This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 8.78 01:56:38.02 +59:15:33.7
131.18803 -2.56331 galactic Cas Second-epoch detections are separated by 0.6" and 7.1 pix
The object was found in VSX 1" X Cas
Type: M
# Max. Min./Amp. JD0 Period
9.450 V 13.200 V 2457020.00000 415.000000000000 C5,4e(N1e)
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 01:56:38.02 +59:15:33.7: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.02 +59:15:33.7: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 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 06 18.3032* 01 56 38.02 +59 15 33.7 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
X Cas,2461209.8032,8.78,0.05,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
X Cas 20260618.3032 8.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 11.57 01:22:51.69 +57:50:37.1
127.11821 -4.77247 galactic Cas Second-epoch detections are separated by 1.6" and 7.1 pix
The object was found in VSX 5" NSVS J0122514+575031
Type: M
# Max. Min./Amp. JD0 Period
12.515 r Y 2.242 r 2458348.91800 285.695348200000 M7
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 01:22:51.69 +57:50:37.1: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:51.69 +57:50:37.1: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 22 51.69 +57 50 37.1 11.6 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
NSVS J0122514+575031,2461209.8032,11.57,0.05,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 J0122514+575031 20260618.3032 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 11.16 01:27:37.85 +64:03:27.1
126.87821 1.46344 galactic Cas Second-epoch detections are separated by 4.2" and 7.5 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 | 01:27:37.85 +64:03:27.1 (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 01:27:37.85 +64:03:27.1: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:37.85 +64:03:27.1: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 27 37.85 +64 03 27.1 11.2 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
target,2461209.8032,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260618.3032 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 11.34 01:05:53.87 +59:06:25.8
124.79097 -3.71238 galactic Cas Second-epoch detections are separated by 1.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:05:53.87 +59:06:25.8 (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 01:05:53.87 +59:06:25.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:53.87 +59:06:25.8: 14.38 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 05 53.87 +59 06 25.8 11.3 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,2461209.8032,11.34,0.05,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 20260618.3032 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.95 01:55:46.74 +57:57:42.4
131.40312 -3.84783 galactic Per Second-epoch detections are separated by 1.3" and 7.4 pix
The object was found in VSX18" ZTF J015546.41+575800.1
Type: RS
# Max. Min./Amp. JD0 Period
13.450 r Y 0.033 r 2458379.91220 0.825740500000
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 01:55:46.74 +57:57:42.4: 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 01:55:46.74 +57:57:42.4: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 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 06 18.3032* 01 55 46.74 +57 57 42.4 10.9 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
ZTF J015546.41+575800.1,2461209.8032,10.95,0.05,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
ZTF J015546.41+575800.1 20260618.3032 10.95CV 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 06 18.3032 2461209.8032 11.18 01:07:02.02 +59:46:18.0
124.89646 -3.04058 galactic Cas Second-epoch detections are separated by 2.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:02.02 +59:46:18.0 (user input) | T | P | (position from user input) J-Ks=0.500+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:02.02 +59:46:18.0: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:02.02 +59:46:18.0: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 06 18.3032* 01 07 02.02 +59 46 18.0 11.2 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
target,2461209.8032,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260618.3032 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.96 01:10:12.08 +59:17:24.2
125.32998 -3.49430 galactic Cas Second-epoch detections are separated by 0.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.5672+59.2942 | 01:10:12.08 +59:17:24.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.414+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:12.08 +59:17:24.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:12.08 +59:17:24.2: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 06 18.3032* 01 10 12.08 +59 17 24.2 11.0 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 J017.5672+59.2942,2461209.8032,10.96,0.05,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
ATO J017.5672+59.2942 20260618.3032 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 11.09 01:22:33.36 +60:44:42.3
126.72692 -1.89717 galactic Cas Second-epoch detections are separated by 0.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:22:33.36 +60:44:42.3 (user input) | T | P | (position from user input) J-Ks=1.158+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:33.36 +60:44:42.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:33.36 +60:44:42.3: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 22 33.36 +60 44 42.3 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
target,2461209.8032,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260618.3032 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.97 01:07:39.19 +59:59:18.0
124.96073 -2.81952 galactic Cas Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:39.19 +59:59:18.0 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.19 +59:59:18.0: 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 01:07:39.19 +59:59:18.0: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 06 18.3032* 01 07 39.19 +59 59 18.0 11.0 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,2461209.8032,10.97,0.05,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
target 20260618.3032 10.97CV 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 06 18.3032 2461209.8032 10.91 01:12:10.20 +58:47:40.8
125.62105 -3.96879 galactic Cas Second-epoch detections are separated by 1.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:12:10.20 +58:47:40.8 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.040 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:10.20 +58:47:40.8: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:10.20 +58:47:40.8: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 06 18.3032* 01 12 10.20 +58 47 40.8 10.9 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,2461209.8032,10.91,0.05,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 20260618.3032 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.78 01:35:27.72 +60:33:48.0
128.31847 -1.84717 galactic Cas Second-epoch detections are separated by 1.6" and 7.2 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 509811625915787136 | 01:35:29.25 +60:33:31.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.155+/-0.047 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:27.72 +60:33:48.0: 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 01:35:27.72 +60:33:48.0: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 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 06 18.3032* 01 35 27.72 +60 33 48.0 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
Gaia DR3 509811625915787136,2461209.8032,10.78,0.05,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 509811625915787136 20260618.3032 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.97 01:12:59.90 +57:34:09.7
125.83133 -5.18096 galactic Cas Second-epoch detections are separated by 2.7" and 7.1 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 | 01:12:59.90 +57:34:09.7 (user input) | T | P | (position from user input) J-Ks=0.831+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:59.90 +57:34:09.7: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:59.90 +57:34:09.7: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 12 59.90 +57 34 09.7 11.0 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,2461209.8032,10.97,0.05,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
target 20260618.3032 10.97CV 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 06 18.3032 2461209.8032 10.71 01:26:05.70 +59:01:14.1
127.38774 -3.55100 galactic Cas Second-epoch detections are separated by 1.0" and 6.8 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 | ATO J021.5231+59.0209 | 01:26:05.70 +59:01:14.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.314+/-0.031 (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 01:26:05.70 +59:01:14.1: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.70 +59:01:14.1: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 26 05.70 +59 01 14.1 10.7 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 J021.5231+59.0209,2461209.8032,10.71,0.05,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 J021.5231+59.0209 20260618.3032 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.79 01:06:13.14 +59:33:46.6
124.80597 -3.25501 galactic Cas Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:13.14 +59:33:46.6 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:13.14 +59:33:46.6: 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 01:06:13.14 +59:33:46.6: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 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 06 18.3032* 01 06 13.14 +59 33 46.6 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,2461209.8032,10.79,0.05,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 20260618.3032 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 06 18.3032 2461209.8032 10.63 01:29:04.41 +58:45:57.7
127.80514 -3.74916 galactic Cas Second-epoch detections are separated by 2.4" and 7.4 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 | ASASSN-V J012906.85+584639.3 | 01:29:06.84 +58:46:39.2 (Gaia DR3) | L (local) | (local) | Gaia3var=VARIABLE J-Ks=0.162+/-0.260 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:04.41 +58:45:57.7: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:04.41 +58:45:57.7: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 06 18.3032* 01 29 04.41 +58 45 57.7 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
ASASSN-V J012906.85+584639.3,2461209.8032,10.63,0.05,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 J012906.85+584639.3 20260618.3032 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.85 01:25:27.74 +59:27:15.4
127.24960 -3.13193 galactic Cas Second-epoch detections are separated by 0.9" and 6.9 pix
The object was found in VSX 4" Gaia DR3 510073344036983552
Type: ROT
# Max. Min./Amp. JD0 Period
14.460 G 14.520 G 1.820050000000 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 01:25:27.74 +59:27:15.4: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:27.74 +59:27:15.4: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 06 18.3032* 01 25 27.74 +59 27 15.4 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
Gaia DR3 510073344036983552,2461209.8032,10.85,0.05,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 510073344036983552 20260618.3032 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.47 02:13:47.67 +58:44:00.9
133.45820 -2.44482 galactic Per Second-epoch detections are separated by 3.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J033.4383+58.7294 | 02:13:47.67 +58:44:00.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.232+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:47.67 +58:44:00.9: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.67 +58:44:00.9: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 02 13 47.67 +58 44 00.9 10.5 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
ATO J033.4383+58.7294,2461209.8032,10.47,0.05,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 J033.4383+58.7294 20260618.3032 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.72 01:24:55.15 +59:41:45.9
127.14967 -2.90120 galactic Cas Second-epoch detections are separated by 2.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:24:55.15 +59:41:45.9 (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 01:24:55.15 +59:41:45.9: 12.71 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:55.15 +59:41:45.9: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 06 18.3032* 01 24 55.15 +59 41 45.9 10.7 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,2461209.8032,10.72,0.05,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 20260618.3032 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.68 01:13:44.77 +57:24:51.5
125.94516 -5.32687 galactic Cas Second-epoch detections are separated by 2.5" and 7.2 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 | 01:13:44.77 +57:24:51.5 (user input) | T | P | (position from user input) J-Ks=0.655+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:44.77 +57:24:51.5: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:44.77 +57:24:51.5: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 13 44.77 +57 24 51.5 10.7 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,2461209.8032,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260618.3032 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.53 01:26:36.82 +59:41:35.3
127.36219 -2.87569 galactic Cas Second-epoch detections are separated by 1.9" and 6.8 pix
The object was found in VSX 1" Gaia DR3 510083239641443712
Type: ROT
# Max. Min./Amp. JD0 Period
13.540 G 13.590 G K
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 01:26:36.82 +59:41:35.3: 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 01:26:36.82 +59:41:35.3: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 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 06 18.3032* 01 26 36.82 +59 41 35.3 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 510083239641443712,2461209.8032,10.53,0.05,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 510083239641443712 20260618.3032 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.41 01:20:45.13 +57:55:09.4
126.82988 -4.73044 galactic Cas Second-epoch detections are separated by 1.0" and 6.9 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 413797116609704704 | 01:20:41.29 +57:55:17.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.023+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:45.13 +57:55:09.4: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:45.13 +57:55:09.4: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 20 45.13 +57 55 09.4 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 413797116609704704,2461209.8032,10.41,0.05,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 413797116609704704 20260618.3032 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.41 01:15:19.75 +57:44:09.9
126.12830 -4.98732 galactic Cas Second-epoch detections are separated by 2.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J018.8211+57.7311 | 01:15:19.75 +57:44:09.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.269+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:19.75 +57:44:09.9: 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 01:15:19.75 +57:44:09.9: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 15 19.75 +57 44 09.9 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
ATO J018.8211+57.7311,2461209.8032,10.41,0.05,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 J018.8211+57.7311 20260618.3032 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.63 01:06:25.63 +61:41:31.8
124.70829 -1.12787 galactic Cas Second-epoch detections are separated by 2.8" and 7.1 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 | 01:06:25.63 +61:41:31.8 (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 01:06:25.63 +61:41:31.8: 10.39 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:25.63 +61:41:31.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.63 +/- 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 06 18.3032* 01 06 25.63 +61 41 31.8 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
target,2461209.8032,10.63,0.05,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 20260618.3032 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.51 01:17:15.42 +58:35:37.7
126.29899 -4.10905 galactic Cas Second-epoch detections are separated by 0.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J019.3185+58.5958 | 01:17:17.58 +58:36:18.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1960IzKry..24..160B [B60] +58 130
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:15.42 +58:35:37.7: 12.76 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:15.42 +58:35:37.7: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 17 15.42 +58 35 37.7 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
ATO J019.3185+58.5958,2461209.8032,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.3185+58.5958 20260618.3032 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.07 01:43:40.25 +61:00:05.1
129.22180 -1.23084 galactic Cas Second-epoch detections are separated by 0.9" and 7.1 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 511234595807697920 | 01:43:38.40 +61:00:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.105+/-0.035 (A)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:40.25 +61:00:05.1: 11.39 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:40.25 +61:00:05.1: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 43 40.25 +61 00 05.1 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
Gaia DR3 511234595807697920,2461209.8032,10.07,0.05,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 511234595807697920 20260618.3032 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 9.60 01:28:26.88 +60:23:26.6
127.49161 -2.15296 galactic Cas Second-epoch detections are separated by 1.1" and 6.8 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 510221984265315200 | 01:28:28.01 +60:23:13.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.247+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:26.88 +60:23:26.6: 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 01:28:26.88 +60:23:26.6: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 28 26.88 +60 23 26.6 9.6 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 510221984265315200,2461209.8032,9.60,0.05,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 510221984265315200 20260618.3032 9.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.33 02:00:21.68 +64:56:36.5
130.14910 3.04195 galactic Cas Second-epoch detections are separated by 3.5" and 7.1 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 518139017740687360 | 02:00:16.12 +64:56:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9IV/V 1928MeUpp..37....1S BD+64 275 J-Ks=1.311+/-0.028 (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 02:00:21.68 +64:56:36.5: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:21.68 +64:56:36.5: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 02 00 21.68 +64 56 36.5 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 518139017740687360,2461209.8032,10.33,0.05,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 518139017740687360 20260618.3032 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.68 01:11:56.84 +58:41:03.8
125.60104 -4.08103 galactic Cas Second-epoch detections are separated by 2.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:11:56.84 +58:41:03.8 (user input) | T | P | (position from user input) J-Ks=0.669+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:56.84 +58:41:03.8: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:56.84 +58:41:03.8: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 11 56.84 +58 41 03.8 10.7 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,2461209.8032,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260618.3032 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.71 01:38:05.86 +61:04:13.3
128.54616 -1.29175 galactic Cas Second-epoch detections are separated by 0.7" and 7.0 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 | DocumentRef: VOTx966231 | 01:38:05.86 +61:04:13.3 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.901+/-0.031 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:05.86 +61:04:13.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:05.86 +61:04:13.3: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 38 05.86 +61 04 13.3 10.7 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
DocumentRef: VOTx966231,2461209.8032,10.71,0.05,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
DocumentRef: VOTx966231 20260618.3032 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.93 01:44:29.99 +65:09:23.9
128.47110 2.85712 galactic Cas Second-epoch detections are separated by 1.5" and 7.5 pix
The object was found in VSX 6" Gaia DR3 519045973088246784
Type: ROT
# Max. Min./Amp. JD0 Period
15.090 G 15.140 G 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 01:44:29.99 +65:09:23.9: 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 01:44:29.99 +65:09:23.9: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 44 29.99 +65 09 23.9 10.9 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 519045973088246784,2461209.8032,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 519045973088246784 20260618.3032 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.73 01:28:07.45 +59:53:50.6
127.52210 -2.64700 galactic Cas Second-epoch detections are separated by 1.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510182298766565376 | 01:28:11.24 +59:54:05.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.868+/-0.053 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:07.45 +59:53:50.6: 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 01:28:07.45 +59:53:50.6: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 06 18.3032* 01 28 07.45 +59 53 50.6 10.7 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 510182298766565376,2461209.8032,10.73,0.05,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 510182298766565376 20260618.3032 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.76 01:09:22.64 +57:26:31.8
125.35423 -5.34518 galactic Cas Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.3204+57.4562 | 01:09:17.29 +57:26:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.782+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.64 +57:26:31.8: 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 01:09:22.64 +57:26:31.8: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 06 18.3032* 01 09 22.64 +57 26 31.8 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
ATO J017.3204+57.4562,2461209.8032,10.76,0.05,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 J017.3204+57.4562 20260618.3032 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.85 01:13:38.93 +58:10:50.3
125.86556 -4.56454 galactic Cas Second-epoch detections are separated by 1.2" and 6.7 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 | DocumentRef: VOTx1267505 | 01:13:41.63 +58:10:34.2 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.593+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:38.93 +58:10:50.3: 13.19 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:38.93 +58:10:50.3: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 06 18.3032* 01 13 38.93 +58 10 50.3 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
DocumentRef: VOTx1267505,2461209.8032,10.85,0.05,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
DocumentRef: VOTx1267505 20260618.3032 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.69 02:00:32.96 +59:40:06.3
131.56372 -2.04008 galactic Cas Second-epoch detections are separated by 2.0" and 6.8 pix
The object was found in VSX 3" ZTF J020033.07+594008.7
Type: SR
# Max. Min./Amp. JD0 Period
13.621 r Y 0.477 r 2458342.93970 344.838134100000 C
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 02:00:32.96 +59:40:06.3: 11.57 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.96 +59:40:06.3: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 06 18.3032* 02 00 32.96 +59 40 06.3 10.7 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
ZTF J020033.07+594008.7,2461209.8032,10.69,0.05,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
ZTF J020033.07+594008.7 20260618.3032 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.92 01:06:55.45 +59:18:57.9
124.91015 -3.49617 galactic Cas Second-epoch detections are separated by 2.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:55.45 +59:18:57.9 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.45 +59:18:57.9: 13.10 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.45 +59:18:57.9: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 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 06 18.3032* 01 06 55.45 +59 18 57.9 10.9 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,2461209.8032,10.92,0.05,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 20260618.3032 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.93 01:34:07.14 +60:12:53.3
128.21321 -2.21856 galactic Cas Second-epoch detections are separated by 2.3" and 7.2 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 509777472336200448 | 01:34:01.93 +60:13:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0IV/V 1928MeUpp..37....1S BD+59 277 J-Ks=0.892+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:07.14 +60:12:53.3: 11.71 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:07.14 +60:12:53.3: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 06 18.3032* 01 34 07.14 +60 12 53.3 10.9 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 509777472336200448,2461209.8032,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509777472336200448 20260618.3032 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.81 01:54:40.24 +58:57:06.0
131.01944 -2.92360 galactic Cas Second-epoch detections are separated by 1.3" and 7.1 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 506318649266040064 | 01:54:41.53 +58:57:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1960IzKry..24..160B [B60] +58 557
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:40.24 +58:57:06.0: 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 01:54:40.24 +58:57:06.0: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 06 18.3032* 01 54 40.24 +58 57 06.0 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
Gaia DR3 506318649266040064,2461209.8032,10.81,0.05,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
Gaia DR3 506318649266040064 20260618.3032 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 06 18.3032 2461209.8032 11.04 01:26:28.47 +59:41:36.1
127.34475 -2.87786 galactic Cas Second-epoch detections are separated by 0.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.6536+59.6928 | 01:26:31.85 +59:41:21.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:28.47 +59:41:36.1: 12.90 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:28.47 +59:41:36.1: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 26 28.47 +59 41 36.1 11.0 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 J021.6536+59.6928,2461209.8032,11.04,0.05,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
ATO J021.6536+59.6928 20260618.3032 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 11.32 01:26:03.85 +62:05:29.2
126.97183 -0.50839 galactic Cas Second-epoch detections are separated by 2.7" and 7.2 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 510832797333241088 | 01:26:05.55 +62:05:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1960IzKry..24..160B [B60] +61 209
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:03.85 +62:05:29.2: 12.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:03.85 +62:05:29.2: 14.46 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 26 03.85 +62 05 29.2 11.3 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 510832797333241088,2461209.8032,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510832797333241088 20260618.3032 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 11.08 01:51:53.69 +63:26:21.8
129.62916 1.35649 galactic Cas Second-epoch detections are separated by 3.1" and 7.4 pix
The object was found in VSX12" ZTF J015152.31+632614.6
Type: EB:
# Max. Min./Amp. JD0 Period
15.451 r Y 0.389 r 2458367.82620 5.408679200000
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 01:51:53.69 +63:26:21.8: 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 01:51:53.69 +63:26:21.8: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 51 53.69 +63 26 21.8 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
ZTF J015152.31+632614.6,2461209.8032,11.08,0.05,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
ZTF J015152.31+632614.6 20260618.3032 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 11.14 02:02:25.92 +64:38:23.1
130.44326 2.80837 galactic Cas Second-epoch detections are separated by 0.6" and 7.4 pix
The object was found in VSX 0" ASASSN-V J020225.96+643822.9
Type: SR
# Max. Min./Amp. JD0 Period
14.090 V 14.200 V 2457555.11300 70.630000000000
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 02:02:25.92 +64:38:23.1: 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 02:02:25.92 +64:38:23.1: 14.22 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 02 02 25.92 +64 38 23.1 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
ASASSN-V J020225.96+643822.9,2461209.8032,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J020225.96+643822.9 20260618.3032 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 11.36 01:24:36.17 +61:08:55.0
126.92335 -1.46585 galactic Cas Second-epoch detections are separated by 0.6" and 6.9 pix
The object was found in VSX 0" Gaia DR3 510685394056841344
Type: ROT
# Max. Min./Amp. JD0 Period
14.210 G 14.240 G 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 01:24:36.17 +61:08:55.0: 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 01:24:36.17 +61:08:55.0: 14.37 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 24 36.17 +61 08 55.0 11.4 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 510685394056841344,2461209.8032,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510685394056841344 20260618.3032 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 11.46 01:23:42.21 +61:03:02.2
126.82794 -1.57683 galactic Cas Second-epoch detections are separated by 3.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx1219036 | 01:23:42.21 +61:03:02.2 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.439+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:42.21 +61:03:02.2: 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 01:23:42.21 +61:03:02.2: 14.86 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 23 42.21 +61 03 02.2 11.5 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
DocumentRef: VOTx1219036,2461209.8032,11.46,0.05,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
DocumentRef: VOTx1219036 20260618.3032 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 11.24 02:00:34.64 +59:38:08.0
131.57583 -2.07083 galactic Cas Second-epoch detections are separated by 1.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx1175694 | 02:00:31.93 +59:38:38.8 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE J-Ks=0.861+/-0.043 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:34.64 +59:38:08.0: 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 02:00:34.64 +59:38:08.0: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.18 +/- 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 06 18.3032* 02 00 34.64 +59 38 08.0 11.2 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
DocumentRef: VOTx1175694,2461209.8032,11.24,0.05,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
DocumentRef: VOTx1175694 20260618.3032 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.07 02:13:47.59 +63:11:26.4
132.06241 1.78818 galactic Cas Second-epoch detections are separated by 2.2" and 7.5 pix
The object was found in VSX 1" NSVS J0213478+631127
Type: L:
# Max. Min./Amp. JD0 Period
11.122 R1 Y 0.644 R1 355.000000000000
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 02:13:47.59 +63:11:26.4: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.59 +63:11:26.4: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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 06 18.3032* 02 13 47.59 +63 11 26.4 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
NSVS J0213478+631127,2461209.8032,10.07,0.05,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 J0213478+631127 20260618.3032 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.41 01:33:44.53 +60:46:17.5
128.07597 -1.67700 galactic Cas Second-epoch detections are separated by 7.3" and 8.2 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 | 01:33:44.53 +60:46:17.5 (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 01:33:44.53 +60:46:17.5: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.53 +60:46:17.5: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.3032* 01 33 44.53 +60 46 17.5 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
target,2461209.8032,10.41,0.05,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 20260618.3032 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.3032 2461209.8032 10.18 02:21:53.12 +64:19:49.8
132.53402 3.15815 galactic Cas Second-epoch detections are separated by 0.3" and 7.3 pix
The object was found in VSX 1" NSVS 1870695
Type: EW
# Max. Min./Amp. JD0 Period
13.211 r Y 0.502 r 2458334.94920 0.787347000000
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 02:21:53.12 +64:19:49.8: 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 02:21:53.12 +64:19:49.8: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 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 06 18.3032* 02 21 53.12 +64 19 49.8 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
NSVS 1870695,2461209.8032,10.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1870695 20260618.3032 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461209.80354972 18.06.2026 07:16:56.696 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
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: 17 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): 25774
Objects passed selection criteria: 25636
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 18052.2
Average stars matched: 16531.5 (91.5758 %)
Memory usage VmPeak: 128420 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 18 02:40:57 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: 2461209.80354972 18.06.2026 07:16:56.696 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 185
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: 94 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): 187652
Objects passed selection criteria: 187176
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 137816
Average stars matched: 126250 (91.6075 %)
Memory usage VmPeak: 1938348 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 18 02:47:14 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_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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: 2461209.80291618
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_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits'
wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
Image size: 938.7'x624.4' 15.6(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: 01:42:49.422 +61:59:51.75 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 01:42:49.422 +61:59:51.75
Angular distance between the image centers 0.0424 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
Image size: 938.7'x624.4' 15.6(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: 01:42:50.121 +61:59:09.84 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 01:42:50.121 +61:59:09.84
Angular distance between the image centers 0.0419 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 01:42:49.422 +61:59:51.75
Second-epoch second image center 01:42:50.121 +61:59:09.84
Angular distance between the image centers 0.01172 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.mp2oULjnlU
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.xB8V0bP617
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_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits &> /tmp/tmp.B7KvevZuWx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits &> /tmp/tmp.xEpnYHnFcJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_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.wcscat
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.wcscat
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.wcscat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat' -> '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 4 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_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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
14.1 mag. fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
14.0 mag. fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.5 (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.mp2oULjnlU (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_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/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.wcscat 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.wcscat 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.wcscat
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.wcscat
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)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=331 sigma_overall_arcsec=7.729 sigma_q1_arcsec=31.346 sigma_q2_arcsec=12.794 sigma_q3_arcsec=22.422 sigma_q4_arcsec=4.202 n_q1=16 n_q2=97 n_q3=37 n_q4=181 worst_quadrant_to_overall_ratio=4.055
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.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.wcscat.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.wcscat.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.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xB8V0bP617 (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_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/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.wcscat 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.wcscat 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.wcscat
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.wcscat
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! :)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=973 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.346 n_q1=119 n_q2=244 n_q3=303 n_q4=307 worst_quadrant_to_overall_ratio=1.316
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.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.wcscat.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.wcscat.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.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.B7KvevZuWx (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.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_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1127, passed=15114
Got 15114 stars (including 13979 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat
util/solve_plate_with_UCAC5 got 15114 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 14713 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 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 14713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 14714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits N_match=969 sigma_overall_arcsec=0.617 sigma_q1_arcsec=0.559 sigma_q2_arcsec=0.595 sigma_q3_arcsec=0.713 sigma_q4_arcsec=0.618 n_q1=297 n_q2=292 n_q3=246 n_q4=134 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xEpnYHnFcJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1116, passed=15032
Got 15032 stars (including 13905 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat
util/solve_plate_with_UCAC5 got 15032 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 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: 967 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 14728 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 728 to 788 (Dec 55.8 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(), 14726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 14726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits N_match=967 sigma_overall_arcsec=0.633 sigma_q1_arcsec=0.564 sigma_q2_arcsec=0.625 sigma_q3_arcsec=0.699 sigma_q4_arcsec=0.653 n_q1=293 n_q2=272 n_q3=251 n_q4=151 worst_quadrant_to_overall_ratio=1.105
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=7.729 worst_q_ratio=4.055
ref2=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.405 worst_q_ratio=1.316
new1=fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits sigma_overall=0.617 worst_q_ratio=1.155
new2=fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits sigma_overall=0.633 worst_q_ratio=1.105
reference average sigma_overall=4.067 worst_q_ratio=2.6855
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png (331 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.16 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png (973 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248_astrometric_residuals.png (969 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.58 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249_astrometric_residuals.png (967 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.59 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:51.69 +57:50:37.1: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.02 +59:15:33.7: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.02 +59:15:33.7: 9.75 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:51.69 +57:50:37.1: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Forced photometry filter KEPT candidate at 01:56:38.02 +59:15:33.7: ref_mag=9.75 +/- 0.00 new_mean_mag=8.7767 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 01:22:51.69 +57:50:37.1: ref_mag=12.53 +/- 0.02 new_mean_mag=11.5674 delta=0.96 (need > 0.90)
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29658.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02633_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 02633_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:15:23.63 +65:01:39.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 08339_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:20:32.63 +62:32:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20109_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 20109_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29658_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 29658_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
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 ####
01:56:38.02 +59:15:33.7
01:22:51.69 +57:50:37.1
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_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
Image size: 938.7'x624.4' 15.6(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: 01:42:49.422 +61:59:51.75 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 01:42:49.422 +61:59:51.75
Angular distance between the image centers 0.0424 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
Image size: 938.7'x624.4' 15.6(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: 01:42:50.121 +61:59:09.84 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 01:42:50.121 +61:59:09.84
Angular distance between the image centers 0.0419 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 01:42:49.422 +61:59:51.75
Second-epoch second image center 01:42:50.121 +61:59:09.84
Angular distance between the image centers 0.01172 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.CIIina5gl8
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.U3m2thQI9e
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_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits &> /tmp/tmp.OMjZ5chApD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits &> /tmp/tmp.tjYQHLtpjB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_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.wcscat
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.wcscat
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.wcscat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat' -> '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 153 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_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
2.3 pix fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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
11.6 mag. fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
11.6 mag. fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 11.1 (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.CIIina5gl8 (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_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/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.wcscat 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.wcscat 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.wcscat
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.wcscat
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)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=344 sigma_overall_arcsec=7.924 sigma_q1_arcsec=24.049 sigma_q2_arcsec=13.165 sigma_q3_arcsec=21.493 sigma_q4_arcsec=4.815 n_q1=16 n_q2=127 n_q3=29 n_q4=172 worst_quadrant_to_overall_ratio=3.035
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.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.wcscat.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.wcscat.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.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.U3m2thQI9e (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_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/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.wcscat 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.wcscat 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.wcscat
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.wcscat
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! :)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=974 sigma_overall_arcsec=0.370 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.313 n_q1=145 n_q2=246 n_q3=288 n_q4=295 worst_quadrant_to_overall_ratio=1.210
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.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.wcscat.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.wcscat.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.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OMjZ5chApD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.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_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=11184, passed=109231
Got 109231 stars (including 97921 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat
util/solve_plate_with_UCAC5 got 109231 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 970 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(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 107077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 970 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(), 107079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 107079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits N_match=967 sigma_overall_arcsec=0.582 sigma_q1_arcsec=0.504 sigma_q2_arcsec=0.565 sigma_q3_arcsec=0.690 sigma_q4_arcsec=0.603 n_q1=292 n_q2=301 n_q3=225 n_q4=149 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tjYQHLtpjB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=11387, passed=110549
Got 110549 stars (including 99048 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat
util/solve_plate_with_UCAC5 got 110549 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 108960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 974 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(), 108959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 108978 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits N_match=970 sigma_overall_arcsec=0.634 sigma_q1_arcsec=0.561 sigma_q2_arcsec=0.582 sigma_q3_arcsec=0.671 sigma_q4_arcsec=0.619 n_q1=292 n_q2=282 n_q3=231 n_q4=165 worst_quadrant_to_overall_ratio=1.058
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-01_20.00sec_4.90C_LIGHT_0248.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-18_CI_Cas-03-Q2b1x1_023805_TTUQ2b1x1_2557567_7rmo2WtY/wcs_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249.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 01:27:37.85 +64:03:27.1: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:12.08 +59:17:24.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.19 +59:59:18.0: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:53.87 +59:06:25.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:33.36 +60:44:42.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:02.02 +59:46:18.0: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:46.74 +57:57:42.4: 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 01:12:10.20 +58:47:40.8: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:33.36 +60:44:42.3: 14.11 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:02.02 +59:46:18.0: 13.81 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:46.74 +57:57:42.4: 13.90 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:37.85 +64:03:27.1: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.05
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Forced photometry filter KEPT candidate at 01:07:02.02 +59:46:18.0: ref_mag=13.81 +/- 0.05 new_mean_mag=11.1839 delta=2.62 (need > 0.90)
Forced photometry filter KEPT candidate at 01:55:46.74 +57:57:42.4: ref_mag=13.90 +/- 0.05 new_mean_mag=10.9418 delta=2.96 (need > 0.90)
Forced photometry reference-image weighted average: 14.11 +/- 0.06
Forced photometry filter KEPT candidate at 01:22:33.36 +60:44:42.3: ref_mag=14.11 +/- 0.06 new_mean_mag=11.0650 delta=3.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:27.72 +60:33:48.0: 13.28 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter KEPT candidate at 01:27:37.85 +64:03:27.1: ref_mag=13.41 +/- 0.03 new_mean_mag=11.1586 delta=2.25 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:53.87 +59:06:25.8: 14.38 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.08
Forced photometry filter KEPT candidate at 01:05:53.87 +59:06:25.8: ref_mag=14.38 +/- 0.08 new_mean_mag=11.3254 delta=3.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.19 +59:59:18.0: 13.74 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:12.08 +59:17:24.2: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Forced photometry filter KEPT candidate at 01:07:39.19 +59:59:18.0: ref_mag=13.74 +/- 0.04 new_mean_mag=10.9645 delta=2.78 (need > 0.90)
Forced photometry filter KEPT candidate at 01:10:12.08 +59:17:24.2: ref_mag=13.87 +/- 0.05 new_mean_mag=10.9517 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:10.20 +58:47:40.8: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 01:12:10.20 +58:47:40.8: ref_mag=13.65 +/- 0.04 new_mean_mag=10.9147 delta=2.73 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:27.72 +60:33:48.0: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry filter KEPT candidate at 01:35:27.72 +60:33:48.0: ref_mag=13.60 +/- 0.04 new_mean_mag=10.7726 delta=2.82 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:59.90 +57:34:09.7: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:59.90 +57:34:09.7: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.06
Forced photometry filter KEPT candidate at 01:12:59.90 +57:34:09.7: ref_mag=13.83 +/- 0.06 new_mean_mag=10.9577 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 01:26:05.70 +59:01:14.1: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.70 +59:01:14.1: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.06
Forced photometry filter KEPT candidate at 01:26:05.70 +59:01:14.1: ref_mag=13.91 +/- 0.06 new_mean_mag=10.7111 delta=3.20 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:13.14 +59:33:46.6: 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 01:06:13.14 +59:33:46.6: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Forced photometry filter KEPT candidate at 01:06:13.14 +59:33:46.6: ref_mag=13.58 +/- 0.04 new_mean_mag=10.7797 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 01:29:04.41 +58:45:57.7: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:27.74 +59:27:15.4: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:04.41 +58:45:57.7: 13.70 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:47.67 +58:44:00.9: 13.26 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.70 +/- 0.05
Forced photometry filter KEPT candidate at 01:29:04.41 +58:45:57.7: ref_mag=13.70 +/- 0.05 new_mean_mag=10.6106 delta=3.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:27.74 +59:27:15.4: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Forced photometry filter KEPT candidate at 01:25:27.74 +59:27:15.4: ref_mag=13.95 +/- 0.05 new_mean_mag=10.8450 delta=3.11 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.67 +58:44:00.9: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 02:13:47.67 +58:44:00.9: ref_mag=13.07 +/- 0.02 new_mean_mag=10.4729 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 01:24:55.15 +59:41:45.9: 12.71 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:55.15 +59:41:45.9: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Forced photometry filter KEPT candidate at 01:24:55.15 +59:41:45.9: ref_mag=13.89 +/- 0.05 new_mean_mag=10.7227 delta=3.17 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:44.77 +57:24:51.5: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:36.82 +59:41:35.3: 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 01:13:44.77 +57:24:51.5: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Forced photometry filter KEPT candidate at 01:13:44.77 +57:24:51.5: ref_mag=13.46 +/- 0.03 new_mean_mag=10.6746 delta=2.79 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:36.82 +59:41:35.3: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.05
Forced photometry filter KEPT candidate at 01:26:36.82 +59:41:35.3: ref_mag=13.64 +/- 0.05 new_mean_mag=10.5273 delta=3.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:45.13 +57:55:09.4: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:45.13 +57:55:09.4: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter KEPT candidate at 01:20:45.13 +57:55:09.4: ref_mag=13.32 +/- 0.03 new_mean_mag=10.3932 delta=2.93 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:19.75 +57:44:09.9: 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 01:15:19.75 +57:44:09.9: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 01:15:19.75 +57:44:09.9: ref_mag=13.40 +/- 0.03 new_mean_mag=10.3875 delta=3.02 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:25.63 +61:41:31.8: 10.39 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:25.63 +61:41:31.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.02
Forced photometry filter KEPT candidate at 01:06:25.63 +61:41:31.8: ref_mag=11.63 +/- 0.02 new_mean_mag=10.6268 delta=1.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:15.42 +58:35:37.7: 12.76 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:15.42 +58:35:37.7: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Forced photometry filter KEPT candidate at 01:17:15.42 +58:35:37.7: ref_mag=13.47 +/- 0.04 new_mean_mag=10.5038 delta=2.96 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:40.25 +61:00:05.1: 11.39 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:40.25 +61:00:05.1: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Forced photometry filter KEPT candidate at 01:43:40.25 +61:00:05.1: ref_mag=12.57 +/- 0.02 new_mean_mag=10.0087 delta=2.56 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:10.50 +60:37:30.1: 7.64 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:10.50 +60:37:30.1: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 7.96 +/- 0.01
Forced photometry filter REJECTED candidate at 01:33:10.50 +60:37:30.1: ref_mag=7.96 +/- 0.01 new_mean_mag=10.2607 delta=-2.30 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:26.88 +60:23:26.6: 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 01:28:26.88 +60:23:26.6: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter KEPT candidate at 01:28:26.88 +60:23:26.6: ref_mag=12.45 +/- 0.01 new_mean_mag=9.5729 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 02:00:21.68 +64:56:36.5: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:21.68 +64:56:36.5: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Forced photometry filter KEPT candidate at 02:00:21.68 +64:56:36.5: ref_mag=13.47 +/- 0.04 new_mean_mag=10.3267 delta=3.14 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:05.29 +57:15:17.1: 10.03 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:05.29 +57:15:17.1: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.02
Forced photometry filter REJECTED candidate at 01:09:05.29 +57:15:17.1: ref_mag=10.87 +/- 0.02 new_mean_mag=10.6102 delta=0.26 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:56.84 +58:41:03.8: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:56.84 +58:41:03.8: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.06
Forced photometry filter KEPT candidate at 01:11:56.84 +58:41:03.8: ref_mag=13.85 +/- 0.06 new_mean_mag=10.6760 delta=3.17 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:05.86 +61:04:13.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:29.99 +65:09:23.9: 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 01:38:05.86 +61:04:13.3: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.06
Forced photometry filter KEPT candidate at 01:38:05.86 +61:04:13.3: ref_mag=13.87 +/- 0.06 new_mean_mag=10.7065 delta=3.17 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:29.99 +65:09:23.9: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.06
Forced photometry filter KEPT candidate at 01:44:29.99 +65:09:23.9: ref_mag=14.00 +/- 0.06 new_mean_mag=10.8657 delta=3.14 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:07.45 +59:53:50.6: 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 01:09:22.64 +57:26:31.8: 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 01:28:07.45 +59:53:50.6: 13.89 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.64 +57:26:31.8: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Forced photometry filter KEPT candidate at 01:28:07.45 +59:53:50.6: ref_mag=13.89 +/- 0.05 new_mean_mag=10.7307 delta=3.16 (need > 0.90)
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Forced photometry filter KEPT candidate at 01:09:22.64 +57:26:31.8: ref_mag=13.88 +/- 0.05 new_mean_mag=10.7572 delta=3.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:38.93 +58:10:50.3: 13.19 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:38.93 +58:10:50.3: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter KEPT candidate at 01:13:38.93 +58:10:50.3: ref_mag=13.75 +/- 0.04 new_mean_mag=10.8441 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 02:00:32.96 +59:40:06.3: 11.57 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.96 +59:40:06.3: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.05
Forced photometry filter KEPT candidate at 02:00:32.96 +59:40:06.3: ref_mag=12.96 +/- 0.05 new_mean_mag=10.6925 delta=2.27 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:45.97 +60:45:59.4: 10.47 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:45.97 +60:45:59.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.02
Forced photometry filter REJECTED candidate at 01:42:45.97 +60:45:59.4: ref_mag=11.49 +/- 0.02 new_mean_mag=10.6834 delta=0.81 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.45 +59:18:57.9: 13.10 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:07.14 +60:12:53.3: 11.71 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.45 +59:18:57.9: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter KEPT candidate at 01:06:55.45 +59:18:57.9: ref_mag=13.82 +/- 0.05 new_mean_mag=10.9053 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:07.14 +60:12:53.3: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.05
Forced photometry filter KEPT candidate at 01:34:07.14 +60:12:53.3: ref_mag=13.32 +/- 0.05 new_mean_mag=10.9350 delta=2.39 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:40.24 +58:57:06.0: 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 01:54:40.24 +58:57:06.0: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.05
Forced photometry filter KEPT candidate at 01:54:40.24 +58:57:06.0: ref_mag=13.97 +/- 0.05 new_mean_mag=10.8138 delta=3.16 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:28.47 +59:41:36.1: 12.90 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:28.47 +59:41:36.1: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.06
Forced photometry filter KEPT candidate at 01:26:28.47 +59:41:36.1: ref_mag=14.00 +/- 0.06 new_mean_mag=11.0308 delta=2.97 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:03.85 +62:05:29.2: 12.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:03.85 +62:05:29.2: 14.46 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.09
Forced photometry filter KEPT candidate at 01:26:03.85 +62:05:29.2: ref_mag=14.46 +/- 0.09 new_mean_mag=11.3081 delta=3.15 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:53.69 +63:26:21.8: 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 01:51:53.69 +63:26:21.8: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Forced photometry filter KEPT candidate at 01:51:53.69 +63:26:21.8: ref_mag=14.17 +/- 0.06 new_mean_mag=11.0381 delta=3.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:25.92 +64:38:23.1: 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 02:02:25.92 +64:38:23.1: 14.22 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.08
Forced photometry filter KEPT candidate at 02:02:25.92 +64:38:23.1: ref_mag=14.22 +/- 0.08 new_mean_mag=11.0917 delta=3.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:36.17 +61:08:55.0: 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 01:24:36.17 +61:08:55.0: 14.37 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.08
Forced photometry filter KEPT candidate at 01:24:36.17 +61:08:55.0: ref_mag=14.37 +/- 0.08 new_mean_mag=11.3425 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 01:23:42.21 +61:03:02.2: 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 01:23:42.21 +61:03:02.2: 14.86 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.11
Forced photometry filter KEPT candidate at 01:23:42.21 +61:03:02.2: ref_mag=14.86 +/- 0.11 new_mean_mag=11.4624 delta=3.40 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:34.64 +59:38:08.0: 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 02:00:34.64 +59:38:08.0: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.07
Forced photometry filter KEPT candidate at 02:00:34.64 +59:38:08.0: ref_mag=14.18 +/- 0.07 new_mean_mag=11.2275 delta=2.95 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:47.59 +63:11:26.4: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.59 +63:11:26.4: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.05
Forced photometry filter KEPT candidate at 02:13:47.59 +63:11:26.4: ref_mag=13.94 +/- 0.05 new_mean_mag=10.0668 delta=3.87 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:44.53 +60:46:17.5: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.53 +60:46:17.5: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 01:33:44.53 +60:46:17.5: ref_mag=13.40 +/- 0.03 new_mean_mag=10.3461 delta=3.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:53.12 +64:19:49.8: 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 02:21:53.12 +64:19:49.8: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Forced photometry filter KEPT candidate at 02:21:53.12 +64:19:49.8: ref_mag=13.92 +/- 0.05 new_mean_mag=10.1752 delta=3.74 (need > 0.90)
Adding exclusion_list_local.txt__out125111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out273140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out273867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out274677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out274780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out274997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out275235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58464.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 302s
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: 33s
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Considering the candidate 247669_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247669_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247671_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247671_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247676_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247676_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247680_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247680_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247703_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247703_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 247704_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247704_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247709_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247709_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:30:06.61 +61:51:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247710_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247710_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247712_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247712_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247714_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247714_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:33:01.66 +59:16:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247718_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247718_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247721_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247721_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:09:21.37 +64:35:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247724_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247724_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247729_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247729_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247736_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247736_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247738_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247738_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247740_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247740_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:10:03.19 +57:48:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247742_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247742_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247743_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247743_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247745_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247745_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:14:01.68 +57:40:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247746_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247746_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247749_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247749_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247750_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247750_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:33:35.37 +59:56:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247753_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247753_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:07:35.13 +57:33:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247755_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247755_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:03:21.91 +57:48:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247757_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247757_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247764_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247764_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247765_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247765_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247766_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247766_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247769_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247769_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247771_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247771_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247774_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247774_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:19:24.13 +58:26:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247778_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247778_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247779_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247779_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 247781_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247781_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:07:34.05 +60:52:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247782_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247782_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:10:37.65 +57:22:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247785_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247785_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:14:45.27 +60:30:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247786_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247786_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:55:14.67 +59:32:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247787_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247787_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:25:26.59 +60:57:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247788_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247788_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:07:08.10 +57:44:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247790_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 247790_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 247791_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247791_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:43:59.32 +61:55:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247794_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247794_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:15:30.74 +63:53:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247796_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247796_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:22:08.42 +60:22:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247797_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247797_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:16:01.02 +62:41:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247798_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 247798_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:47:13.07 +57:44:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252488_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 252488_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:19:11.18 +58:20:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252904_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 252904_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:17:59.22 +57:47:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252925_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 252925_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:38:00.50 +57:56:45.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253251_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 253251_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:26:41.17 +60:46:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253992_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 253992_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:46:08.59 +61:12:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254422_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 254422_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:26:46.70 +57:46:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256395_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 256395_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:18:14.22 +61:44:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256432_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 256432_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:20:11.07 +58:12:09.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 256552_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 256552_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:16:08.64 +58:49:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258453_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 258453_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:15:58.95 +63:12:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259310_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 259310_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:16:05.36 +58:49:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259843_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 259843_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:34:10.42 +62:09:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260389_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 260389_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:42:33.21 +63:52:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260789_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 260789_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:13:36.15 +57:52:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260929_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 260929_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:35:50.66 +61:27:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260962_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 260962_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:19:03.85 +63:57:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261019_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 261019_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:00:51.83 +58:31:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261257_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 261257_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:33:23.20 +57:44:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261328_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 261328_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 261396_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 261396_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:43:03.45 +58:08:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261432_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 261432_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:44:32.39 +58:45:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261508_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 261508_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:04:26.78 +65:05:52.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261970_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 261970_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:19:41.47 +62:51:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262118_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 262118_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:46:33.69 +61:16:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262246_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 262246_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:11:23.12 +61:21:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262530_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 262530_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:00:36.91 +58:30:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262581_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 262581_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:31:32.60 +61:02:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262962_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 262962_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:06:23.52 +62:44:03.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263045_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 263045_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:39:57.15 +60:52:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263158_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 263158_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:58:40.09 +59:16:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263714_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 263714_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:16:24.34 +58:04:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263816_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 263816_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:16:02.36 +58:50:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263873_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 263873_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:14:29.86 +63:16:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263927_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 263927_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 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 264000_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 264000_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:38:07.76 +61:01:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264204_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 264204_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:43:12.74 +64:00:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264304_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 264304_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:02:50.70 +60:13:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264330_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 264330_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
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Considering the candidate 264555_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 264555_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:23:07.65 +61:11:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264672_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 264672_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:38:33.92 +60:47:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264947_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 264947_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:14:00.66 +59:02:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265300_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 265300_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:14:21.83 +59:59:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265318_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 265318_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 265335_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 265335_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:55:53.11 +64:15:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265338_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 265338_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:37:13.55 +58:38:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265473_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 265473_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:02:54.01 +60:15:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265551_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 265551_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:38:12.20 +61:01:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265594_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 265594_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:33:25.05 +58:21:30.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 265851_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 265851_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:58:04.93 +59:36:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265878_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 265878_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:43:07.03 +58:57:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265907_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 265907_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 266121_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 266121_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:31:29.29 +58:12:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266224_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 266224_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:54:30.00 +59:06:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266250_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 266250_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
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Considering the candidate 266495_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 266495_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:08:30.83 +58:24:15.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266643_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 266643_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266703_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 266703_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:58:04.34 +57:58:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266716_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 266716_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266719_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 266719_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266845_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 266845_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:37:13.41 +58:38:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266887_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 266887_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:55:22.21 +64:02:58.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267474_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 267474_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267625_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 267625_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:38:34.10 +58:07:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267668_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 267668_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:44:56.81 +59:46:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267762_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 267762_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:15:05.41 +64:08:39.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267776_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 267776_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:27:04.14 +64:43:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267936_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 267936_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268138_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 268138_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:31:48.35 +64:22:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268255_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 268255_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268633_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 268633_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:54:34.85 +59:52:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268643_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 268643_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:59:06.14 +59:55:34.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268707_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 268707_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268866_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 268866_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:44:28.19 +60:41:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269040_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 269040_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269108_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 269108_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269495_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 269495_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:17:01.78 +63:21:37.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269570_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 269570_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:10:32.85 +59:59:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270201_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 270201_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:34:42.80 +58:42:16.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270227_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 270227_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:49:06.30 +65:23:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270300_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 270300_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270525_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 270525_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270905_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 270905_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:49:34.39 +61:03:37.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271104_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 271104_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:21:23.93 +63:43:15.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271169_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 271169_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:48:39.94 +59:09:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271274_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 271274_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:14:00.42 +61:42:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271309_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 271309_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:56:06.31 +60:57:13.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271448_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 271448_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:48:35.08 +58:41:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271552_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 271552_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:55:05.12 +59:57:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 273140_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 273140_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273189_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 273189_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:43:03.39 +58:57:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 273867_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 273867_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 274677_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 274677_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 274780_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 274780_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 274997_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 274997_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 275235_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 275235_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156692_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 156692_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:56:38.04 +59:15:33.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173490_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 173490_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:22:51.74 +57:50:36.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 70271_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:20:32.59 +62:32:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 72532_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:45:35.75 +63:07:03.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 112593_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:21:55.10 +61:20:58.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58464_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 58464_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125111_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 125111_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21138_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 21138_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:15:23.56 +65:01:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34158_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 34158_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:39:32.60 +64:53:05.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 76113_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 02:02:02.20 +62:41:31.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
The candidate 39378_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249 did not pass the final checks
**** FOUND 01:47:55.54 +64:32:55.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29960_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
Preparing report for the candidate 29960_fd_Cas-03-Q2b1x1_2026-06-18_02-16-56_20.00sec_5.00C_LIGHT_0249
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 337s
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 ####
01:56:38.02 +59:15:33.7
01:22:51.69 +57:50:37.1
01:33:44.53 +60:46:17.5
01:27:37.85 +64:03:27.1
01:05:53.87 +59:06:25.8
01:55:46.74 +57:57:42.4
01:07:02.02 +59:46:18.0
01:10:12.08 +59:17:24.2
01:22:33.36 +60:44:42.3
01:07:39.19 +59:59:18.0
01:12:10.20 +58:47:40.8
01:35:27.72 +60:33:48.0
01:12:59.90 +57:34:09.7
01:26:05.70 +59:01:14.1
01:06:13.14 +59:33:46.6
01:29:04.41 +58:45:57.7
01:25:27.74 +59:27:15.4
02:13:47.67 +58:44:00.9
01:24:55.15 +59:41:45.9
01:13:44.77 +57:24:51.5
01:26:36.82 +59:41:35.3
01:20:45.13 +57:55:09.4
01:15:19.75 +57:44:09.9
01:06:25.63 +61:41:31.8
01:17:15.42 +58:35:37.7
01:43:40.25 +61:00:05.1
01:28:26.88 +60:23:26.6
02:00:21.68 +64:56:36.5
01:11:56.84 +58:41:03.8
01:38:05.86 +61:04:13.3
01:44:29.99 +65:09:23.9
01:28:07.45 +59:53:50.6
01:09:22.64 +57:26:31.8
01:13:38.93 +58:10:50.3
02:00:32.96 +59:40:06.3
01:06:55.45 +59:18:57.9
01:34:07.14 +60:12:53.3
01:54:40.24 +58:57:06.0
01:26:28.47 +59:41:36.1
01:26:03.85 +62:05:29.2
01:51:53.69 +63:26:21.8
02:02:25.92 +64:38:23.1
01:24:36.17 +61:08:55.0
01:23:42.21 +61:03:02.2
02:00:34.64 +59:38:08.0
02:21:53.12 +64:19:49.8
02:13:47.59 +63:11:26.4
########### 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 ####
01:56:38.02 +59:15:33.7
01:22:51.69 +57:50:37.1
01:27:37.85 +64:03:27.1
01:05:53.87 +59:06:25.8
01:55:46.74 +57:57:42.4
01:07:02.02 +59:46:18.0
01:10:12.08 +59:17:24.2
01:22:33.36 +60:44:42.3
01:07:39.19 +59:59:18.0
01:12:10.20 +58:47:40.8
01:35:27.72 +60:33:48.0
01:12:59.90 +57:34:09.7
01:26:05.70 +59:01:14.1
01:06:13.14 +59:33:46.6
01:29:04.41 +58:45:57.7
01:25:27.74 +59:27:15.4
02:13:47.67 +58:44:00.9
01:24:55.15 +59:41:45.9
01:13:44.77 +57:24:51.5
01:26:36.82 +59:41:35.3
01:20:45.13 +57:55:09.4
01:15:19.75 +57:44:09.9
01:06:25.63 +61:41:31.8
01:17:15.42 +58:35:37.7
01:43:40.25 +61:00:05.1
01:28:26.88 +60:23:26.6
02:00:21.68 +64:56:36.5
01:11:56.84 +58:41:03.8
01:38:05.86 +61:04:13.3
01:44:29.99 +65:09:23.9
01:28:07.45 +59:53:50.6
01:09:22.64 +57:26:31.8
01:13:38.93 +58:10:50.3
02:00:32.96 +59:40:06.3
01:06:55.45 +59:18:57.9
01:34:07.14 +60:12:53.3
01:54:40.24 +58:57:06.0
01:26:28.47 +59:41:36.1
01:26:03.85 +62:05:29.2
01:51:53.69 +63:26:21.8
02:02:25.92 +64:38:23.1
01:24:36.17 +61:08:55.0
01:23:42.21 +61:03:02.2
02:00:34.64 +59:38:08.0
02:13:47.59 +63:11:26.4
01:33:44.53 +60:46:17.5
02:21:53.12 +64:19:49.8
###################################################################################
01:56:38.02 +59:15:33.7 -- not an asteroid (will add it to exclusion list)
01:22:51.69 +57:50:37.1 -- not an asteroid (will add it to exclusion list)
01:27:37.85 +64:03:27.1 -- not an asteroid (will add it to exclusion list)
01:05:53.87 +59:06:25.8 -- not an asteroid (will add it to exclusion list)
01:55:46.74 +57:57:42.4 -- not an asteroid (will add it to exclusion list)
01:07:02.02 +59:46:18.0 -- not an asteroid (will add it to exclusion list)
01:10:12.08 +59:17:24.2 -- not an asteroid (will add it to exclusion list)
01:22:33.36 +60:44:42.3 -- not an asteroid (will add it to exclusion list)
01:07:39.19 +59:59:18.0 -- not an asteroid (will add it to exclusion list)
01:12:10.20 +58:47:40.8 -- not an asteroid (will add it to exclusion list)
01:35:27.72 +60:33:48.0 -- not an asteroid (will add it to exclusion list)
01:12:59.90 +57:34:09.7 -- not an asteroid (will add it to exclusion list)
01:26:05.70 +59:01:14.1 -- not an asteroid (will add it to exclusion list)
01:06:13.14 +59:33:46.6 -- not an asteroid (will add it to exclusion list)
01:29:04.41 +58:45:57.7 -- not an asteroid (will add it to exclusion list)
01:25:27.74 +59:27:15.4 -- not an asteroid (will add it to exclusion list)
02:13:47.67 +58:44:00.9 -- not an asteroid (will add it to exclusion list)
01:24:55.15 +59:41:45.9 -- not an asteroid (will add it to exclusion list)
01:13:44.77 +57:24:51.5 -- not an asteroid (will add it to exclusion list)
01:26:36.82 +59:41:35.3 -- not an asteroid (will add it to exclusion list)
01:20:45.13 +57:55:09.4 -- not an asteroid (will add it to exclusion list)
01:15:19.75 +57:44:09.9 -- not an asteroid (will add it to exclusion list)
01:06:25.63 +61:41:31.8 -- not an asteroid (will add it to exclusion list)
01:17:15.42 +58:35:37.7 -- not an asteroid (will add it to exclusion list)
01:43:40.25 +61:00:05.1 -- not an asteroid (will add it to exclusion list)
01:28:26.88 +60:23:26.6 -- not an asteroid (will add it to exclusion list)
02:00:21.68 +64:56:36.5 -- not an asteroid (will add it to exclusion list)
01:11:56.84 +58:41:03.8 -- not an asteroid (will add it to exclusion list)
01:38:05.86 +61:04:13.3 -- not an asteroid (will add it to exclusion list)
01:44:29.99 +65:09:23.9 -- not an asteroid (will add it to exclusion list)
01:28:07.45 +59:53:50.6 -- not an asteroid (will add it to exclusion list)
01:09:22.64 +57:26:31.8 -- not an asteroid (will add it to exclusion list)
01:13:38.93 +58:10:50.3 -- not an asteroid (will add it to exclusion list)
02:00:32.96 +59:40:06.3 -- not an asteroid (will add it to exclusion list)
01:06:55.45 +59:18:57.9 -- not an asteroid (will add it to exclusion list)
01:34:07.14 +60:12:53.3 -- not an asteroid (will add it to exclusion list)
01:54:40.24 +58:57:06.0 -- not an asteroid (will add it to exclusion list)
01:26:28.47 +59:41:36.1 -- not an asteroid (will add it to exclusion list)
01:26:03.85 +62:05:29.2 -- not an asteroid (will add it to exclusion list)
01:51:53.69 +63:26:21.8 -- not an asteroid (will add it to exclusion list)
02:02:25.92 +64:38:23.1 -- not an asteroid (will add it to exclusion list)
01:24:36.17 +61:08:55.0 -- not an asteroid (will add it to exclusion list)
01:23:42.21 +61:03:02.2 -- not an asteroid (will add it to exclusion list)
02:00:34.64 +59:38:08.0 -- not an asteroid (will add it to exclusion list)
02:13:47.59 +63:11:26.4 -- not an asteroid (will add it to exclusion list)
01:33:44.53 +60:46:17.5 -- not an asteroid (will add it to exclusion list)
02:21:53.12 +64:19:49.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:05:53.87 +59:06:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:13.14 +59:33:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:25.63 +61:41:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:55.45 +59:18:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:02.02 +59:46:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.19 +59:59:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.64 +57:26:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:12.08 +59:17:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:56.84 +58:41:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:10.20 +58:47:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:59.90 +57:34:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:38.93 +58:10:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:44.77 +57:24:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:19.75 +57:44:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:15.42 +58:35:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:45.13 +57:55:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:33.36 +60:44:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:51.69 +57:50:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:42.21 +61:03:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:36.17 +61:08:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:55.15 +59:41:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:27.74 +59:27:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:03.85 +62:05:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.70 +59:01:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:28.47 +59:41:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:36.82 +59:41:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:37.85 +64:03:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:07.45 +59:53:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:26.88 +60:23:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:04.41 +58:45:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:44.53 +60:46:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:07.14 +60:12:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:27.72 +60:33:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:05.86 +61:04:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:40.25 +61:00:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:29.99 +65:09:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:53.69 +63:26:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:40.24 +58:57:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:46.74 +57:57:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.02 +59:15:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:21.68 +64:56:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:32.96 +59:40:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:34.64 +59:38:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:25.92 +64:38:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:47.59 +63:11:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:47.67 +58:44:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:53.12 +64:19:49.8 -- 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)
01:05:53.87 +59:06:25.8 -- not a known variable star
01:06:13.14 +59:33:46.6 -- not a known variable star
01:06:25.63 +61:41:31.8 -- not a known variable star
01:06:55.45 +59:18:57.9 -- not a known variable star
01:07:02.02 +59:46:18.0 -- not a known variable star
01:07:39.19 +59:59:18.0 -- not a known variable star
01:09:22.64 +57:26:31.8 -- not a known variable star
01:10:12.08 +59:17:24.2 -- not a known variable star
01:11:56.84 +58:41:03.8 -- not a known variable star
01:12:10.20 +58:47:40.8 -- not a known variable star
01:12:59.90 +57:34:09.7 -- not a known variable star
01:13:38.93 +58:10:50.3 -- not a known variable star
01:13:44.77 +57:24:51.5 -- not a known variable star
01:15:19.75 +57:44:09.9 -- not a known variable star
01:17:15.42 +58:35:37.7 -- not a known variable star
01:20:45.13 +57:55:09.4 -- not a known variable star
01:22:33.36 +60:44:42.3 -- not a known variable star
01:22:51.69 +57:50:37.1 -- a known variable star
01:23:42.21 +61:03:02.2 -- not a known variable star
01:24:36.17 +61:08:55.0 -- a known variable star
01:24:55.15 +59:41:45.9 -- not a known variable star
01:25:27.74 +59:27:15.4 -- a known variable star
01:26:03.85 +62:05:29.2 -- not a known variable star
01:26:05.70 +59:01:14.1 -- not a known variable star
01:26:28.47 +59:41:36.1 -- not a known variable star
01:26:36.82 +59:41:35.3 -- a known variable star
01:27:37.85 +64:03:27.1 -- not a known variable star
01:28:07.45 +59:53:50.6 -- not a known variable star
01:28:26.88 +60:23:26.6 -- not a known variable star
01:29:04.41 +58:45:57.7 -- not a known variable star
01:33:44.53 +60:46:17.5 -- not a known variable star
01:34:07.14 +60:12:53.3 -- not a known variable star
01:35:27.72 +60:33:48.0 -- not a known variable star
01:38:05.86 +61:04:13.3 -- not a known variable star
01:43:40.25 +61:00:05.1 -- not a known variable star
01:44:29.99 +65:09:23.9 -- a known variable star
01:51:53.69 +63:26:21.8 -- a known variable star
01:54:40.24 +58:57:06.0 -- not a known variable star
01:55:46.74 +57:57:42.4 -- a known variable star
01:56:38.02 +59:15:33.7 -- a known variable star
02:00:21.68 +64:56:36.5 -- not a known variable star
02:00:32.96 +59:40:06.3 -- a known variable star
02:00:34.64 +59:38:08.0 -- not a known variable star
02:02:25.92 +64:38:23.1 -- a known variable star
02:13:47.59 +63:11:26.4 -- a known variable star
02:13:47.67 +58:44:00.9 -- not a known variable star
02:21:53.12 +64:19:49.8 -- a known variable star
Found 35 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
47 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 47 (excluding asteroids and hot pixels, 35 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461209.80291618 -observatory V36
07:31:24.28 +22:20:30.8 Mercury (0.7mag)
08:32:34.85 +20:54:13.0 Venus (-4.0mag)
03:19:07.08 +17:51:07.2 Mars (1.3mag)
07:57:02.12 +21:09:00.8 Jupiter (-1.8mag)
00:52:00.47 +03:02:40.7 Saturn (0.8mag)
04:02:34.07 +20:32:10.9 Uranus (5.8mag)
00:16:38.34 +00:19:27.5 Neptune (7.8mag)
20:32:43.33 -23:08:31.3 Pluto (14.5mag)
08:54:30.14 +18:23:25.4 Moon (-9.2mag)
-rw-r--r-- 1 apache apache 361 Jun 18 02:40 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461209.80291618:
07:56:56.98 +21:09:17.2 Io (6.2mag)
07:56:54.15 +21:09:27.9 Europa (6.3mag)
07:57:16.46 +21:08:18.2 Ganymede (5.6mag)
07:57:04.61 +21:08:59.5 Callisto (6.9mag)
07:56:43.55 +20:46:34.2 Himalia (15.6mag)
07:57:06.80 +21:08:45.5 Thebe (16.5mag)
07:56:26.41 +20:57:47.8 Elara (17.6mag)
07:59:42.58 +21:15:10.9 Pasiphae (17.8mag)
08:03:09.37 +21:11:33.4 Carme (18.9mag)
00:52:03.89 +03:03:06.8 Titan (8.6mag)
00:51:57.25 +03:02:37.5 Rhea (9.9mag)
00:52:18.96 +03:05:10.3 Iapetus (11.3mag)
00:52:11.73 +03:02:56.3 Hyperion (14.6mag)
00:52:30.09 +03:03:09.1 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 18 02:41 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461209.80291618:
17:28:16.97 -35:36:33.6 JWST
22:16:34.24 -43:10:09.4 Chandra
20:39:29.37 +36:11:46.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 18 02:40 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461209.80291618 -observatory V36
18:35:57.50 -33:20:33.8 13.6mag P/2010 H2 (Vales)
06:03:30.80 -67:59:53.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:52:48.12 +32:06:19.3 17.5mag C/2017 K2 (PANSTARRS)
17:10:43.10 +15:46:00.5 17.8mag C/2021 G2 (ATLAS)
22:52:26.26 -39:32:45.8 16.0mag P/2021 N1 (ZTF)
23:09:49.34 +31:56:14.7 17.2mag C/2022 E2 (ATLAS)
05:46:22.16 +27:00:39.5 16.5mag C/2022 N2 (PANSTARRS)
09:37:17.60 +30:42:32.1 16.7mag C/2022 QE78 (ATLAS)
08:56:11.14 +04:22:04.0 17.7mag C/2022 R6 (PANSTARRS)
18:21:32.16 +21:42:18.2 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:16:03.46 -11:03:16.9 17.6mag P/2023 B1 (PANSTARRS)
22:09:38.08 +67:05:09.8 17.8mag C/2023 H5 (Lemmon)
17:21:13.44 -07:43:14.4 13.7mag C/2023 R1 (PANSTARRS)
13:17:03.43 +80:37:49.8 18.0mag C/2023 X2 (Lemmon)
07:25:01.49 +64:40:48.0 17.8mag C/2024 A1 (ATLAS)
07:02:18.08 +28:39:24.9 14.0mag C/2024 E1 (Wierzchos)
15:29:41.84 +14:18:29.3 17.4mag C/2024 G6 (ATLAS)
20:05:16.61 +34:03:23.8 13.9mag C/2024 J3 (ATLAS)
04:28:08.37 -15:07:43.1 15.9mag C/2024 T5 (ATLAS)
06:15:15.31 +32:45:26.2 17.9mag C/2025 J1 (Borisov)
11:32:09.43 +52:08:04.5 17.8mag C/2025 L1 (ATLAS)
06:56:00.49 -11:21:38.8 15.0mag C/2025 R3 (PANSTARRS)
09:33:00.91 +23:09:30.4 17.9mag C/2025 V2 (Rankin)
12:40:00.69 +04:35:29.0 17.1mag C/2025 Y1 (ATLAS)
17:53:13.86 +77:03:43.8 17.7mag C/2026 A2 (Bok)
02:17:17.11 +44:05:10.9 16.3mag C/2026 B2 (Sun-Gao)
11:14:14.30 -00:30:27.9 16.6mag A/2026 E1
20:41:47.31 -09:38:35.2 8.2mag 10P/Tempel
11:04:46.95 -01:09:29.8 16.0mag 29P/Schwassmann-Wachmann
03:27:16.99 +26:57:37.6 17.7mag 47P/Ashbrook-Jackson
09:21:31.77 +20:49:11.8 16.9mag 63P/Wild
00:35:04.19 -05:47:22.9 15.6mag 65P/Gunn
07:16:18.15 +34:11:58.1 17.2mag 76P/West-Kohoutek-Ikemura
03:33:42.94 +18:24:10.1 13.8mag 78P/Gehrels
01:41:57.39 +06:55:49.9 15.8mag 88P/Howell
05:27:05.76 +30:50:36.3 15.4mag 93P/Lovas
03:12:16.97 +29:06:39.1 17.4mag 114P/Wiseman-Skiff
07:14:51.95 +32:33:34.6 15.5mag 123P/West-Hartley
10:07:58.35 +10:20:15.5 16.6mag 124P/Mrkos
04:15:43.17 +19:52:15.2 16.3mag 128P/Shoemaker-Holt
04:53:35.57 +19:27:56.7 17.8mag 131P/Mueller
06:39:34.15 +17:16:20.6 15.9mag 141P/Machholz
06:42:56.99 +17:53:52.1 15.9mag 141P-A/Machholz
05:43:23.99 +17:10:38.1 12.7mag 141P-D/Machholz
03:04:34.01 -23:22:53.5 16.4mag 161P/Hartley-IRAS
04:15:24.95 +27:37:10.1 15.0mag 162P/SidingSpring
19:33:44.04 +04:59:01.1 16.3mag 169P/NEAT
00:45:16.92 +04:21:08.3 17.8mag 220P/McNaught
16:44:59.72 -08:07:57.8 16.6mag 235P/LINEAR
07:57:21.57 +34:58:49.0 17.7mag 240P/NEAT
00:59:06.02 +01:56:09.6 16.1mag 260P/McNaught
04:32:18.23 +34:11:21.4 17.5mag 295P/LINEAR
00:46:31.22 +01:28:16.9 17.9mag 320P/McNaught
15:11:11.21 +07:39:08.1 17.5mag 391P/Kowalski
08:15:24.15 +20:27:43.4 17.9mag 450P/LONEOS
07:16:26.32 +40:57:30.6 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 18 02:41 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.18 +22:02:03.40 AT2026lxf 2026-05-8.07 13.94
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:49:13.39 +25:17:59.20 2026-06-15.39 15.93
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
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:49:13.39 +25:17:59.20 2026-06-15.39 15.93
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
19:32:43.68 -22:39:32.70 ASASSN-26cm 2026-04-4.27 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -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
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
-rw-r--r-- 1 apache apache 5.6K Jun 18 02:40 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
-rw-r--r-- 1 apache apache 189K Jun 18 02:40 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
23:09:28.921 -58:33:19.54 AT 2026oub 2026-06-06.75 18.88
00:22:14.997 -31:56:25.40 AT 2026oua 2026-06-06.79 19.42
00:27:47.533 -44:12:30.97 AT 2026otz 2026-06-06.80 19.35
01:16:28.303 -11:27:59.19 AT 2026oty 2026-06-06.79 19.15
13:38:30.343 -11:00:54.54 AT 2026otx 2026-04-16.52 20.06
13:27:19.671 -08:35:13.35 AT 2026otw 2026-06-07.40 20.36
12:24:14.411 -03:42:46.79 AT 2026otv 2026-06-07.40 20.17
11:40:32.768 -07:18:55.82 AT 2026otu 2026-06-07.37 20.18
12:27:47.187 +13:03:22.54 AT 2026ott 2026-05-19.03 20.15
12:22:38.942 +08:51:07.24 AT 2026ots 2026-05-19.02 20.44
09:46:20.889 +09:01:23.97 AT 2026otr 2026-05-18.96 20.1
22:34:44.197 +27:06:25.62 AT 2026otq 2026-06-09.56 18.841
00:15:02.869 -38:28:54.72 AT 2026otp 2026-05-22.42 20.11
23:31:16.630 -35:03:18.75 AT 2026oto 2026-05-04.41 19.11
12:25:14.599 +12:58:16.51 AT 2026otn 2026-05-19.03 20.12
10:04:42.371 +12:40:27.29 AT 2026otm 2026-05-04.99 20.5
18:56:24.084 -24:59:43.12 AT 2026otl 2026-06-07.38 18.4151
14:25:58.906 -19:09:39.58 AT 2026otk 2026-06-09.32 19.3712
16:32:34.784 -13:42:09.08 AT 2026otj 2026-05-22.23 22.76
01:51:40.895 +18:21:06.04 AT 2026oti 2026-06-06.48 18.6484
-rw-r--r-- 1 apache apache 30K Jun 18 02:40 tns_transients_list.txt
