &> /tmp/tmp.8j0qRhbHTM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits &> /tmp/tmp.68iZaNf0lT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.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_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits and wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits and wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat
Found non-empty wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits and wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat
The reference image (wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits) and catalog (wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat) found
'wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat' -> 'wcsmag.cat'
Read 20528 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 289.2411 to 328.0401 deg, Dec +55.9437 to +67.2364 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 289.2411 to 328.0401 deg, Dec 55.9437 to 67.2364 deg
Loaded 16905 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): 10453 out of 11206 total matches.
Matched with Tycho-2 11206 out of 20528 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.666700
a=0.000000 b=1.000000 c=22.666700
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 20528 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 289.2411 to 328.0401 deg, Dec +55.9437 to +67.2364 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 289.2411 to 328.0401 deg, Dec 55.9437 to 67.2364 deg
Loaded 16905 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): 10453 out of 11206 total matches.
Matched with Tycho-2 11206 out of 20528 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits:
Forced-photometry filter: calibrated wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits -> calib.txt_param_ref_wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits (aperture=6.4)
Read 23396 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 289.2192 to 328.1618 deg, Dec +56.0064 to +67.2894 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 289.2192 to 328.1618 deg, Dec 56.0064 to 67.2894 deg
Loaded 16904 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): 10512 out of 11327 total matches.
Matched with Tycho-2 11327 out of 23396 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits:
Forced-photometry filter: calibrated wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits -> calib.txt_param_ref_wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
2.3 pix Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
2.5 pix fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
2.4 pix fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
2.4 pix wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
2.3 pix wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
Limiting magnitude estimates:
15.1 mag. Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
15.2 mag. Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
12.8 mag. fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
13.2 mag. fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.os2wLkAqnb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits' -> 'wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
WCS_IMAGE_NAME=wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
WCS-calibrated image found: wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
Checking if the catalog wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits alredy exist and is non-empty...
Catalog wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
WCS catalog name: wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1743, bad_region=0, passed=20528
Got 20528 stars (including 18763 good ones) from the SExtractor catalog wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat
util/solve_plate_with_UCAC5 got 20528 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 19971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 19970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 19970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits N_match=971 sigma_overall_arcsec=0.634 sigma_q1_arcsec=0.478 sigma_q2_arcsec=0.702 sigma_q3_arcsec=0.514 sigma_q4_arcsec=0.734 n_q1=248 n_q2=238 n_q3=187 n_q4=298 worst_quadrant_to_overall_ratio=1.158
The image catalog is written to wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits -region wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PKKsHjKGE6 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits' -> 'wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
WCS_IMAGE_NAME=wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
WCS-calibrated image found: wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
Checking if the catalog wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits alredy exist and is non-empty...
Catalog wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
WCS catalog name: wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1893, bad_region=0, passed=23394
Got 23394 stars (including 21481 good ones) from the SExtractor catalog wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat
util/solve_plate_with_UCAC5 got 23394 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 22606 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 730 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 22606 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 22606 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits N_match=971 sigma_overall_arcsec=0.655 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.917 sigma_q3_arcsec=0.566 sigma_q4_arcsec=0.777 n_q1=235 n_q2=265 n_q3=171 n_q4=300 worst_quadrant_to_overall_ratio=1.399
The image catalog is written to wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits -region wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8j0qRhbHTM (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
WCS_IMAGE_NAME=wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
WCS-calibrated image found: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
Checking if the catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
WCS catalog name: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=122, bad_region=0, passed=2565
Got 2565 stars (including 2437 good ones) from the SExtractor catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat
util/solve_plate_with_UCAC5 got 2565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 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 727 to 787 (Dec 55.5 to 67.2)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2432 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 727 to 787 (Dec 55.5 to 67.2)
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: 956 matched stars entering correct_measured_positions(), 2432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits N_match=956 sigma_overall_arcsec=0.410 sigma_q1_arcsec=0.432 sigma_q2_arcsec=0.466 sigma_q3_arcsec=0.363 sigma_q4_arcsec=0.379 n_q1=244 n_q2=147 n_q3=322 n_q4=243 worst_quadrant_to_overall_ratio=1.136
The image catalog is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits -region wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.68iZaNf0lT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
WCS_IMAGE_NAME=wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
WCS-calibrated image found: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
Checking if the catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
WCS catalog name: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=118, bad_region=0, passed=3039
Got 3039 stars (including 2917 good ones) from the SExtractor catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat
util/solve_plate_with_UCAC5 got 3039 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 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 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 2933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 2933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 2933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits N_match=960 sigma_overall_arcsec=0.385 sigma_q1_arcsec=0.395 sigma_q2_arcsec=0.411 sigma_q3_arcsec=0.397 sigma_q4_arcsec=0.360 n_q1=239 n_q2=261 n_q3=234 n_q4=226 worst_quadrant_to_overall_ratio=1.068
The image catalog is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits -region wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits sigma_overall=0.634 worst_q_ratio=1.158
ref2=Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits sigma_overall=0.655 worst_q_ratio=1.399
new1=fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits sigma_overall=0.410 worst_q_ratio=1.136
new2=fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits sigma_overall=0.385 worst_q_ratio=1.068
reference average sigma_overall=0.6445 worst_q_ratio=1.2785
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165_astrometric_residuals.png (971 matched stars from wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.53 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248_astrometric_residuals.png (971 matched stars from wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.58 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312_astrometric_residuals.png (956 matched stars from wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313_astrometric_residuals.png (960 matched stars from wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits'
Saving fully-calibrated image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits'
Preparing the HTML report for the field Cep-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cep-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
SExtractor catalog cache: saved Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.cat to cache
SExtractor catalog cache: saved Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
Creating symlink local_wcs_cache/wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.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_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits exists and is non-empty
wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits exists and is non-empty
wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits exists and is non-empty
wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits (1st reference image)
verification OK: wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 20:34:14.356 +61:58:30.49 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits (1st new image)
verification OK: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
Image size: 941.1'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: 20:34:40.940 +61:55:35.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:34:14.356 +61:58:30.49
Second-epoch image center 20:34:40.940 +61:55:35.46
Angular distance between the image centers 0.0713 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits (2nd new image)
verification OK: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
Image size: 941.1'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: 20:34:38.629 +61:56:06.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:34:14.356 +61:58:30.49
Second-epoch image center 20:34:38.629 +61:56:06.79
Angular distance between the image centers 0.0621 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 20:34:40.940 +61:55:35.46
Second-epoch second image center 20:34:38.629 +61:56:06.79
Angular distance between the image centers 0.00981 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits &> /tmp/tmp.p61t8nKv4d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits &> /tmp/tmp.x7NY5PVLgI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits &> /tmp/tmp.wVuVHBzkyQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits &> /tmp/tmp.iJ8eaFN9NH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.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_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits and wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits and wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat
Found non-empty wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits and wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat
The reference image (wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits) and catalog (wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat) found
'wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat' -> 'wcsmag.cat'
Read 138493 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 289.1739 to 328.0664 deg, Dec +55.8690 to +67.2400 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 289.1739 to 328.0664 deg, Dec 55.8690 to 67.2400 deg
Loaded 17126 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): 9005 out of 11664 total matches.
Matched with Tycho-2 11664 out of 138493 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.522700
a=0.000000 b=1.000000 c=22.522700
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 138493 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 289.1739 to 328.0664 deg, Dec +55.8690 to +67.2400 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 289.1739 to 328.0664 deg, Dec 55.8690 to 67.2400 deg
Loaded 17126 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): 9005 out of 11664 total matches.
Matched with Tycho-2 11664 out of 138493 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits:
Forced-photometry filter: calibrated wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits -> calib.txt_param_ref_wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits (aperture=4.8)
Read 143162 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 289.1701 to 328.1617 deg, Dec +55.9610 to +67.2894 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 289.1701 to 328.1617 deg, Dec 55.9610 to 67.2894 deg
Loaded 17017 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): 8934 out of 11551 total matches.
Matched with Tycho-2 11551 out of 143162 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits:
Forced-photometry filter: calibrated wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits -> calib.txt_param_ref_wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 47 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
2.2 pix Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
2.4 pix fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
2.3 pix fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
2.1 pix wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
2.2 pix wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
Limiting magnitude estimates:
15.3 mag. Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
15.4 mag. Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
13.0 mag. fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
13.0 mag. fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.p61t8nKv4d (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits' -> 'wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
WCS_IMAGE_NAME=wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
WCS-calibrated image found: wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
Checking if the catalog wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits alredy exist and is non-empty...
Catalog wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits
WCS catalog name: wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=14626, bad_region=0, passed=138447
Got 138447 stars (including 123641 good ones) from the SExtractor catalog wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat
util/solve_plate_with_UCAC5 got 138447 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 135499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 729 to 788 (Dec 55.9 to 67.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 135501 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 135502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits N_match=971 sigma_overall_arcsec=0.623 sigma_q1_arcsec=0.513 sigma_q2_arcsec=0.704 sigma_q3_arcsec=0.550 sigma_q4_arcsec=0.684 n_q1=227 n_q2=248 n_q3=187 n_q4=309 worst_quadrant_to_overall_ratio=1.129
The image catalog is written to wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits -region wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.x7NY5PVLgI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits' -> 'wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
WCS_IMAGE_NAME=wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
WCS-calibrated image found: wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
Checking if the catalog wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits alredy exist and is non-empty...
Catalog wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat corresponding to the image wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits
WCS catalog name: wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=61, blended=16261, bad_region=1, passed=143101
Got 143101 stars (including 126666 good ones) from the SExtractor catalog wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat
util/solve_plate_with_UCAC5 got 143101 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 139951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 139951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 139951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 971 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits N_match=971 sigma_overall_arcsec=0.653 sigma_q1_arcsec=0.431 sigma_q2_arcsec=0.855 sigma_q3_arcsec=0.580 sigma_q4_arcsec=0.759 n_q1=225 n_q2=261 n_q3=189 n_q4=296 worst_quadrant_to_overall_ratio=1.308
The image catalog is written to wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits -region wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.wVuVHBzkyQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
WCS_IMAGE_NAME=wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
WCS-calibrated image found: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
Checking if the catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
WCS catalog name: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=736, bad_region=29, passed=24786
Got 24786 stars (including 23968 good ones) from the SExtractor catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat
util/solve_plate_with_UCAC5 got 24786 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 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 727 to 788 (Dec 55.4 to 67.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 23281 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 727 to 788 (Dec 55.4 to 67.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 23282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 23282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits N_match=959 sigma_overall_arcsec=0.394 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.463 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.375 n_q1=248 n_q2=154 n_q3=321 n_q4=236 worst_quadrant_to_overall_ratio=1.175
The image catalog is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits -region wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.iJ8eaFN9NH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
WCS_IMAGE_NAME=wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
WCS-calibrated image found: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
Checking if the catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat corresponding to the image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
WCS catalog name: wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=900, bad_region=33, passed=28369
Got 28369 stars (including 27385 good ones) from the SExtractor catalog wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat
util/solve_plate_with_UCAC5 got 28369 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 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 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 27118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 27117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 27117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits N_match=960 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.400 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.334 n_q1=243 n_q2=259 n_q3=230 n_q4=228 worst_quadrant_to_overall_ratio=1.050
The image catalog is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits -region wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-22-16_20.00sec_-0.00C_LIGHTs_0312.fits
Saving fully-calibrated image wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-18_CI_Cep-05-Q1b1x1_042401_TTUQ1b1x1_1912291_39fiogcz/wcs_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313.fits
Preparing the HTML report for the field Cep-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:27:22.40 +57:18:06.6: 12.34 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:40:53.94 +62:05:05.2: 12.66 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:49:39.69 +65:15:03.7: 11.45 +/- 0.01 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 20:24:25.45 +60:16:26.2: 11.33 +/- 0.01 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:25:01.86 +56:01:06.0: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:25:01.86 +56:01:06.0: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 21:25:01.86 +56:01:06.0: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 19:50:33.21 +66:35:36.6: 12.99 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:27:22.40 +57:18:06.6: 12.18 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:40:53.94 +62:05:05.2: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Forced photometry filter REJECTED candidate at 21:27:22.40 +57:18:06.6: ref_mag=12.25 +/- 0.01 new_mean_mag=12.2260 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:40:53.94 +62:05:05.2: ref_mag=12.75 +/- 0.02 new_mean_mag=12.2352 delta=0.52 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:49:39.69 +65:15:03.7: 11.61 +/- 0.01 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 20:24:25.45 +60:16:26.2: 11.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Forced photometry filter REJECTED candidate at 21:49:39.69 +65:15:03.7: ref_mag=11.53 +/- 0.01 new_mean_mag=11.6789 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 11.29 +/- 0.00
Forced photometry filter REJECTED candidate at 20:24:25.45 +60:16:26.2: ref_mag=11.29 +/- 0.00 new_mean_mag=12.4257 delta=-1.14 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:37:38.20 +60:41:33.5: 13.49 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 19:49:13.38 +66:25:53.7: 13.06 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:41.78 +60:44:30.0: 12.81 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 19:50:33.21 +66:35:36.6: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter REJECTED candidate at 19:50:33.21 +66:35:36.6: ref_mag=12.96 +/- 0.02 new_mean_mag=12.1067 delta=0.85 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:37:38.20 +60:41:33.5: 13.51 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 19:49:13.38 +66:25:53.7: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 21:37:38.20 +60:41:33.5: ref_mag=13.50 +/- 0.04 new_mean_mag=12.3872 delta=1.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:49:13.38 +66:25:53.7: ref_mag=13.00 +/- 0.02 new_mean_mag=12.1224 delta=0.88 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:41.78 +60:44:30.0: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 21:34:41.78 +60:44:30.0: ref_mag=12.91 +/- 0.02 new_mean_mag=11.8998 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:35:35.39 +60:51:21.1: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:37:02.75 +60:39:04.7: 12.75 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:35:35.39 +60:51:21.1: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter KEPT candidate at 21:35:35.39 +60:51:21.1: ref_mag=13.39 +/- 0.03 new_mean_mag=12.2352 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:34.25 +60:32:23.2: 13.00 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:37:13.38 +60:31:37.4: 13.45 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:37:02.75 +60:39:04.7: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry filter KEPT candidate at 21:37:02.75 +60:39:04.7: ref_mag=12.83 +/- 0.02 new_mean_mag=11.8573 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:34.25 +60:32:23.2: 13.20 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:26.58 +60:47:37.7: 13.25 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 21:34:34.25 +60:32:23.2: ref_mag=13.09 +/- 0.02 new_mean_mag=12.0744 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:37:13.38 +60:31:37.4: 13.69 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:35:47.32 +60:32:38.4: 13.61 +/- 0.06 detection
Forced photometry filter KEPT candidate at 21:37:13.38 +60:31:37.4: ref_mag=13.55 +/- 0.04 new_mean_mag=12.3940 delta=1.16 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:00.31 +60:50:32.9: 12.97 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:26.58 +60:47:37.7: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Forced photometry filter KEPT candidate at 21:34:26.58 +60:47:37.7: ref_mag=13.34 +/- 0.03 new_mean_mag=12.1927 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:35:47.32 +60:32:38.4: 13.66 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:00.31 +60:50:32.9: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Forced photometry filter KEPT candidate at 21:35:47.32 +60:32:38.4: ref_mag=13.64 +/- 0.04 new_mean_mag=12.4366 delta=1.20 (need > 0.90)
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 21:36:00.31 +60:50:32.9: ref_mag=13.05 +/- 0.02 new_mean_mag=11.9935 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:03.66 +60:35:45.0: 13.56 +/- 0.06 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:03.66 +60:35:45.0: 13.84 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter KEPT candidate at 21:36:03.66 +60:35:45.0: ref_mag=13.68 +/- 0.04 new_mean_mag=12.4115 delta=1.26 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 19:49:36.85 +66:34:23.1: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 19:49:36.85 +66:34:23.1: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Forced photometry filter KEPT candidate at 19:49:36.85 +66:34:23.1: ref_mag=12.91 +/- 0.02 new_mean_mag=11.9964 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:37:00.06 +60:36:57.8: 12.57 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:37:00.06 +60:36:57.8: 12.71 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:52.34 +60:40:02.8: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Forced photometry filter KEPT candidate at 21:37:00.06 +60:36:57.8: ref_mag=12.64 +/- 0.02 new_mean_mag=11.6932 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:52.34 +60:40:02.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 21:36:52.34 +60:40:02.8: ref_mag=13.00 +/- 0.02 new_mean_mag=11.8741 delta=1.13 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:37:12.25 +60:28:04.8: 12.57 +/- 0.02 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:37:12.25 +60:28:04.8: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter KEPT candidate at 21:37:12.25 +60:28:04.8: ref_mag=12.66 +/- 0.02 new_mean_mag=11.6134 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:15.56 +60:46:07.1: 13.36 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:43.40 +60:31:26.3: 12.92 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:15.56 +60:46:07.1: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 21:34:15.56 +60:46:07.1: ref_mag=13.42 +/- 0.03 new_mean_mag=12.3552 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:43.40 +60:31:26.3: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 21:36:43.40 +60:31:26.3: ref_mag=13.02 +/- 0.02 new_mean_mag=11.9351 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:59.36 +60:44:27.6: 13.42 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:59.36 +60:44:27.6: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Forced photometry filter KEPT candidate at 21:36:59.36 +60:44:27.6: ref_mag=13.47 +/- 0.04 new_mean_mag=12.2566 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:15.90 +60:51:08.8: 13.38 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:22.56 +60:35:17.6: 12.89 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:35:49.93 +60:46:14.0: 13.39 +/- 0.05 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 19:49:31.98 +66:29:17.7: 13.16 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:15.90 +60:51:08.8: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry filter KEPT candidate at 21:34:15.90 +60:51:08.8: ref_mag=13.51 +/- 0.04 new_mean_mag=12.3557 delta=1.16 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:22.56 +60:35:17.6: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 21:36:22.56 +60:35:17.6: ref_mag=13.00 +/- 0.02 new_mean_mag=11.9636 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 19:49:31.98 +66:29:17.7: 13.10 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:35:49.93 +60:46:14.0: 13.69 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 21:35:49.93 +60:46:14.0: ref_mag=13.51 +/- 0.04 new_mean_mag=12.3320 delta=1.17 (need > 0.90)
Forced photometry filter KEPT candidate at 19:49:31.98 +66:29:17.7: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1344 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:40.73 +60:41:50.7: 12.84 +/- 0.03 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:34:15.38 +60:50:19.3: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-10_04-18-47_20.00sec_5.00C_LIGHT_0165.fits at 21:36:35.16 +61:00:56.7: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:40.73 +60:41:50.7: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter KEPT candidate at 21:34:40.73 +60:41:50.7: ref_mag=12.93 +/- 0.02 new_mean_mag=11.8850 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:34:15.38 +60:50:19.3: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter KEPT candidate at 21:34:15.38 +60:50:19.3: ref_mag=13.12 +/- 0.03 new_mean_mag=12.0455 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cep-05-Q1b1x1_2026-06-11_03-20-23_20.00sec_5.00C_LIGHT_0248.fits at 21:36:35.16 +61:00:56.7: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry filter KEPT candidate at 21:36:35.16 +61:00:56.7: ref_mag=13.19 +/- 0.03 new_mean_mag=12.1847 delta=1.01 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out70747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out68439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94025.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 42s
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: 14s
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Considering the candidate 166435_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 166435_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 21:23:09.24 +61:43:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166440_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 166440_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
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Considering the candidate 166446_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 166446_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 166453_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 166453_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
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Considering the candidate 166455_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 166455_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 166460_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 166460_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 21:31:53.14 +64:41:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166653_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 166653_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
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Considering the candidate 167124_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 167124_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
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Considering the candidate 167258_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 167258_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
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Considering the candidate 93196_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 93196_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
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Considering the candidate 94478_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 94478_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
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Considering the candidate 72101_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 72101_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 71382_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 71382_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 54811_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 54811_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 21:35:06.94 +59:34:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73485_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 73485_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 75870_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 75870_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
Rejecting candidate due to large distance (33.9") between the two second-epoch detections
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Considering the candidate 43062_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 43062_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 21:32:10.56 +58:49:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71106_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 71106_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 69643_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 69643_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 68439_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 68439_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 49900_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 49900_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 21:32:49.05 +59:17:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72099_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 72099_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 69174_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 69174_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 73543_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 73543_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 53446_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 53446_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 21:34:45.21 +59:29:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85529_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 85529_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
Rejecting candidate due to large distance (35.6") between the two second-epoch detections
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Considering the candidate 120943_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 120943_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 70103_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 70103_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 93247_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 93247_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 46864_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 46864_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 70747_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 70747_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 21:37:00.06 +60:36:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 0.649 2215774074686572672 324.25061581839 +60.61607362141 12.5450 11.9278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71335_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 71335_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 68658_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 68658_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 71723_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 71723_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 69270_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 69270_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 72461_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 72461_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 120385_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 120385_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
Rejecting candidate due to large distance (30.8") between the two second-epoch detections
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Considering the candidate 56025_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 56025_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 21:34:39.19 +59:40:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72898_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 72898_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 70078_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 70078_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 94025_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 94025_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 72365_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 72365_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 71900_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 71900_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 21:36:01.08 +60:43:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54083_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
The candidate 54083_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313 did not pass the final checks
**** FOUND 21:35:07.25 +59:31:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70869_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 70869_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 72706_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 72706_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
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Considering the candidate 76153_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
Preparing report for the candidate 76153_fd_Cep-05-Q1b1x1_2026-07-18_04-23-15_20.00sec_-0.00C_LIGHTs_0313
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 59s
Prepared the HTML report for the field Cep-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:34:34.25 +60:32:23.2
21:37:12.25 +60:28:04.8
21:35:47.32 +60:32:38.4
21:36:43.40 +60:31:26.3
21:37:13.38 +60:31:37.4
21:36:22.56 +60:35:17.6
21:36:03.66 +60:35:45.0
21:34:40.73 +60:41:50.7
21:37:02.75 +60:39:04.7
21:36:52.34 +60:40:02.8
21:34:41.78 +60:44:30.0
21:34:15.56 +60:46:07.1
21:34:26.58 +60:47:37.7
21:37:38.20 +60:41:33.5
21:35:49.93 +60:46:14.0
21:36:59.36 +60:44:27.6
21:34:15.38 +60:50:19.3
21:34:15.90 +60:51:08.8
21:35:35.39 +60:51:21.1
21:36:00.31 +60:50:32.9
21:36:35.16 +61:00:56.7
19:49:36.85 +66:34:23.1
19:49:31.98 +66:29:17.7
########### Completed Cep-05-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 ####
21:37:38.20 +60:41:33.5
21:34:41.78 +60:44:30.0
21:35:35.39 +60:51:21.1
21:37:02.75 +60:39:04.7
21:37:13.38 +60:31:37.4
21:34:34.25 +60:32:23.2
21:34:26.58 +60:47:37.7
21:35:47.32 +60:32:38.4
21:36:00.31 +60:50:32.9
21:36:03.66 +60:35:45.0
19:49:36.85 +66:34:23.1
21:36:52.34 +60:40:02.8
21:37:12.25 +60:28:04.8
21:34:15.56 +60:46:07.1
21:36:43.40 +60:31:26.3
21:36:59.36 +60:44:27.6
21:34:15.90 +60:51:08.8
21:36:22.56 +60:35:17.6
19:49:31.98 +66:29:17.7
21:35:49.93 +60:46:14.0
21:34:40.73 +60:41:50.7
21:34:15.38 +60:50:19.3
21:36:35.16 +61:00:56.7
###################################################################################
21:37:38.20 +60:41:33.5 -- not an asteroid (will add it to exclusion list)
21:34:41.78 +60:44:30.0 -- not an asteroid (will add it to exclusion list)
21:35:35.39 +60:51:21.1 -- not an asteroid (will add it to exclusion list)
21:37:02.75 +60:39:04.7 -- not an asteroid (will add it to exclusion list)
21:37:13.38 +60:31:37.4 -- not an asteroid (will add it to exclusion list)
21:34:34.25 +60:32:23.2 -- not an asteroid (will add it to exclusion list)
21:34:26.58 +60:47:37.7 -- not an asteroid (will add it to exclusion list)
21:35:47.32 +60:32:38.4 -- not an asteroid (will add it to exclusion list)
21:36:00.31 +60:50:32.9 -- not an asteroid (will add it to exclusion list)
21:36:03.66 +60:35:45.0 -- not an asteroid (will add it to exclusion list)
19:49:36.85 +66:34:23.1 -- not an asteroid (will add it to exclusion list)
21:36:52.34 +60:40:02.8 -- not an asteroid (will add it to exclusion list)
21:37:12.25 +60:28:04.8 -- not an asteroid (will add it to exclusion list)
21:34:15.56 +60:46:07.1 -- not an asteroid (will add it to exclusion list)
21:36:43.40 +60:31:26.3 -- not an asteroid (will add it to exclusion list)
21:36:59.36 +60:44:27.6 -- not an asteroid (will add it to exclusion list)
21:34:15.90 +60:51:08.8 -- not an asteroid (will add it to exclusion list)
21:36:22.56 +60:35:17.6 -- not an asteroid (will add it to exclusion list)
19:49:31.98 +66:29:17.7 -- not an asteroid (will add it to exclusion list)
21:35:49.93 +60:46:14.0 -- not an asteroid (will add it to exclusion list)
21:34:40.73 +60:41:50.7 -- not an asteroid (will add it to exclusion list)
21:34:15.38 +60:50:19.3 -- not an asteroid (will add it to exclusion list)
21:36:35.16 +61:00:56.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:49:31.98 +66:29:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:36.85 +66:34:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:15.38 +60:50:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:15.56 +60:46:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:15.90 +60:51:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:26.58 +60:47:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:34.25 +60:32:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:40.73 +60:41:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:41.78 +60:44:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:35.39 +60:51:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:47.32 +60:32:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:35:49.93 +60:46:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:00.31 +60:50:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:03.66 +60:35:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:22.56 +60:35:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:35.16 +61:00:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:43.40 +60:31:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:52.34 +60:40:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:36:59.36 +60:44:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:02.75 +60:39:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:12.25 +60:28:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:13.38 +60:31:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:37:38.20 +60:41:33.5 -- 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)
19:49:31.98 +66:29:17.7 -- not a known variable star
19:49:36.85 +66:34:23.1 -- not a known variable star
21:34:15.38 +60:50:19.3 -- not a known variable star
21:34:15.56 +60:46:07.1 -- a known variable star
21:34:15.90 +60:51:08.8 -- not a known variable star
21:34:26.58 +60:47:37.7 -- not a known variable star
21:34:34.25 +60:32:23.2 -- not a known variable star
21:34:40.73 +60:41:50.7 -- not a known variable star
21:34:41.78 +60:44:30.0 -- not a known variable star
21:35:35.39 +60:51:21.1 -- not a known variable star
21:35:47.32 +60:32:38.4 -- not a known variable star
21:35:49.93 +60:46:14.0 -- not a known variable star
21:36:00.31 +60:50:32.9 -- a known variable star
21:36:03.66 +60:35:45.0 -- a known variable star
21:36:22.56 +60:35:17.6 -- not a known variable star
21:36:35.16 +61:00:56.7 -- not a known variable star
21:36:43.40 +60:31:26.3 -- not a known variable star
21:36:52.34 +60:40:02.8 -- not a known variable star
21:36:59.36 +60:44:27.6 -- not a known variable star
21:37:02.75 +60:39:04.7 -- a known variable star
21:37:12.25 +60:28:04.8 -- not a known variable star
21:37:13.38 +60:31:37.4 -- not a known variable star
21:37:38.20 +60:41:33.5 -- not a known variable star
Found 19 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
23 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
19:49:31.98 +66:29:17.7
19:49:36.85 +66:34:23.1
21:34:15.38 +60:50:19.3
21:34:15.56 +60:46:07.1
21:34:15.90 +60:51:08.8
21:34:26.58 +60:47:37.7
21:34:34.25 +60:32:23.2
21:34:40.73 +60:41:50.7
21:34:41.78 +60:44:30.0
21:35:35.39 +60:51:21.1
21:35:47.32 +60:32:38.4
21:35:49.93 +60:46:14.0
21:36:00.31 +60:50:32.9
21:36:03.66 +60:35:45.0
21:36:22.56 +60:35:17.6
21:36:35.16 +61:00:56.7
21:36:43.40 +60:31:26.3
21:36:52.34 +60:40:02.8
21:36:59.36 +60:44:27.6
21:37:02.75 +60:39:04.7
21:37:12.25 +60:28:04.8
21:37:13.38 +60:31:37.4
21:37:38.20 +60:41:33.5
21:37:00.06 +60:36:57.8
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461239.89058000 -observatory V36
07:12:21.05 +17:31:55.1 Mercury (4.0mag)
10:44:34.31 +09:02:11.5 Venus (-4.2mag)
04:48:00.32 +22:19:03.1 Mars (1.3mag)
08:24:00.02 +19:47:49.9 Jupiter (-1.8mag)
00:56:32.03 +03:22:20.3 Saturn (0.7mag)
04:08:42.19 +20:48:59.9 Uranus (5.8mag)
00:16:55.50 +00:19:34.9 Neptune (7.7mag)
20:30:09.63 -23:21:32.6 Pluto (14.4mag)
11:15:05.89 +02:20:29.0 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 361 Jul 18 05:32 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461239.89058000:
08:23:55.47 +19:48:07.8 Io (6.0mag)
08:24:11.17 +19:47:07.0 Europa (6.3mag)
08:24:15.53 +19:46:48.4 Ganymede (5.6mag)
08:23:34.25 +19:49:30.1 Callisto (6.8mag)
08:22:10.52 +19:35:36.6 Himalia (15.7mag)
08:23:58.27 +19:47:57.7 Thebe (16.6mag)
08:21:31.57 +19:38:19.1 Elara (17.7mag)
08:27:46.00 +19:37:43.7 Pasiphae (17.9mag)
08:28:29.77 +19:54:08.3 Carme (19.0mag)
00:56:41.97 +03:22:29.0 Titan (8.5mag)
00:56:30.83 +03:22:31.0 Rhea (9.8mag)
00:55:57.56 +03:20:09.9 Iapetus (11.2mag)
00:56:19.07 +03:22:10.0 Hyperion (14.5mag)
00:56:21.99 +03:18:24.1 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 18 05:32 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461239.89058000:
17:58:38.43 -31:00:30.0 JWST
16:29:44.30 +46:20:29.4 Chandra
05:25:33.72 +42:12:54.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 18 05:32 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461239.89058000 -observatory V36
02:47:29.51 +15:21:12.8 17.8mag P/1996 R2 (Lagerkvist)
18:12:04.28 -34:32:42.4 13.8mag P/2010 H2 (Vales)
06:33:41.52 -68:17:16.2 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:03:32.89 +32:35:13.4 17.6mag C/2017 K2 (PANSTARRS)
02:28:42.87 +21:24:48.9 15.8mag P/2021 N1 (ZTF)
22:54:25.91 +32:13:23.1 17.3mag C/2022 E2 (ATLAS)
06:21:28.23 +26:50:44.3 16.7mag C/2022 N2 (PANSTARRS)
10:02:35.53 +29:25:06.6 16.9mag C/2022 QE78 (ATLAS)
09:14:58.20 +05:08:05.4 17.9mag C/2022 R6 (PANSTARRS)
15:11:02.51 -11:35:18.1 17.8mag P/2023 B1 (PANSTARRS)
21:39:06.73 +67:28:50.6 17.9mag C/2023 H5 (Lemmon)
16:15:58.96 -10:54:32.1 14.0mag C/2023 R1 (PANSTARRS)
08:14:50.49 +66:09:22.7 17.9mag C/2024 A1 (ATLAS)
07:43:11.42 +30:24:01.1 14.8mag C/2024 E1 (Wierzchos)
15:12:45.36 +15:30:08.8 17.6mag C/2024 G6 (ATLAS)
19:30:49.82 +40:50:04.1 13.7mag C/2024 J3 (ATLAS)
21:38:44.50 +47:08:54.8 17.8mag C/2024 R4 (PANSTARRS)
04:57:08.17 -13:27:52.6 15.7mag C/2024 T5 (ATLAS)
06:41:06.50 +27:43:33.8 18.0mag C/2025 J1 (Borisov)
07:19:44.27 -13:38:50.6 16.9mag C/2025 R3 (PANSTARRS)
10:05:38.84 +22:04:19.0 17.5mag C/2025 V2 (Rankin)
12:47:34.61 +03:34:07.1 17.0mag C/2025 Y1 (ATLAS)
16:30:45.79 +79:07:35.0 17.2mag C/2026 A2 (Bok)
02:54:13.20 +45:34:13.2 16.8mag C/2026 B2 (Sun-Gao)
11:30:51.21 +05:53:02.1 17.0mag A/2026 E1
21:31:18.85 -18:09:59.7 7.1mag 10P/Tempel
11:17:22.25 -02:15:01.8 16.2mag 29P/Schwassmann-Wachmann
04:11:37.70 +30:24:38.4 17.9mag 47P/Ashbrook-Jackson
10:24:49.95 +11:26:02.8 17.1mag 63P/Wild
00:51:25.80 -05:02:48.5 15.5mag 65P/Gunn
04:46:46.38 +20:31:50.5 13.7mag 78P/Gehrels
02:34:51.06 +11:39:35.6 16.4mag 88P/Howell
06:59:08.88 +29:58:24.0 15.8mag 93P/Lovas
04:47:17.99 +31:19:52.7 16.7mag 114P/Wiseman-Skiff
08:28:19.64 +29:45:04.1 15.2mag 123P/West-Hartley
11:03:14.22 -02:04:04.6 16.9mag 124P/Mrkos
05:04:34.45 +21:00:46.4 16.2mag 128P/Shoemaker-Holt
05:51:18.50 +19:36:39.9 17.8mag 131P/Mueller
07:42:08.78 +15:13:48.6 16.5mag 141P-D/Machholz
03:20:20.32 -20:44:34.6 15.1mag 161P/Hartley-IRAS
06:02:04.73 +35:31:03.2 15.5mag 162P/SidingSpring
18:38:48.27 +20:36:21.5 14.0mag 169P/NEAT
01:59:51.22 +08:25:06.7 17.6mag 220P/McNaught
16:35:32.79 -08:44:59.9 17.2mag 235P/LINEAR
09:02:05.71 +32:31:46.5 18.0mag 240P/NEAT
20:37:51.62 -51:09:52.4 17.8mag 259P/Garradd
02:21:57.71 +15:50:54.2 15.6mag 260P/McNaught
06:01:43.75 +37:23:34.6 17.3mag 295P/LINEAR
15:06:33.78 +05:18:47.6 17.6mag 391P/Kowalski
08:41:51.74 +19:20:28.1 17.9mag 450P/LONEOS
08:04:19.08 +38:32:30.8 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Jul 18 05:32 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-26eg 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -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
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
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
04:50:01.03 -02:22:33.80 2026-07-16.17 17.02
-rw-r--r-- 1 apache apache 5.6K Jul 18 05:32 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
-rw-r--r-- 1 apache apache 189K Jul 18 05:32 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:35:24.753 -14:51:35.01 AT 2026svz 2026-06-27.33 22.2271
20:31:55.032 -25:17:26.05 AT 2026svy 2026-06-27.32 22.425
23:12:03.386 -07:08:51.16 AT 2026svx 2026-06-27.43 22.3341
21:38:52.469 -09:12:08.16 AT 2026svw 2026-06-27.33 20.826
21:24:07.399 -08:10:48.32 AT 2026svv 2026-06-27.34 22.9964
20:42:22.608 -20:56:09.99 AT 2026svu 2026-06-27.32 22.8033
22:49:29.419 -09:52:21.90 AT 2026svt 2026-06-27.41 23.2399
23:08:56.975 -10:56:50.31 AT 2026svs 2026-06-27.42 23.0562
23:03:48.038 -10:42:20.17 AT 2026svr 2026-06-27.42 23.1156
21:05:20.116 -12:39:02.09 AT 2026svq 2026-06-27.30 22.4649
04:03:37.997 -49:14:19.96 AT 2026svp 2026-06-26.43 23.1019
21:42:26.450 -12:30:39.78 AT 2026svo 2026-06-26.41 23.1202
22:23:57.549 -05:26:28.43 AT 2026svn 2026-06-26.40 23.0846
21:59:30.646 -08:36:23.43 AT 2026svm 2026-06-26.41 23.0458
00:40:45.913 -42:36:08.06 AT 2026svl 2026-06-26.42 23.627
22:01:49.708 -02:28:35.92 AT 2026svk 2026-06-26.41 22.3804
22:26:37.642 -04:12:59.57 AT 2026svj 2026-06-26.40 22.8575
21:46:45.471 -13:57:34.56 AT 2026svi 2026-06-26.41 22.7499
21:42:08.217 -14:29:27.43 AT 2026svh 2026-06-26.41 23.2705
21:57:43.950 -02:48:28.98 AT 2026svg 2026-06-26.41 21.5213
-rw-r--r-- 1 apache apache 89K Jul 18 05:32 tns_transients_list.txt
