This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8
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 09.3278 2461200.8278 11.39 01:33:43.47 +59:31:30.8
128.27767 -2.90691 galactic Cas Second-epoch detections are separated by 1.5" and 4.0 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 J023.4238+59.5237 | 01:33:43.47 +59:31:30.8 (user input) | dubious (ATLAS) | (ATLAS) | (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 01:33:43.47 +59:31:30.8: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:43.47 +59:31:30.8: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.23 +/- 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 09.3278* 01 33 43.47 +59 31 30.8 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
ATO J023.4238+59.5237,2461200.8278,11.39,0.05,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 J023.4238+59.5237 20260609.3278 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 11.21 01:23:12.04 +57:57:40.4
127.14860 -4.65024 galactic Cas Second-epoch detections are separated by 1.9" and 4.4 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 | 01:23:12.04 +57:57:40.4 (user input) | T | P | (position from user input) J-Ks=0.491+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:12.04 +57:57:40.4: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:12.04 +57:57:40.4: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 09.3278* 01 23 12.04 +57 57 40.4 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,2461200.8278,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260609.3278 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 11.11 01:51:52.54 +64:18:35.3
129.42495 2.20264 galactic Cas Second-epoch detections are separated by 2.1" and 4.3 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 | 01:51:52.54 +64:18:35.3 (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 01:51:52.54 +64:18:35.3: 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 01:51:52.54 +64:18:35.3: 13.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.90 +/- 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 09.3278* 01 51 52.54 +64 18 35.3 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,2461200.8278,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260609.3278 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 11.04 01:44:26.93 +60:39:07.6
129.38547 -1.55369 galactic Cas Second-epoch detections are separated by 0.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:44:26.93 +60:39:07.6 (user input) | T | P | (position from user input) J-Ks=0.275+/-0.041 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:26.93 +60:39:07.6: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:26.93 +60:39:07.6: 13.76 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 09.3278* 01 44 26.93 +60 39 07.6 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,2461200.8278,11.04,0.05,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
target 20260609.3278 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 09.3278 2461200.8278 10.89 01:54:45.45 +57:45:51.0
131.31969 -4.07272 galactic Per Second-epoch detections are separated by 1.4" and 4.6 pix
The object was found in VSX22" Gaia DR3 506102938826140544
Type: ROT
# Max. Min./Amp. JD0 Period
13.250 G 13.270 G 11.769600000000 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 01:54:45.45 +57:45:51.0: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:45.45 +57:45:51.0: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 09.3278* 01 54 45.45 +57 45 51.0 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
Gaia DR3 506102938826140544,2461200.8278,10.89,0.05,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 506102938826140544 20260609.3278 10.89CV 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 09.3278 2461200.8278 11.04 01:10:43.80 +60:59:18.3
125.27005 -1.79572 galactic Cas Second-epoch detections are separated by 1.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:10:43.80 +60:59:18.3 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:43.80 +60:59:18.3: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:43.80 +60:59:18.3: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 09.3278* 01 10 43.80 +60 59 18.3 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,2461200.8278,11.04,0.05,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
target 20260609.3278 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 09.3278 2461200.8278 11.09 01:40:18.24 +61:21:04.6
128.75556 -0.96672 galactic Cas Second-epoch detections are separated by 2.0" and 4.4 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 | 01:40:18.24 +61:21:04.6 (user input) | T | P | (position from user input) J-Ks=0.970+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:18.24 +61:21:04.6: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:18.24 +61:21:04.6: 13.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 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 09.3278* 01 40 18.24 +61 21 04.6 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,2461200.8278,11.09,0.05,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 20260609.3278 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 09.3278 2461200.8278 10.96 01:32:23.25 +61:29:12.8
127.79947 -0.99725 galactic Cas Second-epoch detections are separated by 1.7" and 4.5 pix
The object was found in VSX10" Gaia DR3 510746485668934272
Type: ROT
# Max. Min./Amp. JD0 Period
15.470 G 15.520 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 01:32:23.25 +61:29:12.8: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:23.25 +61:29:12.8: 13.75 +/- 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 09.3278* 01 32 23.25 +61 29 12.8 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
Gaia DR3 510746485668934272,2461200.8278,10.96,0.05,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
Gaia DR3 510746485668934272 20260609.3278 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 09.3278 2461200.8278 10.90 02:00:06.48 +59:00:31.6
131.68352 -2.69120 galactic Cas Second-epoch detections are separated by 0.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 507781618204489856 | 02:00:05.90 +59:00:52.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.381+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:06.48 +59:00:31.6: 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 02:00:06.48 +59:00:31.6: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 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 09.3278* 02 00 06.48 +59 00 31.6 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 507781618204489856,2461200.8278,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507781618204489856 20260609.3278 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.95 01:07:45.96 +57:45:03.5
125.11726 -5.05148 galactic Cas Second-epoch detections are separated by 5.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:45.96 +57:45:03.5 (user input) | T | P | (position from user input) SpType: A9V (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:45.96 +57:45:03.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:45.96 +57:45:03.5: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 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 09.3278* 01 07 45.96 +57 45 03.5 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,2461200.8278,10.95,0.05,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
target 20260609.3278 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 09.3278 2461200.8278 10.96 01:06:12.97 +59:33:47.6
124.80559 -3.25475 galactic Cas Second-epoch detections are separated by 6.5" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx2429469 | 01:06:12.97 +59:33:47.6 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (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 01:06:12.97 +59:33:47.6: 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 01:06:12.97 +59:33:47.6: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 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 09.3278* 01 06 12.97 +59 33 47.6 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
DocumentRef: VOTx2429469,2461200.8278,10.96,0.05,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
DocumentRef: VOTx2429469 20260609.3278 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 09.3278 2461200.8278 10.96 01:07:39.11 +59:59:18.1
124.96056 -2.81951 galactic Cas Second-epoch detections are separated by 1.6" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:07:39.11 +59:59:18.1 (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 01:07:39.11 +59:59:18.1: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.11 +59:59:18.1: 13.75 +/- 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 09.3278* 01 07 39.11 +59 59 18.1 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
target,2461200.8278,10.96,0.05,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
target 20260609.3278 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 09.3278 2461200.8278 10.83 01:17:00.42 +61:01:57.8
126.02418 -1.68542 galactic Cas Second-epoch detections are separated by 1.1" and 4.0 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 510529057246112384 | 01:17:01.47 +61:02:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.436+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:00.42 +61:01:57.8: 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 01:17:00.42 +61:01:57.8: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 09.3278* 01 17 00.42 +61 01 57.8 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
Gaia DR3 510529057246112384,2461200.8278,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510529057246112384 20260609.3278 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.86 01:43:27.28 +58:38:06.4
129.67092 -3.55438 galactic Cas Second-epoch detections are separated by 1.8" and 4.6 pix
The object was found in VSX 1" Gaia DR3 506084487648397824
Type: ROT
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:27.28 +58:38:06.4: 12.72 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.28 +58:38:06.4: 13.69 +/- 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 09.3278* 01 43 27.28 +58 38 06.4 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 506084487648397824,2461200.8278,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506084487648397824 20260609.3278 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.76 02:07:25.47 +57:54:58.3
132.90688 -3.47639 galactic Per Second-epoch detections are separated by 1.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J031.8527+57.9080 | 02:07:25.47 +57:54:58.3 (user input) | dubious (ATLAS) | (ATLAS) | (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 02:07:25.47 +57:54:58.3: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:25.47 +57:54:58.3: 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 09.3278* 02 07 25.47 +57 54 58.3 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J031.8527+57.9080,2461200.8278,10.76,0.05,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 J031.8527+57.9080 20260609.3278 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 09.3278 2461200.8278 10.91 01:08:59.53 +60:47:22.1
125.07335 -2.00927 galactic Cas Second-epoch detections are separated by 2.3" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 522440066710315904 | 01:08:58.80 +60:47:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.504+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:59.53 +60:47:22.1: 13.09 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:59.53 +60:47:22.1: 13.71 +/- 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 09.3278* 01 08 59.53 +60 47 22.1 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 522440066710315904,2461200.8278,10.91,0.05,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
Gaia DR3 522440066710315904 20260609.3278 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 09.3278 2461200.8278 10.79 01:25:45.82 +59:01:23.1
127.34507 -3.55423 galactic Cas Second-epoch detections are separated by 3.9" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx2486955 | 01:25:45.82 +59:01:23.1 (user input) | (GCVS) | (GCVS) | (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 01:25:45.82 +59:01:23.1: 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 01:25:45.82 +59:01:23.1: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 09.3278* 01 25 45.82 +59 01 23.1 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: VOTx2486955,2461200.8278,10.79,0.05,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
DocumentRef: VOTx2486955 20260609.3278 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 09.3278 2461200.8278 10.87 01:35:27.46 +60:33:46.8
128.31800 -1.84759 galactic Cas Second-epoch detections are separated by 1.8" and 4.0 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 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 01:35:27.46 +60:33:46.8: 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 01:35:27.46 +60:33:46.8: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 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 09.3278* 01 35 27.46 +60 33 46.8 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
Gaia DR3 509811625915787136,2461200.8278,10.87,0.05,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 20260609.3278 10.87CV 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 09.3278 2461200.8278 10.63 01:17:15.32 +57:23:49.5
126.41931 -5.29975 galactic Cas Second-epoch detections are separated by 4.1" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:17:15.32 +57:23:49.5 (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 01:17:15.32 +57:23:49.5: 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 01:17:15.32 +57:23:49.5: 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 09.3278* 01 17 15.32 +57 23 49.5 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,2461200.8278,10.63,0.05,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 20260609.3278 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 09.3278 2461200.8278 10.66 01:49:15.78 +59:14:38.4
130.27526 -2.80081 galactic Cas Second-epoch detections are separated by 1.5" and 4.2 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 506536352570768768 | 01:49:14.31 +59:14:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:15.78 +59:14:38.4: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:15.78 +59:14:38.4: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 09.3278* 01 49 15.78 +59 14 38.4 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 506536352570768768,2461200.8278,10.66,0.05,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 506536352570768768 20260609.3278 10.66CV 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 09.3278 2461200.8278 10.54 01:31:23.18 +59:33:42.9
127.97893 -2.91780 galactic Cas Second-epoch detections are separated by 0.6" and 4.2 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 | DocumentRef: VOTx2753666 | 01:31:23.18 +59:33:42.9 (user input) | (GCVS) | (GCVS) | (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 01:31:23.18 +59:33:42.9: 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 01:31:23.18 +59:33:42.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 09.3278* 01 31 23.18 +59 33 42.9 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
DocumentRef: VOTx2753666,2461200.8278,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2753666 20260609.3278 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.51 01:19:08.61 +60:33:58.8
126.33170 -2.12240 galactic Cas Second-epoch detections are separated by 0.6" and 4.2 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 510378080556092032 | 01:19:06.00 +60:34:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:08.61 +60:33:58.8: 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 01:19:08.61 +60:33:58.8: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 09.3278* 01 19 08.61 +60 33 58.8 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 510378080556092032,2461200.8278,10.51,0.05,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
Gaia DR3 510378080556092032 20260609.3278 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 09.3278 2461200.8278 10.28 01:04:09.16 +63:14:40.9
124.36235 0.40827 galactic Cas Second-epoch detections are separated by 5.7" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:04:09.16 +63:14:40.9 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:04:09.16 +63:14:40.9: 11.34 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:09.16 +63:14:40.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 09.3278* 01 04 09.16 +63 14 40.9 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461200.8278,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260609.3278 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.43 01:15:19.62 +57:44:09.2
126.12803 -4.98754 galactic Cas Second-epoch detections are separated by 2.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J018.8211+57.7311 | 01:15:19.62 +57:44:09.2 (user input) | dubious (ATLAS) | (ATLAS) | (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 01:15:19.62 +57:44:09.2: 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 01:15:19.62 +57:44:09.2: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 09.3278* 01 15 19.62 +57 44 09.2 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+57.7311,2461200.8278,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.8211+57.7311 20260609.3278 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.38 02:04:11.04 +57:54:37.8
132.49513 -3.60419 galactic Per Second-epoch detections are separated by 1.5" and 4.2 pix
The object was found in VSX 3" Gaia DR3 505424574514826112
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.890 G 13.920 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:04:11.04 +57:54:37.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:04:11.04 +57:54:37.8: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 09.3278* 02 04 11.04 +57 54 37.8 10.4 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
Gaia DR3 505424574514826112,2461200.8278,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505424574514826112 20260609.3278 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.26 02:00:26.45 +63:04:26.4
130.65137 1.24109 galactic Cas Second-epoch detections are separated by 0.5" and 4.2 pix
The object was found in VSX15" Gaia DR3 508892228030391552
Type: E
# Max. Min./Amp. JD0 Period
13.120 G 13.390 G 3.454060000000 A
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 02:00:26.45 +63:04:26.4: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:26.45 +63:04:26.4: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 09.3278* 02 00 26.45 +63 04 26.4 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 508892228030391552,2461200.8278,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508892228030391552 20260609.3278 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 9.97 01:46:55.17 +59:54:51.7
129.83920 -2.21124 galactic Cas Second-epoch detections are separated by 0.5" and 4.2 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 506617853860840320 | 01:46:52.59 +59:54:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1955ApJS....2..123F LF 5 +59 210 J-Ks=0.866+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:55.17 +59:54:51.7: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:55.17 +59:54:51.7: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 09.3278* 01 46 55.17 +59 54 51.7 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506617853860840320,2461200.8278,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506617853860840320 20260609.3278 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 8.21 01:47:13.05 +57:44:18.9
130.34393 -4.32822 galactic Cas Second-epoch detections are separated by 1.6" and 4.4 pix
The object was found in VSX 4" Gaia DR3 505962471920178944
Type: VAR
# Max. Min./Amp. JD0 Period
13.440 G 13.470 G 0.024984900000 A
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 01:47:13.05 +57:44:18.9: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:13.05 +57:44:18.9: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.71 +/- 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 09.3278* 01 47 13.05 +57 44 18.9 8.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505962471920178944,2461200.8278,8.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505962471920178944 20260609.3278 8.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.60 01:46:38.60 +60:07:32.7
129.76041 -2.01205 galactic Cas Second-epoch detections are separated by 0.7" and 4.3 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 J026.6591+60.1406 | 01:46:39.63 +60:07:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.60 +60:07:32.7: 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 01:46:38.60 +60:07:32.7: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 09.3278* 01 46 38.60 +60 07 32.7 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
ATO J026.6591+60.1406,2461200.8278,10.60,0.05,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
ATO J026.6591+60.1406 20260609.3278 10.60CV 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 09.3278 2461200.8278 10.64 01:51:09.39 +64:52:46.4
129.21818 2.73920 galactic Cas Second-epoch detections are separated by 1.8" and 4.0 pix
The object was found in VSX 3" Gaia DR3 518229967963921664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:09.39 +64:52:46.4: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:09.39 +64:52:46.4: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 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 09.3278* 01 51 09.39 +64 52 46.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 518229967963921664,2461200.8278,10.64,0.05,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 518229967963921664 20260609.3278 10.64CV 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 09.3278 2461200.8278 10.62 01:15:26.33 +58:04:29.8
126.11118 -4.64857 galactic Cas Second-epoch detections are separated by 1.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413485851742499200 | 01:15:28.49 +58:04:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.692+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:26.33 +58:04:29.8: 11.48 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:26.33 +58:04:29.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 09.3278* 01 15 26.33 +58 04 29.8 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
Gaia DR3 413485851742499200,2461200.8278,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413485851742499200 20260609.3278 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.59 02:02:42.34 +60:04:29.1
131.71536 -1.57602 galactic Cas Second-epoch detections are separated by 0.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 507936511903779840 | 02:02:37.17 +60:04:47.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.223+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:42.34 +60:04:29.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:42.34 +60:04:29.1: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 09.3278* 02 02 42.34 +60 04 29.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507936511903779840,2461200.8278,10.59,0.05,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 507936511903779840 20260609.3278 10.59CV 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 09.3278 2461200.8278 10.69 01:22:11.05 +59:09:01.5
126.87206 -3.48591 galactic Cas Second-epoch detections are separated by 1.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 413976852405588480 | 01:22:13.31 +59:08:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1960IzKry..24..160B [B60] +58 184
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:11.05 +59:09:01.5: 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 01:22:11.05 +59:09:01.5: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 09.3278* 01 22 11.05 +59 09 01.5 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
Gaia DR3 413976852405588480,2461200.8278,10.69,0.05,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
Gaia DR3 413976852405588480 20260609.3278 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 09.3278 2461200.8278 10.80 02:02:23.86 +59:42:16.1
131.77889 -1.94286 galactic Cas Second-epoch detections are separated by 2.7" and 4.0 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 J030.6164+59.6920 | 02:02:24.46 +59:41:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.461+/-0.026 (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 02:02:23.86 +59:42:16.1: 13.14 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:23.86 +59:42:16.1: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 09.3278* 02 02 23.86 +59 42 16.1 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 J030.6164+59.6920,2461200.8278,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J030.6164+59.6920 20260609.3278 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.69 02:18:27.81 +59:22:12.8
133.82202 -1.64896 galactic Cas Second-epoch detections are separated by 1.3" and 4.3 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 | DocumentRef: VOTx2686213 | 02:18:22.83 +59:22:33.4 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE SpType: A0 1956ApJ...123..258S Cl* Stock 2 S 134
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:27.81 +59:22:12.8: 11.83 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:27.81 +59:22:12.8: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 09.3278* 02 18 27.81 +59 22 12.8 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
DocumentRef: VOTx2686213,2461200.8278,10.69,0.05,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
DocumentRef: VOTx2686213 20260609.3278 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 09.3278 2461200.8278 10.79 01:44:03.17 +61:54:44.9
129.08260 -0.32933 galactic Cas Second-epoch detections are separated by 1.2" and 4.2 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 511486800591720192 | 01:44:01.89 +61:55:16.8 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B1V 1999A&AS..136..313S Cl* NGC 654 Sto 94
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:03.17 +61:54:44.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:03.17 +61:54:44.9: 13.95 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.12
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 09.3278* 01 44 03.17 +61 54 44.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511486800591720192,2461200.8278,10.79,0.05,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
Gaia DR3 511486800591720192 20260609.3278 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 09.3278 2461200.8278 10.87 02:04:00.80 +58:29:05.8
132.31357 -3.05863 galactic Per Second-epoch detections are separated by 0.6" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J031.0030+58.4847 | 02:04:00.80 +58:29:05.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.288+/-0.029 (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 02:04:00.80 +58:29:05.8: 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 02:04:00.80 +58:29:05.8: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 09.3278* 02 04 00.80 +58 29 05.8 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
ATO J031.0030+58.4847,2461200.8278,10.87,0.05,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 J031.0030+58.4847 20260609.3278 10.87CV 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 09.3278 2461200.8278 10.79 02:10:48.74 +58:01:14.3
133.30563 -3.24348 galactic Per Second-epoch detections are separated by 2.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 506708082540660480 | 02:10:51.97 +58:00:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:48.74 +58:01:14.3: 12.88 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:48.74 +58:01:14.3: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 09.3278* 02 10 48.74 +58 01 14.3 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506708082540660480,2461200.8278,10.79,0.05,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
Gaia DR3 506708082540660480 20260609.3278 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 09.3278 2461200.8278 10.93 02:00:32.91 +59:40:07.8
131.56351 -2.03971 galactic Cas Second-epoch detections are separated by 0.7" and 4.5 pix
The object was found in VSX 2" 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 02:00:32.91 +59:40:07.8: 11.50 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.91 +59:40:07.8: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.83 +/- 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 09.3278* 02 00 32.91 +59 40 07.8 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
ZTF J020033.07+594008.7,2461200.8278,10.93,0.05,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
ZTF J020033.07+594008.7 20260609.3278 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 09.3278 2461200.8278 10.90 01:06:55.35 +59:18:56.7
124.90996 -3.49651 galactic Cas Second-epoch detections are separated by 3.7" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:55.35 +59:18:56.7 (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 01:06:55.35 +59:18:56.7: 13.08 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.35 +59:18:56.7: 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 09.3278* 01 06 55.35 +59 18 56.7 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,2461200.8278,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260609.3278 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 11.03 01:15:35.34 +58:55:23.2
126.05118 -3.80229 galactic Cas Second-epoch detections are separated by 1.8" and 4.6 pix
The object was found in VSX25" Gaia DR3 414098966911274496
Type: ROT
# Max. Min./Amp. JD0 Period
14.970 G 15.010 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:35.34 +58:55:23.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:35.34 +58:55:23.2: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 09.3278* 01 15 35.34 +58 55 23.2 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
Gaia DR3 414098966911274496,2461200.8278,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 414098966911274496 20260609.3278 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 11.19 02:11:59.67 +63:23:12.5
131.80933 1.91204 galactic Cas Second-epoch detections are separated by 3.7" and 4.2 pix
The object was found in VSX13" ZTF J021201.47+632309.0
Type: EW
# Max. Min./Amp. JD0 Period
19.319 r Y 0.453 r 2458289.97240 0.293789200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:59.67 +63:23:12.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:59.67 +63:23:12.5: 14.31 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.31 +/- 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 09.3278* 02 11 59.67 +63 23 12.5 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
ZTF J021201.47+632309.0,2461200.8278,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J021201.47+632309.0 20260609.3278 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 10.97 01:46:02.90 +58:23:58.1
130.05152 -3.71536 galactic Cas Second-epoch detections are separated by 2.7" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.5173+58.4014 | 01:45:58.55 +58:23:57.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 1932MeUpp..55....1S BD+57 384
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:02.90 +58:23:58.1: 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 01:46:02.90 +58:23:58.1: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 09.3278* 01 46 02.90 +58 23 58.1 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 J026.5173+58.4014,2461200.8278,10.97,0.05,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
ATO J026.5173+58.4014 20260609.3278 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 09.3278 2461200.8278 10.99 01:22:24.01 +61:13:52.0
126.64970 -1.41694 galactic Cas Second-epoch detections are separated by 1.9" and 4.2 pix
The object was found in VSX 2" NSVS J0122238+611352
Type: M
# Max. Min./Amp. JD0 Period
14.871 r Y 3.740 r 2458328.87710 325.120339600000
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 01:22:24.01 +61:13:52.0: 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 01:22:24.01 +61:13:52.0: 15.81 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.81 +/- 0.25
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 09.3278* 01 22 24.01 +61 13 52.0 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
NSVS J0122238+611352,2461200.8278,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0122238+611352 20260609.3278 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 11.07 01:50:39.94 +62:00:56.6
129.81927 -0.06143 galactic Cas Second-epoch detections are separated by 0.4" and 4.2 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 511356332360621440 | 01:50:34.89 +62:00:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1955ApJS....2..123F LF 5 +61 158 J-Ks=1.202+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:39.94 +62:00:56.6: 13.34 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.94 +62:00:56.6: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 09.3278* 01 50 39.94 +62 00 56.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511356332360621440,2461200.8278,11.07,0.05,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 511356332360621440 20260609.3278 11.07CV 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 09.3278 2461200.8278 11.21 01:24:11.90 +59:17:53.7
127.10996 -3.30748 galactic Cas Second-epoch detections are separated by 2.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510053346667812608 | 01:24:05.94 +59:18:02.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2 1960IzKry..24..160B [B60] +59 155
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:11.90 +59:17:53.7: 12.77 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:11.90 +59:17:53.7: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.05 +/- 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 09.3278* 01 24 11.90 +59 17 53.7 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
Gaia DR3 510053346667812608,2461200.8278,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510053346667812608 20260609.3278 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.3278 2461200.8278 11.43 01:31:19.96 +58:54:35.9
128.07302 -3.56297 galactic Cas Second-epoch detections are separated by 1.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 509244380989367296 | 01:31:18.47 +58:53:57.7 (Gaia DR3) | E (local) | A (local) | Gaia3var=VARIABLE SpType: A0 1960IzKry..24..160B [B60] +58 284 J-Ks=0.421+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:19.96 +58:54:35.9: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:19.96 +58:54:35.9: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 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 09.3278* 01 31 19.96 +58 54 35.9 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 509244380989367296,2461200.8278,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509244380989367296 20260609.3278 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461200.82803709 09.06.2026 07:52:12.405 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
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: 9 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): 25031
Objects passed selection criteria: 24889
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 17283.8
Average stars matched: 15974 (92.4221 %)
Memory usage VmPeak: 128292 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 9 04:49:16 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: 2461200.82803709 09.06.2026 07:52:12.405 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 208
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: 130 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): 183763
Objects passed selection criteria: 183294
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: 134610
Average stars matched: 124165 (92.2404 %)
Memory usage VmPeak: 1935416 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 9 04:56:56 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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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: 2461200.82755694
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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits'
wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
Image size: 938.9'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: 01:43:04.990 +61:58:48.65 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 01:43:04.990 +61:58:48.65
Angular distance between the image centers 0.0712 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
util/fov_of_wcs_calibrated_image.sh: line 168: echo: write error: Broken pipe
Image size: 938.9'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: 01:43:07.880 +61:59:02.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:07.880 +61:59:02.79
Angular distance between the image centers 0.0767 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 01:43:04.990 +61:58:48.65
Second-epoch second image center 01:43:07.880 +61:59:02.79
Angular distance between the image centers 0.00689 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.CzquTkxU5Z
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.nILY4GQxmb
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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits &> /tmp/tmp.YCssC3JPb2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits &> /tmp/tmp.jd7n1Cx2Er
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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 2 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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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
14.2 mag. fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
14.1 mag. fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.4 (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.CzquTkxU5Z (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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/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.nILY4GQxmb (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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/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
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/util/wcs_image_calibration.sh: line 136: echo: write error: Broken pipe
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.YCssC3JPb2 (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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1100, passed=14122
Got 14122 stars (including 13009 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 14122 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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: 973 matched stars entering correct_measured_positions(), 13819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 13819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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=fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits N_match=973 sigma_overall_arcsec=0.706 sigma_q1_arcsec=0.636 sigma_q2_arcsec=0.657 sigma_q3_arcsec=0.862 sigma_q4_arcsec=0.832 n_q1=270 n_q2=322 n_q3=223 n_q4=158 worst_quadrant_to_overall_ratio=1.220
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.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.jd7n1Cx2Er (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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1087, passed=14122
Got 14122 stars (including 13023 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat
util/solve_plate_with_UCAC5 got 14122 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
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(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 13814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 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(), 13812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 13812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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=fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits N_match=974 sigma_overall_arcsec=0.712 sigma_q1_arcsec=0.616 sigma_q2_arcsec=0.701 sigma_q3_arcsec=0.836 sigma_q4_arcsec=0.756 n_q1=272 n_q2=319 n_q3=231 n_q4=152 worst_quadrant_to_overall_ratio=1.175
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits sigma_overall=0.706 worst_q_ratio=1.220
new2=fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits sigma_overall=0.712 worst_q_ratio=1.175
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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162_astrometric_residuals.png (973 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.66 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163_astrometric_residuals.png (974 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.65 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52554_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 52554_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:19:46.46 +58:12:26.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 08339_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:20:32.63 +62:32:02.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
Image size: 938.9'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: 01:43:04.990 +61:58:48.65 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 01:43:04.990 +61:58:48.65
Angular distance between the image centers 0.0712 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
Image size: 938.9'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: 01:43:07.880 +61:59:02.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:07.880 +61:59:02.79
Angular distance between the image centers 0.0767 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 01:43:04.990 +61:58:48.65
Second-epoch second image center 01:43:07.880 +61:59:02.79
Angular distance between the image centers 0.00689 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.zaIPuCPwfB
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.9MfU53rxYA
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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits &> /tmp/tmp.3NwjAgMHUI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits &> /tmp/tmp.IxxJ5jAR3W
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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 173 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
2.2 pix fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
2.2 pix fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
11.7 mag. fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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.zaIPuCPwfB (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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/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.9MfU53rxYA (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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/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.3NwjAgMHUI (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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=10466, passed=107643
Got 107643 stars (including 97053 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 107643 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 975 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(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 105771 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 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 105768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 105769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 972 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits N_match=972 sigma_overall_arcsec=0.652 sigma_q1_arcsec=0.593 sigma_q2_arcsec=0.577 sigma_q3_arcsec=0.866 sigma_q4_arcsec=0.685 n_q1=256 n_q2=339 n_q3=194 n_q4=183 worst_quadrant_to_overall_ratio=1.328
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.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.IxxJ5jAR3W (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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=10173, passed=108893
Got 108893 stars (including 98599 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat
util/solve_plate_with_UCAC5 got 108893 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.3)
Done reading UCAC5 zone files...
Matched 975 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(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 106628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 106626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 106624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 972 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits N_match=972 sigma_overall_arcsec=0.676 sigma_q1_arcsec=0.622 sigma_q2_arcsec=0.633 sigma_q3_arcsec=0.782 sigma_q4_arcsec=0.718 n_q1=260 n_q2=333 n_q3=195 n_q4=184 worst_quadrant_to_overall_ratio=1.157
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits -region wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-51-30_20.00sec_5.00C_LIGHT_0162.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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_2026-06-09_CI_Cas-03-Q2b1x1_043810_TTUQ2b1x1_1649515_trO5NYY8/wcs_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163.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 01:32:23.25 +61:29:12.8: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:45.45 +57:45:51.0: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:26.93 +60:39:07.6: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:18.24 +61:21:04.6: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:43.47 +59:31:30.8: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:12.04 +57:57:40.4: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:52.54 +64:18:35.3: 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 01:10:43.80 +60:59:18.3: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:45.45 +57:45:51.0: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.05
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:23.25 +61:29:12.8: 13.75 +/- 0.04 detection
Forced photometry filter KEPT candidate at 01:54:45.45 +57:45:51.0: ref_mag=13.65 +/- 0.05 new_mean_mag=10.8120 delta=2.84 (need > 0.90)
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter KEPT candidate at 01:32:23.25 +61:29:12.8: ref_mag=13.75 +/- 0.04 new_mean_mag=10.9666 delta=2.78 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:18.24 +61:21:04.6: 13.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Forced photometry filter KEPT candidate at 01:40:18.24 +61:21:04.6: ref_mag=13.86 +/- 0.04 new_mean_mag=11.0849 delta=2.77 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:52.54 +64:18:35.3: 13.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Forced photometry filter KEPT candidate at 01:51:52.54 +64:18:35.3: ref_mag=13.90 +/- 0.04 new_mean_mag=11.1086 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 01:23:12.04 +57:57:40.4: 13.93 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:43.80 +60:59:18.3: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Forced photometry filter KEPT candidate at 01:23:12.04 +57:57:40.4: ref_mag=13.93 +/- 0.05 new_mean_mag=11.1627 delta=2.77 (need > 0.90)
Forced photometry filter KEPT candidate at 01:10:43.80 +60:59:18.3: ref_mag=13.67 +/- 0.04 new_mean_mag=11.0444 delta=2.62 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:26.93 +60:39:07.6: 13.76 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:43.47 +59:31:30.8: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.06
Forced photometry reference-image weighted average: 13.76 +/- 0.09
Forced photometry filter KEPT candidate at 01:33:43.47 +59:31:30.8: ref_mag=14.23 +/- 0.06 new_mean_mag=11.3963 delta=2.83 (need > 0.90)
Forced photometry filter KEPT candidate at 01:44:26.93 +60:39:07.6: ref_mag=13.76 +/- 0.09 new_mean_mag=11.0190 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:06.48 +59:00:31.6: 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 01:07:45.96 +57:45:03.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:06.48 +59:00:31.6: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter KEPT candidate at 02:00:06.48 +59:00:31.6: ref_mag=13.57 +/- 0.03 new_mean_mag=10.8759 delta=2.69 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:45.96 +57:45:03.5: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Forced photometry filter KEPT candidate at 01:07:45.96 +57:45:03.5: ref_mag=13.57 +/- 0.04 new_mean_mag=10.9414 delta=2.62 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:12.97 +59:33:47.6: 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 01:06:12.97 +59:33:47.6: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter KEPT candidate at 01:06:12.97 +59:33:47.6: ref_mag=13.51 +/- 0.03 new_mean_mag=10.9573 delta=2.55 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.11 +59:59:18.1: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.11 +59:59:18.1: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter KEPT candidate at 01:07:39.11 +59:59:18.1: ref_mag=13.75 +/- 0.04 new_mean_mag=10.9545 delta=2.79 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:00.42 +61:01:57.8: 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 01:17:00.42 +61:01:57.8: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter KEPT candidate at 01:17:00.42 +61:01:57.8: ref_mag=13.78 +/- 0.04 new_mean_mag=10.8225 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 01:43:27.28 +58:38:06.4: 12.72 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.28 +58:38:06.4: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter KEPT candidate at 01:43:27.28 +58:38:06.4: ref_mag=13.65 +/- 0.04 new_mean_mag=10.8538 delta=2.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:25.47 +57:54:58.3: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:25.47 +57:54:58.3: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Forced photometry filter KEPT candidate at 02:07:25.47 +57:54:58.3: ref_mag=13.47 +/- 0.04 new_mean_mag=10.7581 delta=2.71 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:59.53 +60:47:22.1: 13.09 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:59.53 +60:47:22.1: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.05
Forced photometry filter KEPT candidate at 01:08:59.53 +60:47:22.1: ref_mag=13.70 +/- 0.05 new_mean_mag=10.8511 delta=2.84 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:45.82 +59:01:23.1: 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 01:25:45.82 +59:01:23.1: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry filter KEPT candidate at 01:25:45.82 +59:01:23.1: ref_mag=13.59 +/- 0.04 new_mean_mag=10.7794 delta=2.81 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:27.46 +60:33:46.8: 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 01:35:27.46 +60:33:46.8: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Forced photometry filter KEPT candidate at 01:35:27.46 +60:33:46.8: ref_mag=13.61 +/- 0.04 new_mean_mag=10.8248 delta=2.78 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:10.46 +60:37:28.7: 7.46 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:10.46 +60:37:28.7: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 7.70 +/- 0.01
Forced photometry filter REJECTED candidate at 01:33:10.46 +60:37:28.7: ref_mag=7.70 +/- 0.01 new_mean_mag=10.5425 delta=-2.84 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:15.32 +57:23:49.5: 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 01:17:15.32 +57:23:49.5: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry filter KEPT candidate at 01:17:15.32 +57:23:49.5: ref_mag=13.60 +/- 0.04 new_mean_mag=10.6321 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 01:49:15.78 +59:14:38.4: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:15.78 +59:14:38.4: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter KEPT candidate at 01:49:15.78 +59:14:38.4: ref_mag=13.27 +/- 0.02 new_mean_mag=10.6568 delta=2.61 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:23.18 +59:33:42.9: 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 01:31:23.18 +59:33:42.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter KEPT candidate at 01:31:23.18 +59:33:42.9: ref_mag=13.30 +/- 0.03 new_mean_mag=10.5350 delta=2.76 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:08.61 +60:33:58.8: 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 01:19:08.61 +60:33:58.8: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry filter KEPT candidate at 01:19:08.61 +60:33:58.8: ref_mag=13.16 +/- 0.03 new_mean_mag=10.4946 delta=2.66 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:04:09.16 +63:14:40.9: 11.34 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:09.16 +63:14:40.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter KEPT candidate at 01:04:09.16 +63:14:40.9: ref_mag=12.81 +/- 0.02 new_mean_mag=10.2042 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 01:15:19.62 +57:44:09.2: 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 01:15:19.62 +57:44:09.2: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 01:15:19.62 +57:44:09.2: ref_mag=13.38 +/- 0.03 new_mean_mag=10.4281 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 02:04:11.04 +57:54:37.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:04:11.04 +57:54:37.8: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter KEPT candidate at 02:04:11.04 +57:54:37.8: ref_mag=13.12 +/- 0.03 new_mean_mag=10.3720 delta=2.75 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:26.45 +63:04:26.4: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:26.45 +63:04:26.4: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter KEPT candidate at 02:00:26.45 +63:04:26.4: ref_mag=12.90 +/- 0.02 new_mean_mag=10.2598 delta=2.64 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:55.17 +59:54:51.7: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:55.17 +59:54:51.7: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 01:46:55.17 +59:54:51.7: ref_mag=12.65 +/- 0.01 new_mean_mag=9.9757 delta=2.67 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:13.05 +57:44:18.9: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:13.05 +57:44:18.9: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.71 +/- 0.00
Forced photometry filter KEPT candidate at 01:47:13.05 +57:44:18.9: ref_mag=10.71 +/- 0.00 new_mean_mag=8.2035 delta=2.51 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.60 +60:07:32.7: 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 01:46:38.60 +60:07:32.7: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.04
Forced photometry filter KEPT candidate at 01:46:38.60 +60:07:32.7: ref_mag=13.42 +/- 0.04 new_mean_mag=10.5930 delta=2.83 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:09.39 +64:52:46.4: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:26.33 +58:04:29.8: 11.48 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:09.39 +64:52:46.4: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry filter KEPT candidate at 01:51:09.39 +64:52:46.4: ref_mag=13.53 +/- 0.04 new_mean_mag=10.6364 delta=2.89 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:26.33 +58:04:29.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter KEPT candidate at 01:15:26.33 +58:04:29.8: ref_mag=13.12 +/- 0.03 new_mean_mag=10.6129 delta=2.51 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:42.34 +60:04:29.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:42.34 +60:04:29.1: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 02:02:42.34 +60:04:29.1: ref_mag=13.42 +/- 0.03 new_mean_mag=10.5779 delta=2.84 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:11.05 +59:09:01.5: 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 01:22:11.05 +59:09:01.5: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.04
Forced photometry filter KEPT candidate at 01:22:11.05 +59:09:01.5: ref_mag=13.72 +/- 0.04 new_mean_mag=10.6872 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 02:02:23.86 +59:42:16.1: 13.14 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:23.86 +59:42:16.1: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.05
Forced photometry filter KEPT candidate at 02:02:23.86 +59:42:16.1: ref_mag=13.66 +/- 0.05 new_mean_mag=10.7874 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 02:18:27.81 +59:22:12.8: 11.83 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:27.81 +59:22:12.8: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Forced photometry filter KEPT candidate at 02:18:27.81 +59:22:12.8: ref_mag=13.11 +/- 0.03 new_mean_mag=10.6763 delta=2.43 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:49.04 +59:06:40.0: 10.00 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:49.04 +59:06:40.0: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.65 +/- 0.02
Forced photometry filter REJECTED candidate at 02:09:49.04 +59:06:40.0: ref_mag=10.65 +/- 0.02 new_mean_mag=10.7557 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:03.17 +61:54:44.9: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:03.17 +61:54:44.9: 13.95 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.12
Forced photometry filter KEPT candidate at 01:44:03.17 +61:54:44.9: ref_mag=13.95 +/- 0.12 new_mean_mag=10.7833 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 02:04:00.80 +58:29:05.8: 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 02:04:00.80 +58:29:05.8: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Forced photometry filter KEPT candidate at 02:04:00.80 +58:29:05.8: ref_mag=13.80 +/- 0.05 new_mean_mag=10.8606 delta=2.94 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:48.74 +58:01:14.3: 12.88 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:48.74 +58:01:14.3: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter KEPT candidate at 02:10:48.74 +58:01:14.3: ref_mag=13.69 +/- 0.04 new_mean_mag=10.7875 delta=2.90 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:32.91 +59:40:07.8: 11.50 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.91 +59:40:07.8: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.05
Forced photometry filter KEPT candidate at 02:00:32.91 +59:40:07.8: ref_mag=12.83 +/- 0.05 new_mean_mag=10.9256 delta=1.90 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:05.42 +57:15:18.8: 10.17 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:05.42 +57:15:18.8: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.02
Forced photometry filter REJECTED candidate at 01:09:05.42 +57:15:18.8: ref_mag=11.15 +/- 0.02 new_mean_mag=10.6840 delta=0.47 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.35 +59:18:56.7: 13.08 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.35 +59:18:56.7: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter KEPT candidate at 01:06:55.35 +59:18:56.7: ref_mag=13.82 +/- 0.05 new_mean_mag=10.9050 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:35.34 +58:55:23.2: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:35.34 +58:55:23.2: 14.06 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.06
Forced photometry filter KEPT candidate at 01:15:35.34 +58:55:23.2: ref_mag=14.06 +/- 0.06 new_mean_mag=11.0087 delta=3.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:59.67 +63:23:12.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:59.67 +63:23:12.5: 14.31 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.09
Forced photometry filter KEPT candidate at 02:11:59.67 +63:23:12.5: ref_mag=14.31 +/- 0.09 new_mean_mag=11.1561 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 01:46:02.90 +58:23:58.1: 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 01:46:02.90 +58:23:58.1: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.05
Forced photometry filter KEPT candidate at 01:46:02.90 +58:23:58.1: ref_mag=13.78 +/- 0.05 new_mean_mag=10.9530 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 01:22:24.01 +61:13:52.0: 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 01:22:24.01 +61:13:52.0: 15.81 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.81 +/- 0.25
Forced photometry filter KEPT candidate at 01:22:24.01 +61:13:52.0: ref_mag=15.81 +/- 0.25 new_mean_mag=10.9855 delta=4.83 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:36.25 +60:53:51.4: 9.78 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:36.25 +60:53:51.4: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 10.89 +/- 0.03
Forced photometry filter REJECTED candidate at 01:39:36.25 +60:53:51.4: ref_mag=10.89 +/- 0.03 new_mean_mag=11.0536 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:39.94 +62:00:56.6: 13.34 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.94 +62:00:56.6: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Forced photometry filter KEPT candidate at 01:50:39.94 +62:00:56.6: ref_mag=13.96 +/- 0.05 new_mean_mag=11.0589 delta=2.90 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:11.90 +59:17:53.7: 12.77 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:11.90 +59:17:53.7: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.06
Forced photometry filter KEPT candidate at 01:24:11.90 +59:17:53.7: ref_mag=14.05 +/- 0.06 new_mean_mag=11.2032 delta=2.85 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:19.96 +58:54:35.9: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:19.96 +58:54:35.9: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.06
Forced photometry filter KEPT candidate at 01:31:19.96 +58:54:35.9: ref_mag=14.07 +/- 0.06 new_mean_mag=11.4043 delta=2.67 (need > 0.90)
Adding exclusion_list_local.txt__out247627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out264938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270282.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 402s
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: 42s
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Considering the candidate 247627_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247627_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247628_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247628_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247652_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247652_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:09:22.22 +64:35:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247655_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247655_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247657_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247657_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247659_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247659_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247663_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247663_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247666_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247666_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247672_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247672_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:13:40.80 +60:51:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247675_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247675_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247676_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247676_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247677_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247677_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247681_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247681_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:33:35.28 +59:56:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247683_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247683_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247684_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247684_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:07:35.09 +57:33:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247687_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247687_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247692_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247692_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:58:54.90 +58:10:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247694_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247694_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247712_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247712_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247717_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247717_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:33:01.72 +59:16:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247720_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247720_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247722_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247722_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247723_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247723_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:12:30.95 +61:17:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247724_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247724_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247726_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247726_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247734_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247734_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:14:01.30 +57:40:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247735_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247735_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
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Considering the candidate 247736_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247736_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247737_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247737_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:09:38.15 +63:02:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247740_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247740_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247741_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247741_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247742_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247742_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247746_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247746_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:20:45.80 +57:55:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247750_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247750_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247751_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247751_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247758_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247758_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:09:47.66 +58:11:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247759_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247759_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:05:56.89 +63:03:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247760_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247760_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:10:37.50 +57:22:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247761_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247761_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:19:24.10 +58:26:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247763_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247763_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:46:42.57 +61:09:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247765_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247765_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247768_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247768_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:01:30.83 +65:05:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247771_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247771_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247778_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247778_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:12:40.84 +61:20:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247779_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247779_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:14:45.33 +60:30:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247782_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247782_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:07:08.04 +57:44:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247783_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 247783_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 247788_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247788_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:15:55.90 +58:23:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247789_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247789_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:43:59.17 +61:55:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247790_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247790_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:55:14.55 +59:32:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247792_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247792_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:20:24.32 +59:10:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247795_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247795_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:15:16.98 +57:28:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247801_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 247801_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:22:08.34 +60:22:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249389_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 249389_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 251310_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 251310_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:44:01.95 +61:53:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251496_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 251496_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:46:08.64 +61:12:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251954_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 251954_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:38:00.45 +57:56:45.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252168_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 252168_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:26:40.90 +60:46:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252311_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 252311_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:19:11.09 +58:20:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252402_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 252402_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
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Considering the candidate 254944_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 254944_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:28:15.46 +58:44:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254973_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 254973_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:58:16.36 +59:38:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255731_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 255731_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:18:14.00 +61:44:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256236_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 256236_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:46:33.58 +61:16:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256463_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 256463_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:43:52.96 +61:53:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256608_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 256608_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:20:11.04 +58:12:08.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 257035_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 257035_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:15:58.84 +63:12:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257077_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 257077_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:16:08.46 +58:49:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257372_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 257372_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:44:17.62 +61:53:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257571_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 257571_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:11:23.00 +61:21:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257627_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 257627_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:00:51.78 +58:31:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257637_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 257637_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:44:32.33 +58:45:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257684_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 257684_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:31:36.97 +58:38:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257764_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 257764_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:02:54.92 +64:24:58.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 258369_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 258369_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:19:22.16 +58:19:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258992_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 258992_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:43:03.27 +58:08:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259192_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 259192_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:26:35.82 +57:57:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259433_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 259433_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:42:33.40 +63:52:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259481_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 259481_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:39:00.14 +61:11:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259500_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 259500_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:16:36.19 +64:57:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259604_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 259604_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:13:35.89 +57:52:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259689_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 259689_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:16:05.00 +58:49:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259934_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 259934_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:39:56.90 +60:52:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259942_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 259942_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:00:36.75 +58:30:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260237_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 260237_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:13:30.01 +58:34:24.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 260461_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 260461_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:34:10.25 +62:09:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260662_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 260662_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:33:23.17 +57:44:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260755_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 260755_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:19:03.77 +63:57:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260987_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 260987_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:47:18.73 +63:38:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261001_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 261001_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 261167_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 261167_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:21:28.97 +63:55:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261217_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 261217_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:37:13.54 +58:38:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261280_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 261280_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:40:34.89 +60:45:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261316_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 261316_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:35:50.47 +61:27:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261559_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 261559_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:08:30.42 +58:24:17.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261753_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 261753_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:38:11.97 +61:01:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261756_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 261756_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 261822_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 261822_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:01:36.87 +59:57:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262002_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 262002_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 262109_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 262109_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:10:23.85 +60:01:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262423_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 262423_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 262441_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 262441_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:42:55.14 +64:01:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262452_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 262452_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:43:06.97 +58:57:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262553_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 262553_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:14:29.97 +63:16:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262613_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 262613_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:06:23.29 +62:44:03.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262695_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 262695_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:38:33.96 +58:07:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262712_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 262712_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:58:04.20 +57:58:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262803_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 262803_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 262808_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 262808_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:55:22.17 +64:02:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262812_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 262812_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 263023_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 263023_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:42:28.36 +58:17:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263069_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 263069_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:38:07.51 +61:01:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263228_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 263228_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 263247_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 263247_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:37:13.05 +58:38:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263400_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 263400_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:16:02.70 +60:36:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263413_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 263413_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 263458_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 263458_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:33:24.66 +58:21:28.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263497_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 263497_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:14:00.59 +59:02:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263654_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 263654_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:55:53.07 +64:15:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263752_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 263752_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
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Considering the candidate 263753_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 263753_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:10:32.36 +59:59:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263893_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 263893_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 263960_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 263960_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:20:40.60 +60:23:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264026_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264026_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:39:24.17 +58:23:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264105_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264105_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:29:33.99 +63:19:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264110_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264110_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:59:05.92 +59:55:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264115_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264115_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:19:41.10 +62:51:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264125_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264125_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:18:04.31 +65:36:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264189_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264189_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:02:54.04 +60:15:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264263_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 264263_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 264337_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264337_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:38:33.84 +60:47:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264355_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264355_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:16:24.59 +58:04:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264379_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264379_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:01:38.76 +61:45:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264429_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 264429_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 264473_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264473_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:16:37.01 +64:56:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264792_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264792_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:02:50.60 +60:14:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264921_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264921_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:44:56.58 +59:46:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264938_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 264938_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 264971_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 264971_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:31:32.43 +61:02:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265161_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 265161_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
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Considering the candidate 265332_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 265332_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:37:41.20 +58:37:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265338_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 265338_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:48:39.85 +59:09:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265387_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 265387_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:33:46.66 +62:31:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265562_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 265562_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:54:34.86 +59:52:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265569_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 265569_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:49:06.09 +65:23:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265578_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 265578_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:43:12.80 +64:00:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265731_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 265731_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 266083_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 266083_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:42:26.65 +59:34:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266092_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 266092_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:23:07.52 +61:11:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266150_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 266150_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 266571_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 266571_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:43:03.31 +58:57:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266846_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 266846_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:36:07.38 +59:27:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267004_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 267004_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:15:05.41 +64:08:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267121_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 267121_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 267192_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 267192_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:14:00.30 +61:42:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267268_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 267268_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:14:58.30 +60:30:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267621_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 267621_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 267690_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 267690_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 267809_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 267809_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
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Considering the candidate 268239_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 268239_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:31:48.28 +64:22:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268645_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 268645_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 268674_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 268674_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 268958_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 268958_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
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Considering the candidate 269313_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 269313_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:53:03.04 +60:26:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269495_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 269495_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:03:25.34 +57:50:12.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270282_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
Preparing report for the candidate 270282_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21138_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 21138_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:15:23.61 +65:01:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 112593_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:21:55.02 +61:20:59.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 70271_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:20:32.57 +62:32:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 72532_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:45:35.67 +63:07:03.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34158_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 34158_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:39:32.48 +64:53:04.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 76113_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 02:02:02.08 +62:41:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163
The candidate 39378_fd_Cas-03-Q2b1x1_2026-06-09_02-52-12_20.00sec_4.90C_LIGHT_0163 did not pass the final checks
**** FOUND 01:47:55.48 +64:32:55.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 448s
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 ####
01:33:43.47 +59:31:30.8
01:23:12.04 +57:57:40.4
01:51:52.54 +64:18:35.3
01:44:26.93 +60:39:07.6
01:54:45.45 +57:45:51.0
01:10:43.80 +60:59:18.3
01:40:18.24 +61:21:04.6
01:32:23.25 +61:29:12.8
02:00:06.48 +59:00:31.6
01:07:45.96 +57:45:03.5
01:06:12.97 +59:33:47.6
01:07:39.11 +59:59:18.1
01:17:00.42 +61:01:57.8
01:43:27.28 +58:38:06.4
02:07:25.47 +57:54:58.3
01:08:59.53 +60:47:22.1
01:25:45.82 +59:01:23.1
01:35:27.46 +60:33:46.8
01:17:15.32 +57:23:49.5
01:49:15.78 +59:14:38.4
01:31:23.18 +59:33:42.9
01:19:08.61 +60:33:58.8
01:04:09.16 +63:14:40.9
01:15:19.62 +57:44:09.2
02:04:11.04 +57:54:37.8
02:00:26.45 +63:04:26.4
01:46:55.17 +59:54:51.7
01:47:13.05 +57:44:18.9
01:46:38.60 +60:07:32.7
01:51:09.39 +64:52:46.4
01:15:26.33 +58:04:29.8
02:02:42.34 +60:04:29.1
01:22:11.05 +59:09:01.5
02:02:23.86 +59:42:16.1
02:18:27.81 +59:22:12.8
01:44:03.17 +61:54:44.9
02:04:00.80 +58:29:05.8
02:10:48.74 +58:01:14.3
02:00:32.91 +59:40:07.8
01:06:55.35 +59:18:56.7
01:15:35.34 +58:55:23.2
02:11:59.67 +63:23:12.5
01:46:02.90 +58:23:58.1
01:22:24.01 +61:13:52.0
01:50:39.94 +62:00:56.6
01:24:11.90 +59:17:53.7
01:31:19.96 +58:54:35.9
########### 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 ####
01:33:43.47 +59:31:30.8
01:23:12.04 +57:57:40.4
01:51:52.54 +64:18:35.3
01:44:26.93 +60:39:07.6
01:54:45.45 +57:45:51.0
01:10:43.80 +60:59:18.3
01:40:18.24 +61:21:04.6
01:32:23.25 +61:29:12.8
02:00:06.48 +59:00:31.6
01:07:45.96 +57:45:03.5
01:06:12.97 +59:33:47.6
01:07:39.11 +59:59:18.1
01:17:00.42 +61:01:57.8
01:43:27.28 +58:38:06.4
02:07:25.47 +57:54:58.3
01:08:59.53 +60:47:22.1
01:25:45.82 +59:01:23.1
01:35:27.46 +60:33:46.8
01:17:15.32 +57:23:49.5
01:49:15.78 +59:14:38.4
01:31:23.18 +59:33:42.9
01:19:08.61 +60:33:58.8
01:04:09.16 +63:14:40.9
01:15:19.62 +57:44:09.2
02:04:11.04 +57:54:37.8
02:00:26.45 +63:04:26.4
01:46:55.17 +59:54:51.7
01:47:13.05 +57:44:18.9
01:46:38.60 +60:07:32.7
01:51:09.39 +64:52:46.4
01:15:26.33 +58:04:29.8
02:02:42.34 +60:04:29.1
01:22:11.05 +59:09:01.5
02:02:23.86 +59:42:16.1
02:18:27.81 +59:22:12.8
01:44:03.17 +61:54:44.9
02:04:00.80 +58:29:05.8
02:10:48.74 +58:01:14.3
02:00:32.91 +59:40:07.8
01:06:55.35 +59:18:56.7
01:15:35.34 +58:55:23.2
02:11:59.67 +63:23:12.5
01:46:02.90 +58:23:58.1
01:22:24.01 +61:13:52.0
01:50:39.94 +62:00:56.6
01:24:11.90 +59:17:53.7
01:31:19.96 +58:54:35.9
###################################################################################
01:33:43.47 +59:31:30.8 -- not an asteroid (will add it to exclusion list)
01:23:12.04 +57:57:40.4 -- not an asteroid (will add it to exclusion list)
01:51:52.54 +64:18:35.3 -- not an asteroid (will add it to exclusion list)
01:44:26.93 +60:39:07.6 -- not an asteroid (will add it to exclusion list)
01:54:45.45 +57:45:51.0 -- not an asteroid (will add it to exclusion list)
01:10:43.80 +60:59:18.3 -- not an asteroid (will add it to exclusion list)
01:40:18.24 +61:21:04.6 -- not an asteroid (will add it to exclusion list)
01:32:23.25 +61:29:12.8 -- not an asteroid (will add it to exclusion list)
02:00:06.48 +59:00:31.6 -- not an asteroid (will add it to exclusion list)
01:07:45.96 +57:45:03.5 -- not an asteroid (will add it to exclusion list)
01:06:12.97 +59:33:47.6 -- not an asteroid (will add it to exclusion list)
01:07:39.11 +59:59:18.1 -- not an asteroid (will add it to exclusion list)
01:17:00.42 +61:01:57.8 -- not an asteroid (will add it to exclusion list)
01:43:27.28 +58:38:06.4 -- not an asteroid (will add it to exclusion list)
02:07:25.47 +57:54:58.3 -- not an asteroid (will add it to exclusion list)
01:08:59.53 +60:47:22.1 -- not an asteroid (will add it to exclusion list)
01:25:45.82 +59:01:23.1 -- not an asteroid (will add it to exclusion list)
01:35:27.46 +60:33:46.8 -- not an asteroid (will add it to exclusion list)
01:17:15.32 +57:23:49.5 -- not an asteroid (will add it to exclusion list)
01:49:15.78 +59:14:38.4 -- not an asteroid (will add it to exclusion list)
01:31:23.18 +59:33:42.9 -- not an asteroid (will add it to exclusion list)
01:19:08.61 +60:33:58.8 -- not an asteroid (will add it to exclusion list)
01:04:09.16 +63:14:40.9 -- not an asteroid (will add it to exclusion list)
01:15:19.62 +57:44:09.2 -- not an asteroid (will add it to exclusion list)
02:04:11.04 +57:54:37.8 -- not an asteroid (will add it to exclusion list)
02:00:26.45 +63:04:26.4 -- not an asteroid (will add it to exclusion list)
01:46:55.17 +59:54:51.7 -- not an asteroid (will add it to exclusion list)
01:47:13.05 +57:44:18.9 -- not an asteroid (will add it to exclusion list)
01:46:38.60 +60:07:32.7 -- not an asteroid (will add it to exclusion list)
01:51:09.39 +64:52:46.4 -- not an asteroid (will add it to exclusion list)
01:15:26.33 +58:04:29.8 -- not an asteroid (will add it to exclusion list)
02:02:42.34 +60:04:29.1 -- not an asteroid (will add it to exclusion list)
01:22:11.05 +59:09:01.5 -- not an asteroid (will add it to exclusion list)
02:02:23.86 +59:42:16.1 -- not an asteroid (will add it to exclusion list)
02:18:27.81 +59:22:12.8 -- not an asteroid (will add it to exclusion list)
01:44:03.17 +61:54:44.9 -- not an asteroid (will add it to exclusion list)
02:04:00.80 +58:29:05.8 -- not an asteroid (will add it to exclusion list)
02:10:48.74 +58:01:14.3 -- not an asteroid (will add it to exclusion list)
02:00:32.91 +59:40:07.8 -- not an asteroid (will add it to exclusion list)
01:06:55.35 +59:18:56.7 -- not an asteroid (will add it to exclusion list)
01:15:35.34 +58:55:23.2 -- not an asteroid (will add it to exclusion list)
02:11:59.67 +63:23:12.5 -- not an asteroid (will add it to exclusion list)
01:46:02.90 +58:23:58.1 -- not an asteroid (will add it to exclusion list)
01:22:24.01 +61:13:52.0 -- not an asteroid (will add it to exclusion list)
01:50:39.94 +62:00:56.6 -- not an asteroid (will add it to exclusion list)
01:24:11.90 +59:17:53.7 -- not an asteroid (will add it to exclusion list)
01:31:19.96 +58:54:35.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:04:09.16 +63:14:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:12.97 +59:33:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:55.35 +59:18:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.11 +59:59:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:45.96 +57:45:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:59.53 +60:47:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:43.80 +60:59:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:19.62 +57:44:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:26.33 +58:04:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:35.34 +58:55:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:00.42 +61:01:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:15.32 +57:23:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:08.61 +60:33:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:11.05 +59:09:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:24.01 +61:13:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:12.04 +57:57:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:11.90 +59:17:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:45.82 +59:01:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:19.96 +58:54:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:23.18 +59:33:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:23.25 +61:29:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:43.47 +59:31:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:27.46 +60:33:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:18.24 +61:21:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:27.28 +58:38:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:03.17 +61:54:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:26.93 +60:39:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:02.90 +58:23:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.60 +60:07:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:55.17 +59:54:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:13.05 +57:44:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:15.78 +59:14:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:39.94 +62:00:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:09.39 +64:52:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:52.54 +64:18:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:45.45 +57:45:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:06.48 +59:00:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:26.45 +63:04:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:32.91 +59:40:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:23.86 +59:42:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:42.34 +60:04:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:00.80 +58:29:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:11.04 +57:54:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:25.47 +57:54:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:48.74 +58:01:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:59.67 +63:23:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:27.81 +59:22:12.8 -- 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)
01:04:09.16 +63:14:40.9 -- not a known variable star
01:06:12.97 +59:33:47.6 -- not a known variable star
01:06:55.35 +59:18:56.7 -- not a known variable star
01:07:39.11 +59:59:18.1 -- not a known variable star
01:07:45.96 +57:45:03.5 -- not a known variable star
01:08:59.53 +60:47:22.1 -- not a known variable star
01:10:43.80 +60:59:18.3 -- not a known variable star
01:15:19.62 +57:44:09.2 -- not a known variable star
01:15:26.33 +58:04:29.8 -- not a known variable star
01:15:35.34 +58:55:23.2 -- a known variable star
01:17:00.42 +61:01:57.8 -- not a known variable star
01:17:15.32 +57:23:49.5 -- not a known variable star
01:19:08.61 +60:33:58.8 -- not a known variable star
01:22:11.05 +59:09:01.5 -- not a known variable star
01:22:24.01 +61:13:52.0 -- a known variable star
01:23:12.04 +57:57:40.4 -- not a known variable star
01:24:11.90 +59:17:53.7 -- not a known variable star
01:25:45.82 +59:01:23.1 -- not a known variable star
01:31:19.96 +58:54:35.9 -- not a known variable star
01:31:23.18 +59:33:42.9 -- not a known variable star
01:32:23.25 +61:29:12.8 -- a known variable star
01:33:43.47 +59:31:30.8 -- not a known variable star
01:35:27.46 +60:33:46.8 -- not a known variable star
01:40:18.24 +61:21:04.6 -- not a known variable star
01:43:27.28 +58:38:06.4 -- a known variable star
01:44:03.17 +61:54:44.9 -- not a known variable star
01:44:26.93 +60:39:07.6 -- not a known variable star
01:46:02.90 +58:23:58.1 -- not a known variable star
01:46:38.60 +60:07:32.7 -- not a known variable star
01:46:55.17 +59:54:51.7 -- not a known variable star
01:47:13.05 +57:44:18.9 -- a known variable star
01:49:15.78 +59:14:38.4 -- not a known variable star
01:50:39.94 +62:00:56.6 -- not a known variable star
01:51:09.39 +64:52:46.4 -- a known variable star
01:51:52.54 +64:18:35.3 -- not a known variable star
01:54:45.45 +57:45:51.0 -- a known variable star
02:00:06.48 +59:00:31.6 -- not a known variable star
02:00:26.45 +63:04:26.4 -- a known variable star
02:00:32.91 +59:40:07.8 -- a known variable star
02:02:23.86 +59:42:16.1 -- not a known variable star
02:02:42.34 +60:04:29.1 -- not a known variable star
02:04:00.80 +58:29:05.8 -- not a known variable star
02:04:11.04 +57:54:37.8 -- a known variable star
02:07:25.47 +57:54:58.3 -- not a known variable star
02:10:48.74 +58:01:14.3 -- not a known variable star
02:11:59.67 +63:23:12.5 -- a known variable star
02:18:27.81 +59:22:12.8 -- not a known variable star
Found 36 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, 36 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)2461200.82755694 -observatory V36
06:50:24.27 +24:46:60.0 Mercury (0.1mag)
07:48:33.56 +23:09:04.5 Venus (-4.0mag)
02:52:54.79 +15:58:06.9 Mars (1.3mag)
07:49:23.12 +21:29:03.5 Jupiter (-1.9mag)
00:49:41.72 +02:50:25.5 Saturn (0.9mag)
04:00:28.61 +20:26:14.2 Uranus (5.8mag)
00:16:12.48 +00:17:10.1 Neptune (7.8mag)
20:33:17.59 -23:04:58.6 Pluto (14.5mag)
23:56:50.38 +01:16:13.9 Moon (-10.1mag)
-rw-r--r-- 1 apache apache 362 Jun 9 04:49 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461200.82755694:
07:49:19.08 +21:29:14.8 Io (6.0mag)
07:49:34.30 +21:28:29.1 Europa (6.2mag)
07:49:13.64 +21:29:36.6 Ganymede (5.6mag)
07:49:30.00 +21:28:36.8 Callisto (6.7mag)
07:49:36.38 +21:05:26.3 Himalia (15.6mag)
07:49:22.63 +21:29:06.4 Thebe (16.5mag)
07:49:33.94 +21:20:22.8 Elara (17.5mag)
07:51:37.33 +21:40:08.2 Pasiphae (17.7mag)
07:55:55.22 +21:30:51.1 Carme (18.9mag)
00:49:35.59 +02:50:12.8 Titan (8.7mag)
00:49:39.04 +02:50:22.7 Rhea (9.9mag)
00:50:13.30 +02:52:41.3 Iapetus (11.3mag)
00:49:41.93 +02:49:57.3 Hyperion (14.7mag)
00:50:22.58 +02:52:12.2 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 9 04:49 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461200.82755694:
17:26:23.30 -35:22:19.0 JWST
17:52:07.75 +35:21:11.9 Chandra
09:11:38.55 -52:20:13.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 9 04:49 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461200.82755694 -observatory V36
18:42:43.42 -32:44:11.1 13.6mag P/2010 H2 (Vales)
05:54:35.31 -68:03:09.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:49:28.64 +31:58:58.3 17.5mag C/2017 K2 (PANSTARRS)
17:14:16.60 +15:24:28.0 17.8mag C/2021 G2 (ATLAS)
21:22:48.07 -48:52:54.4 16.8mag P/2021 N1 (ZTF)
23:12:22.69 +31:38:06.1 17.2mag C/2022 E2 (ATLAS)
05:35:25.96 +26:58:54.7 16.5mag C/2022 N2 (PANSTARRS)
09:30:32.73 +31:02:34.0 16.6mag C/2022 QE78 (ATLAS)
08:51:09.35 +03:59:09.0 17.7mag C/2022 R6 (PANSTARRS)
18:27:28.88 +21:37:23.6 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:18:58.08 -11:00:38.1 17.6mag P/2023 B1 (PANSTARRS)
22:14:02.76 +66:35:52.0 17.7mag C/2023 H5 (Lemmon)
17:43:35.01 -06:48:00.9 13.7mag C/2023 R1 (PANSTARRS)
13:17:33.34 +82:44:04.8 17.9mag C/2023 X2 (Lemmon)
07:11:59.69 +64:20:50.1 17.7mag C/2024 A1 (ATLAS)
06:48:59.45 +27:56:06.0 13.7mag C/2024 E1 (Wierzchos)
15:36:24.15 +13:37:28.8 17.4mag C/2024 G6 (ATLAS)
20:12:17.11 +31:28:20.4 14.0mag C/2024 J3 (ATLAS)
04:19:09.82 -15:51:07.9 16.0mag C/2024 T5 (ATLAS)
06:06:58.21 +34:17:40.3 17.9mag C/2025 J1 (Borisov)
11:34:22.96 +52:41:00.1 17.5mag C/2025 L1 (ATLAS)
06:46:19.11 -10:55:17.4 14.2mag C/2025 R3 (PANSTARRS)
09:25:05.66 +23:19:28.5 17.9mag C/2025 V2 (Rankin)
12:39:40.72 +04:41:11.9 17.2mag C/2025 Y1 (ATLAS)
18:11:03.14 +75:22:33.7 17.9mag C/2026 A2 (Bok)
02:02:37.86 +43:29:45.2 16.1mag C/2026 B2 (Sun-Gao)
11:11:33.08 -03:20:13.2 16.5mag A/2026 E1
20:25:42.31 -08:39:13.4 8.7mag 10P/Tempel
11:02:16.44 -00:59:04.2 16.0mag 29P/Schwassmann-Wachmann
03:13:28.57 +25:47:49.5 17.7mag 47P/Ashbrook-Jackson
09:02:23.89 +23:26:41.0 16.9mag 63P/Wild
00:27:53.81 -06:17:43.1 15.7mag 65P/Gunn
06:47:07.10 +33:32:29.0 16.9mag 76P/West-Kohoutek-Ikemura
03:11:55.41 +17:21:37.4 13.8mag 78P/Gehrels
01:23:13.01 +05:05:41.5 15.6mag 88P/Howell
04:58:17.60 +30:23:09.6 15.3mag 93P/Lovas
02:46:09.94 +27:48:23.3 17.6mag 114P/Wiseman-Skiff
06:53:15.22 +32:59:45.1 15.6mag 123P/West-Hartley
09:52:09.11 +14:09:07.8 16.5mag 124P/Mrkos
04:00:54.45 +19:19:32.5 16.3mag 128P/Shoemaker-Holt
04:35:49.18 +19:08:08.3 17.7mag 131P/Mueller
06:03:09.50 +18:31:55.3 14.8mag 141P/Machholz
06:05:51.11 +17:43:52.6 14.7mag 141P-A/Machholz
04:59:47.15 +16:19:30.5 11.7mag 141P-D/Machholz
02:58:28.66 -24:32:35.3 16.8mag 161P/Hartley-IRAS
03:45:16.84 +24:15:41.6 14.9mag 162P/SidingSpring
19:36:31.46 +02:03:55.8 16.8mag 169P/NEAT
00:21:23.31 +02:41:12.2 17.9mag 220P/McNaught
16:51:18.97 -08:25:18.9 16.4mag 235P/LINEAR
07:37:13.16 +35:26:37.1 17.5mag 240P/NEAT
00:35:19.68 -01:59:12.3 16.4mag 260P/McNaught
04:07:18.66 +32:41:08.6 17.6mag 295P/LINEAR
23:59:23.99 -08:16:41.3 17.6mag 320P/McNaught
15:14:43.89 +08:03:36.0 17.4mag 391P/Kowalski
08:08:02.50 +20:43:04.3 17.9mag 450P/LONEOS
07:01:49.36 +41:36:56.6 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 9 04:49 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
-rw-r--r-- 1 apache apache 5.6K Jun 9 04:49 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
-rw-r--r-- 1 apache apache 189K Jun 9 04:49 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:54:07.658 +36:09:50.41 AT 2026nzq 2026-05-24.31 21.1
21:44:04.717 +27:46:38.98 AT 2026nzp 2026-05-17.58 20.83
12:27:36.098 -15:58:04.48 AT 2026nzo 2026-05-17.30 21.29
14:11:34.726 -18:41:44.43 AT 2026nzn 2026-05-12.39 20.14
14:39:35.732 +03:36:10.16 AT 2026nzm 2026-05-17.43 21.46
18:57:23.847 +36:06:28.19 AT 2026nzl 2026-05-20.54 20.51
13:57:08.090 +14:19:48.68 AT 2026nzk 2026-05-17.29 20.8
20:45:44.317 -10:53:29.02 AT 2026nzj 2026-05-21.57 20.34
16:39:34.881 +16:26:14.93 AT 2026nzi 2026-05-25.50 21.83
20:58:52.189 -01:30:50.16 AT 2026nzh 2026-05-24.58 21.41
19:48:21.568 -26:10:28.53 AT 2026nzg 2026-05-17.56 21.45
12:26:04.245 +14:58:26.65 AT 2026nzf 2026-05-21.38 20.69
18:26:57.143 +35:10:02.54 AT 2026nze 2026-05-20.52 21.27
20:32:23.257 -22:31:24.00 AT 2026nzd 2026-06-01.46 19.2469
12:23:45.699 -19:15:23.33 AT 2026nzc 2026-06-01.19 18.8563
13:34:02.732 +31:31:27.24 AT 2026nzb 2026-05-14.45 18.822
18:41:54.001 +51:59:06.99 AT 2026nza 2026-06-01.06 19.06
15:30:36.749 +74:35:36.76 AT 2026nyz 2026-06-01.00 18.495
11:56:02.494 +23:53:38.13 AT 2026nyy 2026-05-30.32 20.08
00:30:02.916 +22:54:14.63 AT 2026nyx 2026-05-31.48 19.2096
-rw-r--r-- 1 apache apache 30K Jun 9 04:49 tns_transients_list.txt
