This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN
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 05 03.4293 2461163.9293 10.81 01:07:41.83 +60:54:06.9
124.90849 -1.90742 galactic Cas Second-epoch detections are separated by 1.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:41.83 +60:54:06.9 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:41.83 +60:54:06.9: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:41.83 +60:54:06.9: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 07 41.83 +60 54 06.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.9293,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.4293 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.79 01:12:31.07 +61:17:18.9
125.46170 -1.47958 galactic Cas Second-epoch detections are separated by 2.9" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:31.07 +61:17:18.9 (user input) | T | P | (position from user input) J-Ks=0.331+/-0.037 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:31.07 +61:17:18.9: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:31.07 +61:17:18.9: 13.51 +/- 0.04 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!
TCP 2026 05 03.4293* 01 12 31.07 +61 17 18.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.9293,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.4293 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.38 01:08:24.95 +61:34:58.6
124.95084 -1.22223 galactic Cas Second-epoch detections are separated by 3.2" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 522537957607670016 | 01:08:22.26 +61:34:35.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.214+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:24.95 +61:34:58.6: 12.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:24.95 +61:34:58.6: 12.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.97 +/- 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!
TCP 2026 05 03.4293* 01 08 24.95 +61 34 58.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522537957607670016,2461163.9293,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522537957607670016 20260503.4293 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.49 01:05:57.17 +63:03:34.4
124.57510 0.23413 galactic Cas Second-epoch detections are separated by 1.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 523282292613942656 | 01:05:59.30 +63:03:46.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:57.17 +63:03:34.4: 10.46 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:57.17 +63:03:34.4: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 05 57.17 +63 03 34.4 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 523282292613942656,2461163.9293,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523282292613942656 20260503.4293 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.30 01:25:15.40 +64:40:33.0
126.53988 2.04126 galactic Cas Second-epoch detections are separated by 2.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512840196327698304 | 01:25:16.38 +64:40:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.479+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:15.40 +64:40:33.0: 11.04 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:15.40 +64:40:33.0: 13.08 +/- 0.02 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!
TCP 2026 05 03.4293* 01 25 15.40 +64 40 33.0 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512840196327698304,2461163.9293,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512840196327698304 20260503.4293 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.46 01:15:54.28 +64:24:55.3
125.57041 1.66903 galactic Cas Second-epoch detections are separated by 1.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 524780377209160704 | 01:15:54.61 +64:25:14.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:54.28 +64:24:55.3: 10.71 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:54.28 +64:24:55.3: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 15 54.28 +64 24 55.3 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 524780377209160704,2461163.9293,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524780377209160704 20260503.4293 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.23 01:39:04.22 +61:53:23.8
128.51131 -0.46472 galactic Cas Second-epoch detections are separated by 0.9" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511521503928366976 | 01:39:01.96 +61:53:26.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:04.22 +61:53:23.8: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:04.22 +61:53:23.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 39 04.22 +61 53 23.8 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511521503928366976,2461163.9293,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511521503928366976 20260503.4293 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.21 01:14:45.36 +60:30:04.6
125.80084 -2.24052 galactic Cas Second-epoch detections are separated by 3.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510401067222116992 | 01:14:43.22 +60:30:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5: 1935BSD...C01....0S BSD 8- 705 J-Ks=0.606+/-0.039 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:45.36 +60:30:04.6: 12.79 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:45.36 +60:30:04.6: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 14 45.36 +60 30 04.6 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510401067222116992,2461163.9293,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510401067222116992 20260503.4293 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.97 01:45:35.12 +59:17:56.1
129.80410 -2.84843 galactic Cas Second-epoch detections are separated by 0.2" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.3995+59.3029 | 01:45:35.12 +59:17:56.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.464+/-0.026 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:35.12 +59:17:56.1: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:35.12 +59:17:56.1: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 45 35.12 +59 17 56.1 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.3995+59.3029,2461163.9293,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.3995+59.3029 20260503.4293 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.96 01:56:28.25 +62:04:57.0
130.46398 0.16553 galactic Cas Second-epoch detections are separated by 2.5" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 508724449429663744 | 01:56:28.08 +62:04:59.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:28.25 +62:04:57.0: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:28.25 +62:04:57.0: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 56 28.25 +62 04 57.0 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508724449429663744,2461163.9293,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508724449429663744 20260503.4293 9.96CV 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 05 03.4293 2461163.9293 9.97 01:12:40.98 +61:20:38.3
125.47691 -1.42275 galactic Cas Second-epoch detections are separated by 0.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 522563173351220736 | 01:12:36.96 +61:20:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.300+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:40.98 +61:20:38.3: 12.33 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:40.98 +61:20:38.3: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 12 40.98 +61 20 38.3 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 522563173351220736,2461163.9293,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522563173351220736 20260503.4293 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.90 01:42:49.53 +60:21:22.8
129.24914 -1.88360 galactic Cas Second-epoch detections are separated by 1.5" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:42:49.53 +60:21:22.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:49.53 +60:21:22.8: 12.75 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:49.53 +60:21:22.8: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 42 49.53 +60 21 22.8 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.9293,9.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.4293 9.90CV 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 05 03.4293 2461163.9293 9.77 01:55:14.55 +59:32:02.2
130.94832 -2.34107 galactic Cas Second-epoch detections are separated by 1.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506368711405378560 | 01:55:13.64 +59:31:39.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.224+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:14.55 +59:32:02.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:14.55 +59:32:02.2: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 55 14.55 +59 32 02.2 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506368711405378560,2461163.9293,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506368711405378560 20260503.4293 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.38 01:19:48.71 +61:38:15.1
126.29555 -1.04877 galactic Cas Second-epoch detections are separated by 0.6" and 3.3 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 510901241928240128 | 01:19:47.76 +61:38:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2: 1935BSD...C01....0S BSD 8-1789/90 J-Ks=0.282+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:48.71 +61:38:15.1: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:48.71 +61:38:15.1: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 19 48.71 +61 38 15.1 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510901241928240128,2461163.9293,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510901241928240128 20260503.4293 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.33 01:23:56.35 +62:06:41.6
126.72274 -0.52074 galactic Cas Second-epoch detections are separated by 1.7" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 511023356437978368 | 01:23:54.69 +62:06:22.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1960IzKry..24..160B [B60] +61 189 J-Ks=0.301+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:56.35 +62:06:41.6: 11.82 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:56.35 +62:06:41.6: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 23 56.35 +62 06 41.6 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511023356437978368,2461163.9293,9.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511023356437978368 20260503.4293 9.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 8.79 02:13:07.38 +58:04:47.3
133.57884 -3.09339 galactic Per Second-epoch detections are separated by 0.8" and 3.9 pix
The object was found in VSX 1" UX Per
Type: DCEP
# Max. Min./Amp. JD0 Period
11.020 V 12.070 V 2437402.94500 4.565815000000 F5-G3
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:07.38 +58:04:47.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:07.38 +58:04:47.3: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 02 13 07.38 +58 04 47.3 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
UX Per,2461163.9293,8.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UX Per 20260503.4293 8.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 8.94 01:22:08.34 +60:22:44.7
126.71988 -2.26667 galactic Cas Second-epoch detections are separated by 0.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510262906714846080 | 01:22:06.83 +60:22:27.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1960IzKry..24..160B [B60] +60 176 J-Ks=0.245+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:08.34 +60:22:44.7: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:08.34 +60:22:44.7: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 22 08.34 +60 22 44.7 8.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510262906714846080,2461163.9293,8.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510262906714846080 20260503.4293 8.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 8.79 01:16:01.09 +62:41:57.8
125.74614 -0.03797 galactic Cas Second-epoch detections are separated by 0.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 523030538810955648 | 01:16:01.09 +62:41:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1960IzKry..24..160B [B60] +62 89 J-Ks=0.197+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:01.09 +62:41:57.8: 11.02 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:01.09 +62:41:57.8: 11.38 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 16 01.09 +62 41 57.8 8.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 523030538810955648,2461163.9293,8.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523030538810955648 20260503.4293 8.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.30 01:46:30.05 +61:12:58.8
129.51194 -0.94998 galactic Cas Second-epoch detections are separated by 0.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | V0983 Cas | 01:46:27.67 +61:12:25.4 (Gaia DR3) | BE (local) | B8II: (local) | Gaia3var=VARIABLE SpType: B6 1933LicOB..16..119Z Cl* NGC 663 Zug 35 J-Ks=0.193+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:30.05 +61:12:58.8: 12.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:30.05 +61:12:58.8: 12.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 46 30.05 +61 12 58.8 9.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0983 Cas,2461163.9293,9.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0983 Cas 20260503.4293 9.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.38 01:19:11.13 +58:20:30.5
126.57673 -4.33344 galactic Cas Second-epoch detections are separated by 0.5" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413877380962478336 | 01:19:10.27 +58:20:57.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B1 1951UppAn...2j...1B NGC 457 120 J-Ks=0.002+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:11.13 +58:20:30.5: 12.56 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:11.13 +58:20:30.5: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 19 11.13 +58 20 30.5 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413877380962478336,2461163.9293,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413877380962478336 20260503.4293 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.54 01:40:01.51 +60:52:33.1
128.81180 -1.44000 galactic Cas Second-epoch detections are separated by 1.1" and 3.3 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 | ASASSN-V J013956.73+605213.0 | 01:39:56.73 +60:52:13.0 (Gaia DR3) | SR (local) | 450.000000000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.372+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:01.51 +60:52:33.1: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:01.51 +60:52:33.1: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 40 01.51 +60 52 33.1 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013956.73+605213.0,2461163.9293,9.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013956.73+605213.0 20260503.4293 9.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.99 01:18:14.15 +61:44:37.0
126.09841 -0.96327 galactic Cas Second-epoch detections are separated by 0.6" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:14.15 +61:44:37.0 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:14.15 +61:44:37.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:14.15 +61:44:37.0: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 18 14.15 +61 44 37.0 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.9293,9.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.4293 9.99CV 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 05 03.4293 2461163.9293 9.83 01:25:42.75 +65:40:09.8
126.45622 3.03245 galactic Cas Second-epoch detections are separated by 2.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 525281273472220544 | 01:25:45.20 +65:40:30.5 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE J-Ks=0.362+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:42.75 +65:40:09.8: 11.69 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:42.75 +65:40:09.8: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 25 42.75 +65 40 09.8 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 525281273472220544,2461163.9293,9.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 525281273472220544 20260503.4293 9.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.95 02:07:28.02 +60:16:11.2
132.22885 -1.22239 galactic Cas Second-epoch detections are separated by 0.5" and 3.6 pix
The object was found in VSX 0" Gaia DR3 507587382604105088
Type: RS
# Max. Min./Amp. JD0 Period
12.180 G 12.440 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:28.02 +60:16:11.2: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:28.02 +60:16:11.2: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 02 07 28.02 +60 16 11.2 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507587382604105088,2461163.9293,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507587382604105088 20260503.4293 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.11 01:29:32.92 +61:46:27.0
127.42228 -0.76486 galactic Cas Second-epoch detections are separated by 1.4" and 3.0 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 | 01:29:32.92 +61:46:27.0 (user input) | T | P | (position from user input) J-Ks=0.908+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:32.92 +61:46:27.0: 12.88 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:32.92 +61:46:27.0: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 29 32.92 +61 46 27.0 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.9293,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.4293 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.04 01:59:37.36 +62:54:28.8
130.60530 1.05653 galactic Cas Second-epoch detections are separated by 3.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:59:37.36 +62:54:28.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:37.36 +62:54:28.8: 12.15 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:37.36 +62:54:28.8: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 59 37.36 +62 54 28.8 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.9293,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.4293 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.24 02:11:50.28 +59:02:57.0
133.11990 -2.22301 galactic Per Second-epoch detections are separated by 4.7" and 3.1 pix
The object was found in VSX 1" NSVS J0211521+590234
Type: SR
# Max. Min./Amp. JD0 Period
13.888 r Y 0.567 r 2458346.14140 174.387018500000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:50.28 +59:02:57.0: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:50.28 +59:02:57.0: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 02 11 50.28 +59 02 57.0 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0211521+590234,2461163.9293,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0211521+590234 20260503.4293 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.37 01:23:56.46 +60:54:48.3
126.87374 -1.70933 galactic Cas Second-epoch detections are separated by 1.9" and 3.3 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 510306681022260864 | 01:23:51.35 +60:54:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.339+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:56.46 +60:54:48.3: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:56.46 +60:54:48.3: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 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!
TCP 2026 05 03.4293* 01 23 56.46 +60 54 48.3 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510306681022260864,2461163.9293,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510306681022260864 20260503.4293 10.37CV 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 05 03.4293 2461163.9293 10.38 02:20:52.80 +63:53:40.5
132.57949 2.71094 galactic Cas Second-epoch detections are separated by 1.7" and 3.3 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 515115223323344128 | 02:20:49.36 +63:53:39.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.307+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:52.80 +63:53:40.5: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:52.80 +63:53:40.5: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 02 20 52.80 +63 53 40.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 515115223323344128,2461163.9293,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 515115223323344128 20260503.4293 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.29 02:11:23.02 +61:21:06.8
132.36338 -0.04731 galactic Cas Second-epoch detections are separated by 1.3" and 3.6 pix
The object was found in VSX19" Gaia DR3 507740455237382016
Type: ROT
# Max. Min./Amp. JD0 Period
14.500 G 14.530 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:23.02 +61:21:06.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:23.02 +61:21:06.8: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 02 11 23.02 +61 21 06.8 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507740455237382016,2461163.9293,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507740455237382016 20260503.4293 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.35 02:10:23.82 +60:01:12.8
132.65103 -1.35314 galactic Cas Second-epoch detections are separated by 1.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:10:23.82 +60:01:12.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.329+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:23.82 +60:01:12.8: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:23.82 +60:01:12.8: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 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!
TCP 2026 05 03.4293* 02 10 23.82 +60 01 12.8 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.9293,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.4293 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.37 01:44:32.26 +58:45:35.5
129.78359 -3.40371 galactic Cas Second-epoch detections are separated by 2.4" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506461620135299584 | 01:44:30.78 +58:46:10.9 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B8: 1955ApJS....2..123F LF 5 +58 58 J-Ks=0.189+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:32.26 +58:45:35.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:32.26 +58:45:35.5: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 44 32.26 +58 45 35.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506461620135299584,2461163.9293,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506461620135299584 20260503.4293 10.37CV 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 05 03.4293 2461163.9293 10.37 02:16:36.20 +64:57:47.8
131.78876 3.56629 galactic Cas Second-epoch detections are separated by 0.9" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:16:36.20 +64:57:47.8 (user input) | T | P | (position from user input) J-Ks=0.520+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:36.20 +64:57:47.8: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:36.20 +64:57:47.8: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 02 16 36.20 +64 57 47.8 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461163.9293,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260503.4293 10.37CV 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 05 03.4293 2461163.9293 10.55 01:39:24.44 +63:23:52.9
128.27143 1.02467 galactic Cas Second-epoch detections are separated by 3.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 512471653773856768 | 01:39:21.54 +63:23:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.054 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:24.44 +63:23:52.9: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:24.44 +63:23:52.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 39 24.44 +63 23 52.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512471653773856768,2461163.9293,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512471653773856768 20260503.4293 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 11.11 01:27:56.55 +62:46:05.1
127.09403 0.19171 galactic Cas Second-epoch detections are separated by 1.4" and 3.3 pix
The object was found in VSX 3" Gaia DR3 512378916841008256
Type: E
# Max. Min./Amp. JD0 Period
14.550 G 14.640 G 1.395540000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:56.55 +62:46:05.1: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:56.55 +62:46:05.1: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 03.4293* 01 27 56.55 +62 46 05.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512378916841008256,2461163.9293,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512378916841008256 20260503.4293 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 10.52 02:07:46.75 +62:11:10.7
131.70811 0.62242 galactic Cas Second-epoch detections are separated by 1.1" and 3.5 pix
The object was found in ASASSN-V 2" ASASSN-V J020746.87+621112.3
Type: SR
MeanMag 15.53 m Amp. 1.57 m Period 397.2118966 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:46.75 +62:11:10.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:46.75 +62:11:10.7: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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!
TCP 2026 05 03.4293* 02 07 46.75 +62 11 10.7 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461163.9293,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260503.4293 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 03.4293 2461163.9293 9.94 01:39:32.50 +64:53:04.2
128.01029 2.48812 galactic Cas Second-epoch detections are separated by 0.9" and 3.0 pix
The object was found in VSX 2" ASASSN-V J013932.54+645302.3
Type: YSO
# Max. Min./Amp. JD0 Period
12.800 g 16.100 g
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:32.50 +64:53:04.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:32.50 +64:53:04.2: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 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!
TCP 2026 05 03.4293* 01 39 32.50 +64 53 04.2 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013932.54+645302.3,2461163.9293,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013932.54+645302.3 20260503.4293 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461163.92961866 03.05.2026 10:18:29.052 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.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.: -7.62
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: 6 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): 24036
Objects passed selection criteria: 23857
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: 15368.5
Average stars matched: 14336.5 (93.285 %)
Memory usage VmPeak: 128288 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 05:20:33 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: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461163.92961866 03.05.2026 10:18:29.052 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 116
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
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: 40 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): 178115
Objects passed selection criteria: 177593
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 120408
Average stars matched: 111709 (92.7758 %)
Memory usage VmPeak: 1934660 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 29 15:05:05 CDT 2026
VaST build number 1.0rc89-35-gf9552f12
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 3 05:25:07 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.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: 2461163.92900851
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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/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_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
Image size: 939.0'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 01:42:34.553 +62:03:31.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:34.553 +62:03:31.21
Angular distance between the image centers 0.0744 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
Image size: 939.0'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:36.960 +62:03:40.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:36.960 +62:03:40.89
Angular distance between the image centers 0.0779 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 01:42:34.553 +62:03:31.21
Second-epoch second image center 01:42:36.960 +62:03:40.89
Angular distance between the image centers 0.00541 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.mtsBBVJP4l
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.zx3GFCm3we
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits &> /tmp/tmp.bOOl43YJfQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits &> /tmp/tmp.S5LYpTHIdr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 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 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 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): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929150
a=0.000000 b=1.000000 c=22.929150
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 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 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 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): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.8)
Read 31681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.0659 to 45.7628 deg, Dec +55.3336 to +67.4023 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 7.0659 to 45.7628 deg, Dec 55.3336 to 67.4023 deg
Loaded 26179 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): 14497 out of 16269 total matches.
Matched with Tycho-2 16269 out of 31681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
2.5 pix fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
13.7 mag. fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
13.7 mag. fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mtsBBVJP4l (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/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 266 matched stars entering correct_measured_positions(), 9996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 337 matched stars entering correct_measured_positions(), 10041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.88"
Excluding outliers - 331 stars left (next iteration limit 292)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zx3GFCm3we (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/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bOOl43YJfQ (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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=687, passed=9141
Got 9141 stars (including 8443 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat
util/solve_plate_with_UCAC5 got 9141 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (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 729 to 788 (Dec 55.9 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(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 8920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 67.3)
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(), 8920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 8920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 971 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.S5LYpTHIdr (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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=725, passed=9127
Got 9127 stars (including 8397 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat
util/solve_plate_with_UCAC5 got 9127 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (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 729 to 788 (Dec 55.9 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(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 8877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 67.3)
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: 970 matched stars entering correct_measured_positions(), 8876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 8876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 970 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52599_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 52599_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:19:46.50 +58:12:25.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/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_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
Image size: 939.0'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 01:42:34.553 +62:03:31.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:34.553 +62:03:31.21
Angular distance between the image centers 0.0744 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
Image size: 939.0'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:36.960 +62:03:40.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:36.960 +62:03:40.89
Angular distance between the image centers 0.0779 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 01:42:34.553 +62:03:31.21
Second-epoch second image center 01:42:36.960 +62:03:40.89
Angular distance between the image centers 0.00541 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.4j9ucgxhcM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.QSK36x0xs2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits &> /tmp/tmp.CTqWOhuxqx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits &> /tmp/tmp.s2HWqpOGia
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
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_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 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 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 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): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.035150
a=0.000000 b=1.000000 c=20.035150
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.76
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 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 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 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): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=4.4)
Read 218998 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9707 to 45.8168 deg, Dec +55.3262 to +67.4140 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 6.9707 to 45.8168 deg, Dec 55.3262 to 67.4140 deg
Loaded 26295 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): 10859 out of 16691 total matches.
Matched with Tycho-2 16691 out of 218998 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 105 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.3 pix fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
2.3 pix fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.0 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
12.8 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
12.7 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
11.1 mag. fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
11.1 mag. fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
All-image limiting magnitude estimate: 11.1 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.4j9ucgxhcM (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/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=35398, passed=222522
Got 222522 stars (including 186791 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 222522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 275 matched stars entering correct_measured_positions(), 212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 264 matched stars entering correct_measured_positions(), 49591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 434 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 49636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
Accuracy estimation diagnostic: 344 matched stars entering correct_measured_positions(), 64908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.78"
Excluding outliers - 344 stars left (next iteration limit 290)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QSK36x0xs2 (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/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=35098, passed=218974
Got 218974 stars (including 183551 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 218974 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.CTqWOhuxqx (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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=4594, passed=70976
Got 70976 stars (including 66287 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat
util/solve_plate_with_UCAC5 got 70976 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (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 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 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: 968 matched stars entering correct_measured_positions(), 69846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 69848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 69848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 967 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.s2HWqpOGia (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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=13, blended=4733, passed=72866
Got 72866 stars (including 68046 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat
util/solve_plate_with_UCAC5 got 72866 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (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 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 71313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 67.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 71314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 71314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-17-36_20.00sec_-5.00C_LIGHT_0407.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.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_2026-05-03_CI_Cas-03-Q2b1x1_051905_TTUQ2b1x1_3736053_1vSorFlN/wcs_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408.fits
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:10.49 +60:37:29.5: 7.57 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:06.55 +62:48:53.0: 10.42 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:24.95 +61:34:58.6: 12.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:41.83 +60:54:06.9: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:54.28 +64:24:55.3: 10.71 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:31.07 +61:17:18.9: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:15.40 +64:40:33.0: 11.04 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:57.17 +63:03:34.4: 10.46 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:04.22 +61:53:23.8: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:10.49 +60:37:29.5: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 7.84 +/- 0.01
Forced photometry filter REJECTED candidate at 01:33:10.49 +60:37:29.5: ref_mag=7.84 +/- 0.01 new_mean_mag=10.5040 delta=-2.66 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:41.83 +60:54:06.9: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.05
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:24.95 +61:34:58.6: 12.97 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:15.40 +64:40:33.0: 13.08 +/- 0.02 detection
Forced photometry filter KEPT candidate at 01:07:41.83 +60:54:06.9: ref_mag=13.68 +/- 0.05 new_mean_mag=10.8052 delta=2.87 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:54.28 +64:24:55.3: 13.10 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:06.55 +62:48:53.0: 13.52 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:31.07 +61:17:18.9: 13.51 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:57.17 +63:03:34.4: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.04
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter KEPT candidate at 01:08:24.95 +61:34:58.6: ref_mag=12.97 +/- 0.04 new_mean_mag=10.3349 delta=2.64 (need > 0.90)
Forced photometry reference-image weighted average: 12.22 +/- 0.02
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry reference-image weighted average: 11.56 +/- 0.02
Forced photometry filter KEPT candidate at 01:25:15.40 +64:40:33.0: ref_mag=12.66 +/- 0.02 new_mean_mag=10.2751 delta=2.38 (need > 0.90)
Forced photometry reference-image weighted average: 12.06 +/- 0.02
Forced photometry filter KEPT candidate at 01:15:54.28 +64:24:55.3: ref_mag=12.22 +/- 0.02 new_mean_mag=10.4495 delta=1.77 (need > 0.90)
Forced photometry filter KEPT candidate at 01:12:31.07 +61:17:18.9: ref_mag=13.51 +/- 0.04 new_mean_mag=10.7645 delta=2.75 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:05:06.55 +62:48:53.0: ref_mag=11.56 +/- 0.02 new_mean_mag=11.0295 delta=0.53 (need > 0.90)
Forced photometry filter KEPT candidate at 01:05:57.17 +63:03:34.4: ref_mag=12.06 +/- 0.02 new_mean_mag=10.4898 delta=1.57 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:04.22 +61:53:23.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter KEPT candidate at 01:39:04.22 +61:53:23.8: ref_mag=12.90 +/- 0.02 new_mean_mag=10.2156 delta=2.69 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:45.36 +60:30:04.6: 12.79 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:35.12 +59:17:56.1: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:28.25 +62:04:57.0: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:45.36 +60:30:04.6: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Forced photometry filter KEPT candidate at 01:14:45.36 +60:30:04.6: ref_mag=13.05 +/- 0.03 new_mean_mag=10.2065 delta=2.84 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:35.12 +59:17:56.1: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Forced photometry filter KEPT candidate at 01:45:35.12 +59:17:56.1: ref_mag=12.63 +/- 0.02 new_mean_mag=9.9495 delta=2.68 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:28.25 +62:04:57.0: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter KEPT candidate at 01:56:28.25 +62:04:57.0: ref_mag=12.81 +/- 0.02 new_mean_mag=9.9651 delta=2.84 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:40.98 +61:20:38.3: 12.33 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:40.98 +61:20:38.3: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter KEPT candidate at 01:12:40.98 +61:20:38.3: ref_mag=12.71 +/- 0.02 new_mean_mag=9.9673 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:49.53 +60:21:22.8: 12.75 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:14.55 +59:32:02.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:49.53 +60:21:22.8: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 01:42:49.53 +60:21:22.8: ref_mag=12.64 +/- 0.01 new_mean_mag=9.9062 delta=2.73 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:48.71 +61:38:15.1: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:14.55 +59:32:02.2: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Forced photometry filter KEPT candidate at 01:55:14.55 +59:32:02.2: ref_mag=12.51 +/- 0.02 new_mean_mag=9.7697 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:56.35 +62:06:41.6: 11.82 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:07.38 +58:04:47.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:08.34 +60:22:44.7: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:01.09 +62:41:57.8: 11.02 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:48.71 +61:38:15.1: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry filter KEPT candidate at 01:19:48.71 +61:38:15.1: ref_mag=11.96 +/- 0.01 new_mean_mag=9.3732 delta=2.59 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:56.35 +62:06:41.6: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Forced photometry filter KEPT candidate at 01:23:56.35 +62:06:41.6: ref_mag=11.85 +/- 0.01 new_mean_mag=9.3303 delta=2.52 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:07.38 +58:04:47.3: 11.52 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:08.34 +60:22:44.7: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Forced photometry filter KEPT candidate at 02:13:07.38 +58:04:47.3: ref_mag=11.52 +/- 0.01 new_mean_mag=8.7950 delta=2.72 (need > 0.90)
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Forced photometry filter KEPT candidate at 01:22:08.34 +60:22:44.7: ref_mag=11.67 +/- 0.01 new_mean_mag=8.9355 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:01.09 +62:41:57.8: 11.38 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.00
Forced photometry filter KEPT candidate at 01:16:01.09 +62:41:57.8: ref_mag=11.38 +/- 0.00 new_mean_mag=8.7938 delta=2.58 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:30.05 +61:12:58.8: 12.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:30.05 +61:12:58.8: 12.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.03
Forced photometry filter KEPT candidate at 01:46:30.05 +61:12:58.8: ref_mag=12.17 +/- 0.03 new_mean_mag=9.2990 delta=2.87 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:11.13 +58:20:30.5: 12.56 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:11.13 +58:20:30.5: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.02
Forced photometry filter KEPT candidate at 01:19:11.13 +58:20:30.5: ref_mag=12.14 +/- 0.02 new_mean_mag=9.3820 delta=2.76 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:01.51 +60:52:33.1: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:01.51 +60:52:33.1: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Forced photometry filter KEPT candidate at 01:40:01.51 +60:52:33.1: ref_mag=12.42 +/- 0.02 new_mean_mag=9.5373 delta=2.88 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:14.15 +61:44:37.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:14.15 +61:44:37.0: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Forced photometry filter KEPT candidate at 01:18:14.15 +61:44:37.0: ref_mag=12.77 +/- 0.02 new_mean_mag=9.9929 delta=2.78 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:42.75 +65:40:09.8: 11.69 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:42.75 +65:40:09.8: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 01:25:42.75 +65:40:09.8: ref_mag=12.60 +/- 0.01 new_mean_mag=9.7846 delta=2.81 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:28.02 +60:16:11.2: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:28.02 +60:16:11.2: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Forced photometry filter KEPT candidate at 02:07:28.02 +60:16:11.2: ref_mag=12.64 +/- 0.02 new_mean_mag=9.9479 delta=2.69 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:32.92 +61:46:27.0: 12.88 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:37.36 +62:54:28.8: 12.15 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:32.92 +61:46:27.0: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Forced photometry filter KEPT candidate at 01:29:32.92 +61:46:27.0: ref_mag=13.00 +/- 0.03 new_mean_mag=10.1039 delta=2.90 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:37.36 +62:54:28.8: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Forced photometry filter KEPT candidate at 01:59:37.36 +62:54:28.8: ref_mag=12.90 +/- 0.03 new_mean_mag=10.0461 delta=2.85 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:50.28 +59:02:57.0: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:50.28 +59:02:57.0: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.07
Forced photometry filter KEPT candidate at 02:11:50.28 +59:02:57.0: ref_mag=14.22 +/- 0.07 new_mean_mag=10.2324 delta=3.99 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:56.46 +60:54:48.3: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:52.80 +63:53:40.5: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:23.02 +61:21:06.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:56.46 +60:54:48.3: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.04
Forced photometry filter KEPT candidate at 01:23:56.46 +60:54:48.3: ref_mag=13.30 +/- 0.04 new_mean_mag=10.3719 delta=2.93 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:52.80 +63:53:40.5: 12.92 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:23.02 +61:21:06.8: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Forced photometry filter KEPT candidate at 02:20:52.80 +63:53:40.5: ref_mag=12.92 +/- 0.03 new_mean_mag=10.3605 delta=2.56 (need > 0.90)
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Forced photometry filter KEPT candidate at 02:11:23.02 +61:21:06.8: ref_mag=13.22 +/- 0.03 new_mean_mag=10.2853 delta=2.94 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:23.82 +60:01:12.8: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:23.82 +60:01:12.8: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Forced photometry filter KEPT candidate at 02:10:23.82 +60:01:12.8: ref_mag=13.38 +/- 0.04 new_mean_mag=10.3442 delta=3.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:32.26 +58:45:35.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:32.26 +58:45:35.5: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Forced photometry filter KEPT candidate at 01:44:32.26 +58:45:35.5: ref_mag=12.98 +/- 0.03 new_mean_mag=10.3717 delta=2.60 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:36.20 +64:57:47.8: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:36.20 +64:57:47.8: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Forced photometry filter KEPT candidate at 02:16:36.20 +64:57:47.8: ref_mag=13.28 +/- 0.03 new_mean_mag=10.3632 delta=2.91 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:24.44 +63:23:52.9: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:24.44 +63:23:52.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 01:39:24.44 +63:23:52.9: ref_mag=13.22 +/- 0.02 new_mean_mag=10.5498 delta=2.67 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:56.55 +62:46:05.1: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:56.55 +62:46:05.1: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry filter KEPT candidate at 01:27:56.55 +62:46:05.1: ref_mag=13.91 +/- 0.05 new_mean_mag=11.1058 delta=2.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:46.75 +62:11:10.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:46.75 +62:11:10.7: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Forced photometry filter KEPT candidate at 02:07:46.75 +62:11:10.7: ref_mag=13.85 +/- 0.04 new_mean_mag=10.5039 delta=3.35 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:32.50 +64:53:04.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:32.50 +64:53:04.2: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Forced photometry filter KEPT candidate at 01:39:32.50 +64:53:04.2: ref_mag=13.52 +/- 0.04 new_mean_mag=9.9319 delta=3.59 (need > 0.90)
Adding exclusion_list_local.txt__out247627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out252777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out256334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out256395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out257844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out260059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out260079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out260701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out260707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out260727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84112.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 52s
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: 24s
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Considering the candidate 247622_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 247622_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
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Considering the candidate 247627_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247627_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247628_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 247628_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:33:35.40 +59:56:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247635_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247635_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247638_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247638_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247641_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 247641_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:32:22.11 +60:27:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247642_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247642_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247644_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 247644_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
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Considering the candidate 247645_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247645_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247648_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247648_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247649_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247649_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247654_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 247654_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:14:55.85 +60:30:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247655_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 247655_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:46:42.44 +61:09:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247657_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247657_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247659_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247659_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247661_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247661_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247662_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247662_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247663_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 247663_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:07:08.23 +57:44:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247664_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 247664_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:43:51.74 +61:53:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247665_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247665_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247666_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247666_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247669_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 247669_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:43:59.29 +61:55:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247670_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 247670_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:16:20.80 +62:42:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247675_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247675_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247676_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247676_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247677_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247677_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247678_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247678_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 247679_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 247679_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 250278_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 250278_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:46:19.58 +61:15:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251144_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 251144_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 251862_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 251862_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:44:02.28 +61:53:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251894_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 251894_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 252147_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 252147_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:46:08.70 +61:12:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252325_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 252325_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 252607_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 252607_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:38:00.45 +57:56:46.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252777_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 252777_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 253157_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 253157_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:17:59.17 +57:47:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253990_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 253990_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 254797_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 254797_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:28:15.39 +58:44:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255208_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 255208_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 255227_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 255227_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:42:49.35 +61:25:56.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255893_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 255893_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:19:12.14 +65:35:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255990_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 255990_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 255997_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 255997_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:58:16.31 +59:38:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256334_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 256334_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 256395_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 256395_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 257011_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 257011_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:18:18.99 +57:42:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257228_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 257228_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:16:08.73 +58:49:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257319_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 257319_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:20:11.09 +58:12:08.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257329_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 257329_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 257366_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 257366_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:46:33.63 +61:16:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257397_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 257397_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:38:33.34 +60:48:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257456_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 257456_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:33:47.45 +60:38:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257471_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 257471_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 02:05:03.75 +64:21:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257575_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 257575_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:20:18.50 +58:13:42.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257673_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 257673_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257844_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 257844_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257895_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 257895_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:44:17.70 +61:53:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258133_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 258133_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 02:00:51.96 +58:31:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258356_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 258356_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:26:41.05 +60:46:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258438_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 258438_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:45:50.36 +57:50:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258474_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 258474_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:29:21.00 +63:17:35.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258825_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 258825_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:43:53.28 +61:53:15.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259029_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 259029_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:51:02.41 +64:49:54.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259185_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 259185_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:33:59.37 +58:28:33.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259337_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 259337_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259571_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 259571_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 02:04:26.60 +65:05:53.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259576_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 259576_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 02:15:59.00 +63:12:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259803_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 259803_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:39:00.42 +61:11:52.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259978_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 259978_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260059_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 260059_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260079_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 260079_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260371_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 260371_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:07:40.39 +63:30:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260701_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 260701_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260707_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 260707_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260711_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 260711_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:55:18.90 +63:39:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260727_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 260727_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260761_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 260761_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:42:33.01 +63:52:58.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260820_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 260820_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 02:02:54.93 +64:25:00.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261013_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 261013_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:17:01.00 +61:40:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261199_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 261199_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:52:48.70 +60:28:34.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261416_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 261416_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 261595_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 261595_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:27:52.44 +62:46:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261641_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 261641_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:16:05.21 +58:49:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261728_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 261728_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:16:12.75 +62:42:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261946_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 261946_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:13:35.87 +57:52:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262177_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 262177_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:34:10.31 +62:09:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262527_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 262527_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 262629_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 262629_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:29:33.18 +63:19:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262927_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 262927_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:49:34.24 +61:03:37.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263095_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 263095_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:29:34.19 +63:19:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263190_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 263190_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:35:50.59 +61:27:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264583_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 264583_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 02:03:15.32 +62:12:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265338_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 265338_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 265397_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 265397_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:35:01.06 +60:22:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265436_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 265436_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 265476_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 265476_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 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 241649_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 241649_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 70271_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 02:20:32.46 +62:32:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 72532_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:45:35.68 +63:07:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190057_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 190057_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 84112_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 84112_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 14452_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 14452_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 34158_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
Preparing report for the candidate 34158_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
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Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408
The candidate 39378_fd_Cas-03-Q2b1x1_2026-05-03_05-18-29_20.00sec_-4.90C_LIGHT_0408 did not pass the final checks
**** FOUND 01:47:55.71 +64:32:55.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 78s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:07:41.83 +60:54:06.9
01:12:31.07 +61:17:18.9
01:08:24.95 +61:34:58.6
01:05:57.17 +63:03:34.4
01:25:15.40 +64:40:33.0
01:15:54.28 +64:24:55.3
01:39:04.22 +61:53:23.8
01:14:45.36 +60:30:04.6
01:45:35.12 +59:17:56.1
01:56:28.25 +62:04:57.0
01:12:40.98 +61:20:38.3
01:42:49.53 +60:21:22.8
01:55:14.55 +59:32:02.2
01:19:48.71 +61:38:15.1
01:23:56.35 +62:06:41.6
02:13:07.38 +58:04:47.3
01:22:08.34 +60:22:44.7
01:16:01.09 +62:41:57.8
01:46:30.05 +61:12:58.8
01:19:11.13 +58:20:30.5
01:40:01.51 +60:52:33.1
01:18:14.15 +61:44:37.0
01:25:42.75 +65:40:09.8
02:07:28.02 +60:16:11.2
01:29:32.92 +61:46:27.0
01:59:37.36 +62:54:28.8
02:11:50.28 +59:02:57.0
01:23:56.46 +60:54:48.3
02:20:52.80 +63:53:40.5
02:11:23.02 +61:21:06.8
02:10:23.82 +60:01:12.8
01:44:32.26 +58:45:35.5
02:16:36.20 +64:57:47.8
01:39:24.44 +63:23:52.9
01:27:56.55 +62:46:05.1
01:39:32.50 +64:53:04.2
02:07:46.75 +62:11:10.7
########### Completed Cas-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:07:41.83 +60:54:06.9
01:12:31.07 +61:17:18.9
01:08:24.95 +61:34:58.6
01:05:57.17 +63:03:34.4
01:25:15.40 +64:40:33.0
01:15:54.28 +64:24:55.3
01:39:04.22 +61:53:23.8
01:14:45.36 +60:30:04.6
01:45:35.12 +59:17:56.1
01:56:28.25 +62:04:57.0
01:12:40.98 +61:20:38.3
01:42:49.53 +60:21:22.8
01:55:14.55 +59:32:02.2
01:19:48.71 +61:38:15.1
01:23:56.35 +62:06:41.6
02:13:07.38 +58:04:47.3
01:22:08.34 +60:22:44.7
01:16:01.09 +62:41:57.8
01:46:30.05 +61:12:58.8
01:19:11.13 +58:20:30.5
01:40:01.51 +60:52:33.1
01:18:14.15 +61:44:37.0
01:25:42.75 +65:40:09.8
02:07:28.02 +60:16:11.2
01:29:32.92 +61:46:27.0
01:59:37.36 +62:54:28.8
02:11:50.28 +59:02:57.0
01:23:56.46 +60:54:48.3
02:20:52.80 +63:53:40.5
02:11:23.02 +61:21:06.8
02:10:23.82 +60:01:12.8
01:44:32.26 +58:45:35.5
02:16:36.20 +64:57:47.8
01:39:24.44 +63:23:52.9
01:27:56.55 +62:46:05.1
02:07:46.75 +62:11:10.7
01:39:32.50 +64:53:04.2
###################################################################################
01:07:41.83 +60:54:06.9 -- not an asteroid (will add it to exclusion list)
01:12:31.07 +61:17:18.9 -- not an asteroid (will add it to exclusion list)
01:08:24.95 +61:34:58.6 -- not an asteroid (will add it to exclusion list)
01:05:57.17 +63:03:34.4 -- not an asteroid (will add it to exclusion list)
01:25:15.40 +64:40:33.0 -- not an asteroid (will add it to exclusion list)
01:15:54.28 +64:24:55.3 -- not an asteroid (will add it to exclusion list)
01:39:04.22 +61:53:23.8 -- not an asteroid (will add it to exclusion list)
01:14:45.36 +60:30:04.6 -- not an asteroid (will add it to exclusion list)
01:45:35.12 +59:17:56.1 -- not an asteroid (will add it to exclusion list)
01:56:28.25 +62:04:57.0 -- not an asteroid (will add it to exclusion list)
01:12:40.98 +61:20:38.3 -- not an asteroid (will add it to exclusion list)
01:42:49.53 +60:21:22.8 -- not an asteroid (will add it to exclusion list)
01:55:14.55 +59:32:02.2 -- not an asteroid (will add it to exclusion list)
01:19:48.71 +61:38:15.1 -- not an asteroid (will add it to exclusion list)
01:23:56.35 +62:06:41.6 -- not an asteroid (will add it to exclusion list)
02:13:07.38 +58:04:47.3 -- not an asteroid (will add it to exclusion list)
01:22:08.34 +60:22:44.7 -- not an asteroid (will add it to exclusion list)
01:16:01.09 +62:41:57.8 -- not an asteroid (will add it to exclusion list)
01:46:30.05 +61:12:58.8 -- not an asteroid (will add it to exclusion list)
01:19:11.13 +58:20:30.5 -- not an asteroid (will add it to exclusion list)
01:40:01.51 +60:52:33.1 -- not an asteroid (will add it to exclusion list)
01:18:14.15 +61:44:37.0 -- not an asteroid (will add it to exclusion list)
01:25:42.75 +65:40:09.8 -- not an asteroid (will add it to exclusion list)
02:07:28.02 +60:16:11.2 -- not an asteroid (will add it to exclusion list)
01:29:32.92 +61:46:27.0 -- not an asteroid (will add it to exclusion list)
01:59:37.36 +62:54:28.8 -- not an asteroid (will add it to exclusion list)
02:11:50.28 +59:02:57.0 -- not an asteroid (will add it to exclusion list)
01:23:56.46 +60:54:48.3 -- not an asteroid (will add it to exclusion list)
02:20:52.80 +63:53:40.5 -- not an asteroid (will add it to exclusion list)
02:11:23.02 +61:21:06.8 -- not an asteroid (will add it to exclusion list)
02:10:23.82 +60:01:12.8 -- not an asteroid (will add it to exclusion list)
01:44:32.26 +58:45:35.5 -- not an asteroid (will add it to exclusion list)
02:16:36.20 +64:57:47.8 -- not an asteroid (will add it to exclusion list)
01:39:24.44 +63:23:52.9 -- not an asteroid (will add it to exclusion list)
01:27:56.55 +62:46:05.1 -- not an asteroid (will add it to exclusion list)
02:07:46.75 +62:11:10.7 -- not an asteroid (will add it to exclusion list)
01:39:32.50 +64:53:04.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:05:57.17 +63:03:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:41.83 +60:54:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:24.95 +61:34:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:31.07 +61:17:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:40.98 +61:20:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:45.36 +60:30:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:54.28 +64:24:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:01.09 +62:41:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:14.15 +61:44:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:11.13 +58:20:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:48.71 +61:38:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:08.34 +60:22:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:56.35 +62:06:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:56.46 +60:54:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:15.40 +64:40:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:42.75 +65:40:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:56.55 +62:46:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:32.92 +61:46:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:04.22 +61:53:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:24.44 +63:23:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:32.50 +64:53:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:01.51 +60:52:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:49.53 +60:21:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:32.26 +58:45:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:35.12 +59:17:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:30.05 +61:12:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:14.55 +59:32:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:28.25 +62:04:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:37.36 +62:54:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:28.02 +60:16:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:46.75 +62:11:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:23.82 +60:01:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:23.02 +61:21:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:50.28 +59:02:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:07.38 +58:04:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:36.20 +64:57:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:52.80 +63:53:40.5 -- 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)
01:05:57.17 +63:03:34.4 -- not a known variable star
01:07:41.83 +60:54:06.9 -- not a known variable star
01:08:24.95 +61:34:58.6 -- not a known variable star
01:12:31.07 +61:17:18.9 -- not a known variable star
01:12:40.98 +61:20:38.3 -- not a known variable star
01:14:45.36 +60:30:04.6 -- not a known variable star
01:15:54.28 +64:24:55.3 -- not a known variable star
01:16:01.09 +62:41:57.8 -- not a known variable star
01:18:14.15 +61:44:37.0 -- not a known variable star
01:19:11.13 +58:20:30.5 -- not a known variable star
01:19:48.71 +61:38:15.1 -- not a known variable star
01:22:08.34 +60:22:44.7 -- not a known variable star
01:23:56.35 +62:06:41.6 -- not a known variable star
01:23:56.46 +60:54:48.3 -- not a known variable star
01:25:15.40 +64:40:33.0 -- not a known variable star
01:25:42.75 +65:40:09.8 -- not a known variable star
01:27:56.55 +62:46:05.1 -- a known variable star
01:29:32.92 +61:46:27.0 -- not a known variable star
01:39:04.22 +61:53:23.8 -- not a known variable star
01:39:24.44 +63:23:52.9 -- not a known variable star
01:39:32.50 +64:53:04.2 -- a known variable star
01:40:01.51 +60:52:33.1 -- not a known variable star
01:42:49.53 +60:21:22.8 -- not a known variable star
01:44:32.26 +58:45:35.5 -- not a known variable star
01:45:35.12 +59:17:56.1 -- not a known variable star
01:46:30.05 +61:12:58.8 -- not a known variable star
01:55:14.55 +59:32:02.2 -- not a known variable star
01:56:28.25 +62:04:57.0 -- not a known variable star
01:59:37.36 +62:54:28.8 -- not a known variable star
02:07:28.02 +60:16:11.2 -- a known variable star
02:07:46.75 +62:11:10.7 -- a known variable star
02:10:23.82 +60:01:12.8 -- not a known variable star
02:11:23.02 +61:21:06.8 -- a known variable star
02:11:50.28 +59:02:57.0 -- a known variable star
02:13:07.38 +58:04:47.3 -- a known variable star
02:16:36.20 +64:57:47.8 -- not a known variable star
02:20:52.80 +63:53:40.5 -- not a known variable star
Found 30 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
37 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
01:05:57.17 +63:03:34.4
01:07:41.83 +60:54:06.9
01:08:24.95 +61:34:58.6
01:12:31.07 +61:17:18.9
01:12:40.98 +61:20:38.3
01:14:45.36 +60:30:04.6
01:15:54.28 +64:24:55.3
01:16:01.09 +62:41:57.8
01:18:14.15 +61:44:37.0
01:19:11.13 +58:20:30.5
01:19:48.71 +61:38:15.1
01:22:08.34 +60:22:44.7
01:23:56.35 +62:06:41.6
01:23:56.46 +60:54:48.3
01:25:15.40 +64:40:33.0
01:25:42.75 +65:40:09.8
01:27:56.55 +62:46:05.1
01:29:32.92 +61:46:27.0
01:39:04.22 +61:53:23.8
01:39:24.44 +63:23:52.9
01:39:32.50 +64:53:04.2
01:40:01.51 +60:52:33.1
01:42:49.53 +60:21:22.8
01:44:32.26 +58:45:35.5
01:45:35.12 +59:17:56.1
01:46:30.05 +61:12:58.8
01:55:14.55 +59:32:02.2
01:56:28.25 +62:04:57.0
01:59:37.36 +62:54:28.8
02:07:28.02 +60:16:11.2
02:07:46.75 +62:11:10.7
02:10:23.82 +60:01:12.8
02:11:23.02 +61:21:06.8
02:11:50.28 +59:02:57.0
02:13:07.38 +58:04:47.3
02:16:36.20 +64:57:47.8
02:20:52.80 +63:53:40.5
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461163.92900851 -observatory V36
01:54:49.61 +10:01:00.1 Mercury (-1.0mag)
04:36:29.74 +23:03:42.9 Venus (-3.9mag)
01:07:13.71 +06:12:09.8 Mars (1.2mag)
07:22:02.63 +22:29:34.3 Jupiter (-2.0mag)
00:36:40.92 +01:35:02.8 Saturn (0.9mag)
03:51:35.53 +19:59:44.3 Uranus (5.8mag)
00:12:59.05 -00:02:00.4 Neptune (7.8mag)
20:34:13.16 -22:54:30.2 Pluto (14.5mag)
15:51:10.05 -26:04:39.8 Moon (-12.2mag)
-rw-r--r-- 1 apache apache 363 May 3 05:20 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461163.92900851:
07:21:56.18 +22:29:50.0 Io (5.9mag)
07:21:58.74 +22:29:46.0 Europa (6.0mag)
07:21:44.42 +22:30:16.7 Ganymede (5.4mag)
07:22:36.05 +22:28:16.6 Callisto (6.7mag)
07:24:29.49 +22:10:22.9 Himalia (15.4mag)
07:22:07.17 +22:29:23.1 Thebe (16.3mag)
07:24:56.49 +22:39:20.6 Elara (17.4mag)
07:22:05.67 +23:00:26.4 Pasiphae (17.5mag)
07:29:55.61 +22:28:59.7 Carme (18.6mag)
00:36:36.24 +01:35:31.4 Titan (8.7mag)
00:36:37.34 +01:35:14.8 Rhea (10.0mag)
00:36:14.99 +01:33:02.2 Iapetus (11.5mag)
00:36:56.22 +01:34:57.7 Hyperion (14.7mag)
00:38:02.49 +01:41:49.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 3 05:20 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461163.92900851:
16:38:15.95 -26:07:50.5 JWST
18:06:47.76 +32:25:08.9 Chandra
20:46:29.29 +37:28:56.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 3 05:20 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461163.92900851 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
06:44:18.15 +29:11:32.6 17.8mag P/2009 WX51 (Catalina)
18:55:53.58 -29:54:56.9 13.8mag P/2010 H2 (Vales)
05:20:24.40 -68:55:35.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:36:55.84 +31:34:29.5 17.3mag C/2017 K2 (PANSTARRS)
17:27:17.25 +12:30:13.9 17.7mag C/2021 G2 (ATLAS)
23:13:45.73 +29:59:15.1 17.1mag C/2022 E2 (ATLAS)
04:50:02.35 +26:28:03.8 16.2mag C/2022 N2 (PANSTARRS)
09:08:59.52 +31:57:26.7 16.4mag C/2022 QE78 (ATLAS)
08:35:08.55 +01:31:38.7 17.5mag C/2022 R6 (PANSTARRS)
18:47:59.56 +19:53:46.5 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:34:07.71 -11:16:11.3 17.5mag P/2023 B1 (PANSTARRS)
09:01:45.93 -09:18:49.1 17.8mag C/2023 F3 (ATLAS)
22:08:23.22 +64:02:07.1 17.6mag C/2023 H5 (Lemmon)
18:59:07.00 -04:12:16.2 13.9mag C/2023 R1 (PANSTARRS)
19:13:17.17 +88:08:50.6 17.9mag C/2023 X2 (Lemmon)
06:29:37.37 +63:32:50.9 17.3mag C/2024 A1 (ATLAS)
05:47:44.66 +22:52:51.4 12.1mag C/2024 E1 (Wierzchos)
16:06:40.31 +09:09:16.9 17.3mag C/2024 G6 (ATLAS)
20:23:35.06 +20:14:17.0 14.4mag C/2024 J3 (ATLAS)
03:42:36.62 -19:54:20.4 16.2mag C/2024 T5 (ATLAS)
05:32:15.60 +41:17:45.5 17.8mag C/2025 J1 (Borisov)
12:33:44.68 +52:10:58.3 16.0mag C/2025 L1 (ATLAS)
03:54:59.96 -29:13:42.7 18.0mag C/2025 Q3 (ATLAS)
04:27:30.94 -02:35:34.8 8.8mag C/2025 R3 (PANSTARRS)
12:47:05.69 +03:56:10.4 17.3mag C/2025 Y1 (ATLAS)
05:01:04.22 +01:38:17.9 16.8mag C/2026 A1 (MAPS)
00:45:38.28 +39:55:44.8 15.1mag C/2026 B2 (Sun-Gao)
19:16:36.69 -08:47:04.3 10.8mag 10P/Tempel
14:37:28.26 +00:59:56.1 15.6mag 24P/Schaumasse
10:59:33.63 -01:04:19.5 15.8mag 29P/Schwassmann-Wachmann
10:40:02.05 -03:01:27.1 17.3mag 43P/Wolf-Harrington
02:15:49.25 +20:22:10.8 17.4mag 47P/Ashbrook-Jackson
07:44:45.02 +33:05:24.6 16.9mag 63P/Wild
23:50:19.35 -09:28:32.0 15.7mag 65P/Gunn
04:52:05.14 +26:38:38.7 16.1mag 76P/West-Kohoutek-Ikemura
01:44:48.83 +11:32:51.4 14.1mag 78P/Gehrels
23:53:06.45 -04:17:17.5 14.9mag 88P/Howell
03:01:34.68 +24:53:47.8 15.0mag 93P/Lovas
05:29:40.16 +33:02:14.6 16.0mag 123P/West-Hartley
08:51:50.46 +30:23:19.9 16.3mag 124P/Mrkos
03:00:39.88 +16:13:13.3 16.4mag 128P/Shoemaker-Holt
03:22:02.50 +16:26:01.0 17.6mag 131P/Mueller
03:00:12.43 +17:57:29.7 10.8mag 141P/Machholz
03:05:57.85 +11:00:56.6 10.8mag 141P-A/Machholz
01:46:04.13 +06:51:03.5 11.0mag 141P-D/Machholz
01:51:45.94 +07:16:19.2 14.9mag 162P/SidingSpring
22:24:02.25 -07:24:59.5 18.0mag 218P/LINEAR
17:15:42.01 -11:47:36.1 16.1mag 235P/LINEAR
06:13:07.48 +35:39:14.0 17.0mag 240P/NEAT
07:48:45.31 -03:30:40.7 17.9mag 242P/Spahr
23:00:38.83 -15:51:39.2 17.4mag 260P/McNaught
02:35:31.64 +24:45:24.4 17.8mag 295P/LINEAR
15:34:23.78 +07:56:19.9 17.4mag 391P/Kowalski
07:42:29.87 +21:19:55.2 17.7mag 450P/LONEOS
06:02:19.60 +44:00:33.1 17.6mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K May 3 05:20 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
21:00:10.71 -32:17:03.90 2026-04-27.36 16.15
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:00:10.71 -32:17:03.90 2026-04-27.36 16.15
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
-rw-r--r-- 1 apache apache 188K May 3 05:20 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:51:37.106 +66:06:26.69 AT 2026knw 2026-04-20.29 20.1292
07:25:11.821 +59:27:11.75 AT 2026knv 2026-04-20.16 18.5877
10:10:53.458 +45:56:52.48 SN 2026knu 2026-04-20.18 19.5784
13:23:31.702 -27:27:16.87 AT 2026knt 2026-04-21.45 19.6
14:59:13.174 -10:47:02.79 AT 2026kns 2026-04-09.59 20.1
14:45:20.668 -24:47:31.93 AT 2026knr 2026-03-24.65 20.36
11:45:24.981 +14:40:44.45 AT 2026knq 2026-04-13.92 20.18
04:52:30.865 -15:17:09.10 AT 2026knp 2026-04-20.71 18.098
17:25:02.776 +69:43:35.23 AT 2026kno 2026-04-23.10 19.208
15:15:42.943 -39:27:45.41 AT 2026knn 2026-04-14.63 19.62
21:02:34.025 +19:12:44.83 AT 2026knm 2026-04-22.60 18.74
14:38:36.298 -39:37:27.88 AT 2026knl 2026-04-21.52 20.1
13:24:43.943 +16:55:43.96 AT 2026knk 2026-04-20.96 20.03
13:55:11.417 +21:19:35.16 AT 2026knj 2026-04-20.98 19.3
16:21:58.180 +07:39:22.34 AT 2026kni 2026-04-22.11 19.97
18:25:00.619 +56:31:13.17 AT 2026knh 2026-04-14.18 19.89
11:52:14.846 +19:25:04.67 AT 2026kng 2026-04-12.92 20.24
17:52:14.690 -78:03:43.36 AT 2026kne 2026-04-23.29 18.712
19:46:54.481 -51:39:39.32 AT 2026knd 2026-04-20.32 17.94
21:24:26.061 +26:56:11.62 AT 2026knc 2026-04-23.59 17.66
-rw-r--r-- 1 apache apache 30K May 3 05:20 tns_transients_list.txt
