This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.39 01:25:00.79 +59:33:43.7
127.17889 -3.03246 galactic Cas Second-epoch detections are separated by 3.9" and 5.1 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 510086091499587328 | 01:25:05.43 +59:33:35.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.141+/-0.051 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:00.79 +59:33:43.7: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:00.79 +59:33:43.7: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 25 00.79 +59 33 43.7 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 510086091499587328,2461176.8930,11.39,0.05,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
Gaia DR3 510086091499587328 20260516.3930 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 05 16.3930 2461176.8930 11.55 01:20:35.65 +63:20:53.0
126.19474 0.66117 galactic Cas Second-epoch detections are separated by 3.4" and 4.8 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 | 01:20:35.65 +63:20:53.0 (user input) | T | P | (position from user input) J-Ks=0.480+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:35.65 +63:20:53.0: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:35.65 +63:20:53.0: 14.43 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 20 35.65 +63 20 53.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461176.8930,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260516.3930 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.36 01:44:27.79 +63:24:10.7
128.82568 1.13962 galactic Cas Second-epoch detections are separated by 1.8" 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 | target | 01:44:27.79 +63:24:10.7 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:27.79 +63:24:10.7: 12.83 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:27.79 +63:24:10.7: 14.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 44 27.79 +63 24 10.7 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
target,2461176.8930,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260516.3930 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.36 01:49:53.19 +63:40:48.9
129.35642 1.53993 galactic Cas Second-epoch detections are separated by 2.8" 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 | target | 01:49:53.19 +63:40:48.9 (user input) | T | P | (position from user input) J-Ks=0.868+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:53.19 +63:40:48.9: 12.16 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:53.19 +63:40:48.9: 13.92 +/- 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 05 16.3930* 01 49 53.19 +63 40 48.9 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
target,2461176.8930,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260516.3930 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.40 01:46:36.33 +64:06:19.9
128.91109 1.87608 galactic Cas Second-epoch detections are separated by 3.2" 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 | 01:46:36.33 +64:06:19.9 (user input) | T | P | (position from user input) J-Ks=0.862+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:36.33 +64:06:19.9: 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 01:46:36.33 +64:06:19.9: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 05 16.3930* 01 46 36.33 +64 06 19.9 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
target,2461176.8930,11.40,0.05,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 20260516.3930 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.21 01:37:23.59 +59:20:12.7
128.77006 -3.01297 galactic Cas Second-epoch detections are separated by 1.0" 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 | target | 01:37:23.59 +59:20:12.7 (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 01:37:23.59 +59:20:12.7: 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 01:37:23.59 +59:20:12.7: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 37 23.59 +59 20 12.7 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
target,2461176.8930,11.21,0.05,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 20260516.3930 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 05 16.3930 2461176.8930 11.08 01:09:24.69 +58:01:36.0
125.31776 -4.76180 galactic Cas Second-epoch detections are separated by 0.7" 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 | target | 01:09:24.69 +58:01:36.0 (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 01:09:24.69 +58:01:36.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:24.69 +58:01:36.0: 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 05 16.3930* 01 09 24.69 +58 01 36.0 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,2461176.8930,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260516.3930 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.21 01:22:33.02 +60:44:43.0
126.72621 -1.89706 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 | 01:22:33.02 +60:44:43.0 (user input) | T | P | (position from user input) J-Ks=1.158+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:33.02 +60:44:43.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:33.02 +60:44:43.0: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 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 05 16.3930* 01 22 33.02 +60 44 43.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461176.8930,11.21,0.05,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 20260516.3930 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 05 16.3930 2461176.8930 11.11 01:30:01.08 +60:10:49.8
127.71498 -2.33247 galactic Cas Second-epoch detections are separated by 2.5" and 4.8 pix
The object was found in VSX22" Gaia DR3 509459713474637440
Type: VAR
# Max. Min./Amp. JD0 Period
13.340 G 13.370 G 0.014865300000 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 01:30:01.08 +60:10:49.8: 12.56 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:01.08 +60:10:49.8: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 05 16.3930* 01 30 01.08 +60 10 49.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509459713474637440,2461176.8930,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509459713474637440 20260516.3930 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.31 01:42:09.06 +64:21:26.0
128.38552 2.02378 galactic Cas Second-epoch detections are separated by 1.5" 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 | target | 01:42:09.06 +64:21:26.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:09.06 +64:21:26.0: 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 01:42:09.06 +64:21:26.0: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 42 09.06 +64 21 26.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461176.8930,11.31,0.05,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 20260516.3930 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.98 01:56:31.39 +58:17:39.4
131.41568 -3.50135 galactic Cas Second-epoch detections are separated by 0.7" 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 | 01:56:31.39 +58:17:39.4 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.458+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:31.39 +58:17:39.4: 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 01:56:31.39 +58:17:39.4: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 56 31.39 +58 17 39.4 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,2461176.8930,10.98,0.05,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 20260516.3930 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.16 01:17:36.00 +57:49:40.9
126.42167 -4.86634 galactic Cas Second-epoch detections are separated by 1.2" and 4.8 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 | 01:17:36.00 +57:49:40.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:36.00 +57:49:40.9: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:36.00 +57:49:40.9: 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 05 16.3930* 01 17 36.00 +57 49 40.9 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,2461176.8930,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260516.3930 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.04 01:24:54.87 +59:41:46.9
127.14905 -2.90100 galactic Cas Second-epoch detections are separated by 4.2" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:24:54.87 +59:41:46.9 (user input) | T | P | (position from user input) J-Ks=0.217+/-0.043 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:54.87 +59:41:46.9: 12.93 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:54.87 +59:41:46.9: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 24 54.87 +59 41 46.9 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,2461176.8930,11.04,0.05,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 20260516.3930 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 05 16.3930 2461176.8930 10.99 01:09:10.42 +58:09:35.8
125.27701 -4.63102 galactic Cas Second-epoch detections are separated by 0.8" and 4.8 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 | 01:09:10.42 +58:09:35.8 (user input) | T | P | (position from user input) J-Ks=0.750+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:10.42 +58:09:35.8: 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 01:09:10.42 +58:09:35.8: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 09 10.42 +58 09 35.8 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
target,2461176.8930,10.99,0.05,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
target 20260516.3930 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 05 16.3930 2461176.8930 11.06 01:47:27.53 +58:28:39.1
130.21555 -3.59976 galactic Cas Second-epoch detections are separated by 5.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.8623+58.4762 | 01:47:26.06 +58:28:04.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1960IzKry..24..160B [B60] +58 471
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:27.53 +58:28:39.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:27.53 +58:28:39.1: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 47 27.53 +58 28 39.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.8623+58.4762,2461176.8930,11.06,0.05,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 J026.8623+58.4762 20260516.3930 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.08 01:26:05.65 +59:01:14.9
127.38760 -3.55080 galactic Cas Second-epoch detections are separated by 1.6" 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 J021.5231+59.0209 | 01:26:05.65 +59:01:14.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.314+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.65 +59:01:14.9: 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 01:26:05.65 +59:01:14.9: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 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 05 16.3930* 01 26 05.65 +59 01 14.9 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
ATO J021.5231+59.0209,2461176.8930,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.5231+59.0209 20260516.3930 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.91 01:09:21.61 +64:35:17.0
124.85396 1.78321 galactic Cas Second-epoch detections are separated by 2.9" 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 | target | 01:09:21.61 +64:35:17.0 (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 01:09:21.61 +64:35:17.0: 12.82 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:21.61 +64:35:17.0: 13.61 +/- 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 05 16.3930* 01 09 21.61 +64 35 17.0 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,2461176.8930,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260516.3930 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 05 16.3930 2461176.8930 10.87 01:43:27.18 +58:38:07.4
129.67065 -3.55415 galactic Cas Second-epoch detections are separated by 2.9" and 4.9 pix
The object was found in VSX 3" 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 01:43:27.18 +58:38:07.4: 12.75 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.18 +58:38:07.4: 13.63 +/- 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 05 16.3930* 01 43 27.18 +58 38 07.4 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 506084487648397824,2461176.8930,10.87,0.05,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 506084487648397824 20260516.3930 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 05 16.3930 2461176.8930 11.13 02:00:06.36 +59:00:32.7
131.68319 -2.69098 galactic Cas Second-epoch detections are separated by 1.7" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02:00:06.36 +59:00:32.7: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:06.36 +59:00:32.7: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 02 00 06.36 +59 00 32.7 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 507781618204489856,2461176.8930,11.13,0.05,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 20260516.3930 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.05 01:06:13.06 +59:33:47.0
124.80579 -3.25491 galactic Cas Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:13.06 +59:33:47.0 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:13.06 +59:33:47.0: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:13.06 +59:33:47.0: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 06 13.06 +59 33 47.0 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,2461176.8930,11.05,0.05,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 20260516.3930 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.91 01:54:45.35 +57:45:52.5
131.31937 -4.07237 galactic Per Second-epoch detections are separated by 1.1" and 4.5 pix
The object was found in VSX23" 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 01:54:45.35 +57:45:52.5: 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 01:54:45.35 +57:45:52.5: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 54 45.35 +57 45 52.5 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 506102938826140544,2461176.8930,10.91,0.05,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 506102938826140544 20260516.3930 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 05 16.3930 2461176.8930 10.93 01:40:18.08 +61:21:06.8
128.75513 -0.96618 galactic Cas Second-epoch detections are separated by 2.9" 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 | target | 01:40:18.08 +61:21:06.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:18.08 +61:21:06.8: 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 01:40:18.08 +61:21:06.8: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 40 18.08 +61 21 06.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461176.8930,10.93,0.05,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
target 20260516.3930 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 05 16.3930 2461176.8930 10.96 01:10:11.63 +59:17:23.8
125.32903 -3.49448 galactic Cas Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J017.5672+59.2942 | 01:10:11.63 +59:17:23.8 (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 01:10:11.63 +59:17:23.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:11.63 +59:17:23.8: 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 05 16.3930* 01 10 11.63 +59 17 23.8 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
ATO J017.5672+59.2942,2461176.8930,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.5672+59.2942 20260516.3930 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 05 16.3930 2461176.8930 11.04 01:10:02.85 +57:48:13.3
125.41825 -4.97819 galactic Cas Second-epoch detections are separated by 1.7" and 5.1 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 | 01:10:02.85 +57:48:13.3 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:02.85 +57:48:13.3: 12.96 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:02.85 +57:48:13.3: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 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 05 16.3930* 01 10 02.85 +57 48 13.3 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,2461176.8930,11.04,0.05,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 20260516.3930 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 05 16.3930 2461176.8930 10.91 02:00:46.33 +57:54:00.7
132.06095 -3.73739 galactic Per Second-epoch detections are separated by 2.4" 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 J030.1940+57.8929 | 02:00:46.33 +57:54:00.7 (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 02:00:46.33 +57:54:00.7: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:46.33 +57:54:00.7: 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 05 16.3930* 02 00 46.33 +57 54 00.7 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 J030.1940+57.8929,2461176.8930,10.91,0.05,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
ATO J030.1940+57.8929 20260516.3930 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 05 16.3930 2461176.8930 10.99 01:08:25.53 +59:48:03.7
125.06959 -3.00019 galactic Cas Second-epoch detections are separated by 1.7" and 4.9 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 | 01:08:25.53 +59:48:03.7 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:25.53 +59:48:03.7: 12.47 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:25.53 +59:48:03.7: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 08 25.53 +59 48 03.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461176.8930,10.99,0.05,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
target 20260516.3930 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 05 16.3930 2461176.8930 10.95 01:06:59.62 +61:28:38.0
124.78832 -1.33844 galactic Cas Second-epoch detections are separated by 4.6" and 5.0 pix
The object was found in VSX 8" Gaia DR3 522542355648755328
Type: L
# Max. Min./Amp. JD0 Period
17.340 G 17.500 G O
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 01:06:59.62 +61:28:38.0: 13.02 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:59.62 +61:28:38.0: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 06 59.62 +61 28 38.0 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 522542355648755328,2461176.8930,10.95,0.05,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
Gaia DR3 522542355648755328 20260516.3930 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 05 16.3930 2461176.8930 10.78 02:07:25.37 +57:54:58.4
132.90666 -3.47643 galactic Per Second-epoch detections are separated by 1.9" 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 506730034109607680 | 02:07:24.66 +57:55:23.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.827+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:25.37 +57:54:58.4: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:25.37 +57:54:58.4: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 02 07 25.37 +57 54 58.4 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 506730034109607680,2461176.8930,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506730034109607680 20260516.3930 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.84 01:07:39.16 +59:59:18.2
124.96066 -2.81947 galactic Cas Second-epoch detections are separated by 4.2" 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 | 01:07:39.16 +59:59:18.2 (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 01:07:39.16 +59:59:18.2: 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 01:07:39.16 +59:59:18.2: 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 05 16.3930* 01 07 39.16 +59 59 18.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461176.8930,10.84,0.05,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 20260516.3930 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.94 01:51:47.02 +58:37:57.5
130.73147 -3.32229 galactic Cas Second-epoch detections are separated by 1.8" 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 506225156418009984 | 01:51:45.68 +58:37:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:47.02 +58:37:57.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:47.02 +58:37:57.5: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 51 47.02 +58 37 57.5 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
Gaia DR3 506225156418009984,2461176.8930,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506225156418009984 20260516.3930 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.69 01:20:44.87 +57:55:09.3
126.82931 -4.73053 galactic Cas Second-epoch detections are separated by 3.8" 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 413797116609704704 | 01:20:41.29 +57:55:17.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.023+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:44.87 +57:55:09.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:44.87 +57:55:09.3: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 20 44.87 +57 55 09.3 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413797116609704704,2461176.8930,10.69,0.05,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 413797116609704704 20260516.3930 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 05 16.3930 2461176.8930 10.72 01:09:45.72 +61:46:39.2
125.09681 -1.01714 galactic Cas Second-epoch detections are separated by 1.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 522632790482932992 | 01:09:44.37 +61:46:54.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A8 1935BSD...C01....0S BSD 8-1650
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:45.72 +61:46:39.2: 12.53 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:45.72 +61:46:39.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 09 45.72 +61 46 39.2 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 522632790482932992,2461176.8930,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522632790482932992 20260516.3930 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.76 01:26:38.62 +59:41:40.1
127.36577 -2.87385 galactic Cas Second-epoch detections are separated by 2.2" and 5.0 pix
The object was found in VSX 6" Gaia DR3 510083239641442688
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.660 G 13.680 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 01:26:38.62 +59:41:40.1: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:38.62 +59:41:40.1: 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 05 16.3930* 01 26 38.62 +59 41 40.1 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
Gaia DR3 510083239641442688,2461176.8930,10.76,0.05,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
Gaia DR3 510083239641442688 20260516.3930 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 05 16.3930 2461176.8930 10.66 01:13:44.70 +57:24:51.1
125.94501 -5.32699 galactic Cas Second-epoch detections are separated by 1.3" and 4.8 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 | 01:13:44.70 +57:24:51.1 (user input) | T | P | (position from user input) J-Ks=0.655+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:44.70 +57:24:51.1: 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 01:13:44.70 +57:24:51.1: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 13 44.70 +57 24 51.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461176.8930,10.66,0.05,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
target 20260516.3930 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 05 16.3930 2461176.8930 10.62 01:37:09.87 +58:51:06.9
128.82715 -3.49545 galactic Cas Second-epoch detections are separated by 0.4" and 4.6 pix
The object was found in VSX16" Gaia DR3 509131131290597376
Type: ROT
# Max. Min./Amp. JD0 Period
16.600 G 16.660 G 1.529270000000 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 01:37:09.87 +58:51:06.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:09.87 +58:51:06.9: 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 05 16.3930* 01 37 09.87 +58 51 06.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509131131290597376,2461176.8930,10.62,0.05,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 509131131290597376 20260516.3930 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 05 16.3930 2461176.8930 10.70 02:05:14.69 +63:02:38.1
131.18320 1.36064 galactic Cas Second-epoch detections are separated by 3.8" and 4.7 pix
The object was found in VSX10" ZTF J020514.76+630248.4
Type: EW
# Max. Min./Amp. JD0 Period
16.621 r Y 0.211 r 2458457.67520 0.337767600000
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 02:05:14.69 +63:02:38.1: 13.00 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:05:14.69 +63:02:38.1: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 02 05 14.69 +63 02 38.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J020514.76+630248.4,2461176.8930,10.70,0.05,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 J020514.76+630248.4 20260516.3930 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.57 01:31:23.07 +59:33:42.9
127.97870 -2.91783 galactic Cas Second-epoch detections are separated by 1.0" 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 | ATO J022.8294+59.5638 | 01:31:23.07 +59:33:42.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.833+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:23.07 +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 01:31:23.07 +59:33:42.9: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 31 23.07 +59 33 42.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.8294+59.5638,2461176.8930,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.8294+59.5638 20260516.3930 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.38 01:09:46.02 +58:12:06.9
125.35233 -4.58367 galactic Cas Second-epoch detections are separated by 2.9" 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 | target | 01:09:46.02 +58:12:06.9 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.229+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:46.02 +58:12:06.9: 12.57 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:46.02 +58:12:06.9: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 09 46.02 +58 12 06.9 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461176.8930,10.38,0.05,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
target 20260516.3930 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.14 01:46:55.22 +59:54:51.7
129.83930 -2.21122 galactic Cas Second-epoch detections are separated by 1.0" 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 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 01:46:55.22 +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 01:46:55.22 +59:54:51.7: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 46 55.22 +59 54 51.7 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506617853860840320,2461176.8930,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506617853860840320 20260516.3930 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 9.94 01:53:47.13 +60:15:59.7
130.59355 -1.67442 galactic Cas Second-epoch detections are separated by 1.3" 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 508091916700729984 | 01:53:49.28 +60:16:10.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5 1955ApJS....2..123F LF 5 +60 340 J-Ks=0.162+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:53:47.13 +60:15:59.7: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:53:47.13 +60:15:59.7: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 53 47.13 +60 15 59.7 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508091916700729984,2461176.8930,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508091916700729984 20260516.3930 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 9.62 01:20:24.33 +59:10:24.8
126.64254 -3.48933 galactic Cas Second-epoch detections are separated by 0.6" 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 J020.1204+59.1623 | 01:20:25.01 +59:10:05.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.296+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:24.33 +59:10:24.8: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:24.33 +59:10:24.8: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 20 24.33 +59 10 24.8 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J020.1204+59.1623,2461176.8930,9.62,0.05,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
ATO J020.1204+59.1623 20260516.3930 9.62CV 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 05 16.3930 2461176.8930 9.54 01:30:43.82 +60:47:34.5
127.70949 -1.71383 galactic Cas Second-epoch detections are separated by 1.8" and 4.5 pix
The object was found in VSX 1" Gaia DR3 510607049549022848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.370 G 12.390 G 1.920160000000 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 01:30:43.82 +60:47:34.5: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:43.82 +60:47:34.5: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 30 43.82 +60 47 34.5 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510607049549022848,2461176.8930,9.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510607049549022848 20260516.3930 9.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.42 01:18:27.99 +58:11:23.3
126.49867 -4.49464 galactic Cas Second-epoch detections are separated by 1.9" and 5.1 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 J019.6245+58.1745 | 01:18:29.87 +58:10:59.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8III 1951UppAn...2j...1B NGC 457 236 J-Ks=0.371+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:27.99 +58:11:23.3: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:27.99 +58:11:23.3: 13.11 +/- 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 05 16.3930* 01 18 27.99 +58 11 23.3 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J019.6245+58.1745,2461176.8930,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.6245+58.1745 20260516.3930 10.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.68 01:09:09.36 +61:37:28.7
125.03585 -1.17471 galactic Cas Second-epoch detections are separated by 2.0" and 4.7 pix
The object was found in VSX 1" Gaia DR3 522536136541501952
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.570 G 13.610 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 01:09:09.36 +61:37:28.7: 13.09 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:09.36 +61:37:28.7: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 09 09.36 +61 37 28.7 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 522536136541501952,2461176.8930,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522536136541501952 20260516.3930 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.53 01:46:38.40 +60:07:33.6
129.75995 -2.01189 galactic Cas Second-epoch detections are separated by 0.4" 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 | 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 01:46:38.40 +60:07:33.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.40 +60:07:33.6: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 46 38.40 +60 07 33.6 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.6591+60.1406,2461176.8930,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.6591+60.1406 20260516.3930 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.85 02:04:00.85 +58:29:06.4
132.31363 -3.05843 galactic Per Second-epoch detections are separated by 0.5" 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 | ATO J031.0030+58.4847 | 02:04:00.85 +58:29:06.4 (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 02:04:00.85 +58:29:06.4: 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 02:04:00.85 +58:29:06.4: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 02 04 00.85 +58 29 06.4 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 J031.0030+58.4847,2461176.8930,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J031.0030+58.4847 20260516.3930 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.96 01:24:35.78 +59:32:43.9
127.12860 -3.05576 galactic Cas Second-epoch detections are separated by 1.2" and 4.5 pix
The object was found in VSX18" Gaia DR3 510086538176193664
Type: ROT
# Max. Min./Amp. JD0 Period
15.760 G 15.790 G 5.255500000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:35.78 +59:32:43.9: 12.77 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:35.78 +59:32:43.9: 14.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 24 35.78 +59 32 43.9 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 510086538176193664,2461176.8930,10.96,0.05,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 510086538176193664 20260516.3930 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 05 16.3930 2461176.8930 10.98 01:59:33.90 +63:37:10.1
130.41338 1.74167 galactic Cas Second-epoch detections are separated by 0.3" 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 | target | 01:59:33.90 +63:37:10.1 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:33.90 +63:37:10.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:33.90 +63:37:10.1: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 59 33.90 +63 37 10.1 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,2461176.8930,10.98,0.05,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 20260516.3930 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.84 01:56:05.50 +59:57:20.8
130.94807 -1.90589 galactic Cas Second-epoch detections are separated by 3.0" 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 507884903579236736 | 01:56:09.98 +59:57:31.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 1955ApJS....2..123F LF 5 +59 300 J-Ks=0.297+/-0.045 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:05.50 +59:57:20.8: 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 01:56:05.50 +59:57:20.8: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 56 05.50 +59 57 20.8 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 507884903579236736,2461176.8930,10.84,0.05,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 507884903579236736 20260516.3930 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 10.91 01:44:03.15 +61:54:45.7
129.08252 -0.32912 galactic Cas Second-epoch detections are separated by 1.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 01:44:03.15 +61:54:45.7: 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 01:44:03.15 +61:54:45.7: 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 05 16.3930* 01 44 03.15 +61 54 45.7 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
Gaia DR3 511486800591720192,2461176.8930,10.91,0.05,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 511486800591720192 20260516.3930 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 05 16.3930 2461176.8930 10.99 02:20:32.65 +62:45:43.1
132.92736 1.63233 galactic Cas Second-epoch detections are separated by 2.0" and 4.4 pix
The object was found in VSX15" ZTF J022034.82+624545.5
Type: SR
# Max. Min./Amp. JD0 Period
14.855 r Y 0.593 r 2458302.30000 111.117252300000
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 02:20:32.65 +62:45:43.1: 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 02:20:32.65 +62:45:43.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 02 20 32.65 +62 45 43.1 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
ZTF J022034.82+624545.5,2461176.8930,10.99,0.05,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
ZTF J022034.82+624545.5 20260516.3930 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 05 16.3930 2461176.8930 10.90 01:22:11.00 +59:09:03.3
126.87189 -3.48543 galactic Cas Second-epoch detections are separated by 1.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 J-Ks=0.462+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:11.00 +59:09:03.3: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:11.00 +59:09:03.3: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 22 11.00 +59 09 03.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413976852405588480,2461176.8930,10.90,0.05,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 413976852405588480 20260516.3930 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 05 16.3930 2461176.8930 11.07 01:41:34.20 +59:13:56.8
129.31427 -3.01666 galactic Cas Second-epoch detections are separated by 2.2" 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 | 01:41:34.20 +59:13:56.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:34.20 +59:13:56.8: 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 01:41:34.20 +59:13:56.8: 14.08 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 41 34.20 +59 13 56.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461176.8930,11.07,0.05,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
target 20260516.3930 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 05 16.3930 2461176.8930 10.98 01:09:22.61 +57:26:30.6
125.35419 -5.34552 galactic Cas Second-epoch detections are separated by 1.3" 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 J017.3204+57.4562 | 01:09:17.29 +57:26:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.782+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.61 +57:26:30.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.61 +57:26:30.6: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 09 22.61 +57 26 30.6 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
ATO J017.3204+57.4562,2461176.8930,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.3204+57.4562 20260516.3930 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.19 01:21:55.47 +63:45:20.5
126.29481 1.08318 galactic Cas Second-epoch detections are separated by 2.1" 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 | target | 01:21:55.47 +63:45:20.5 (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 01:21:55.47 +63:45:20.5: 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 01:21:55.47 +63:45:20.5: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 21 55.47 +63 45 20.5 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
target,2461176.8930,11.19,0.05,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
target 20260516.3930 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 05 16.3930 2461176.8930 11.11 02:00:32.82 +59:40:06.6
131.56341 -2.04008 galactic Cas Second-epoch detections are separated by 3.2" and 5.0 pix
The object was found in VSX 3" ZTF J020033.07+594008.7
Type: SR
# Max. Min./Amp. JD0 Period
13.621 r Y 0.477 r 2458342.93970 344.838134100000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:32.82 +59:40:06.6: 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 02:00:32.82 +59:40:06.6: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 02 00 32.82 +59 40 06.6 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
ZTF J020033.07+594008.7,2461176.8930,11.11,0.05,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
ZTF J020033.07+594008.7 20260516.3930 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.07 01:52:55.26 +59:33:31.1
130.65661 -2.38783 galactic Cas Second-epoch detections are separated by 1.0" and 4.6 pix
The object was found in VSX17" Gaia DR3 506553498077188608
Type: ROT
# Max. Min./Amp. JD0 Period
15.360 G 15.380 G 2.474540000000 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 01:52:55.26 +59:33:31.1: 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 01:52:55.26 +59:33:31.1: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 52 55.26 +59 33 31.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506553498077188608,2461176.8930,11.07,0.05,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 506553498077188608 20260516.3930 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 05 16.3930 2461176.8930 11.11 01:42:17.61 +63:24:25.5
128.58689 1.09508 galactic Cas Second-epoch detections are separated by 1.5" 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 512081945620708864 | 01:42:22.23 +63:24:27.0 (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 01:42:17.61 +63:24:25.5: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:17.61 +63:24:25.5: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 05 16.3930* 01 42 17.61 +63 24 25.5 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 512081945620708864,2461176.8930,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512081945620708864 20260516.3930 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.19 01:36:51.84 +60:56:00.1
128.42333 -1.45313 galactic Cas Second-epoch detections are separated by 1.7" 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 509917110306382208 | 01:36:53.71 +60:55:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.245+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:51.84 +60:56:00.1: 12.23 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:51.84 +60:56:00.1: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 05 16.3930* 01 36 51.84 +60 56 00.1 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509917110306382208,2461176.8930,11.19,0.05,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
Gaia DR3 509917110306382208 20260516.3930 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 05 16.3930 2461176.8930 11.23 01:58:04.23 +59:07:28.4
131.40031 -2.64725 galactic Cas Second-epoch detections are separated by 8.5" and 5.2 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 | ATO J029.5360+59.1114 | 01:58:05.43 +59:06:51.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 1960IzKry..24..160B [B60] +58 592
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:04.23 +59:07:28.4: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:04.23 +59:07:28.4: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 58 04.23 +59 07 28.4 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
ATO J029.5360+59.1114,2461176.8930,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J029.5360+59.1114 20260516.3930 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.36 01:51:40.21 +60:56:16.1
130.18322 -1.08311 galactic Cas Second-epoch detections are separated by 2.5" 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 508195305151165312 | 01:51:34.71 +60:55:58.1 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.600+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:40.21 +60:56:16.1: 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 01:51:40.21 +60:56:16.1: 14.12 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 51 40.21 +60 56 16.1 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 508195305151165312,2461176.8930,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508195305151165312 20260516.3930 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.36 02:01:06.50 +64:35:47.8
130.31811 2.72865 galactic Cas Second-epoch detections are separated by 1.8" 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 | Gaia DR3 518077479449762560 | 02:01:07.64 +64:35:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.841+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:06.50 +64:35:47.8: 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 02:01:06.50 +64:35:47.8: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 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 05 16.3930* 02 01 06.50 +64 35 47.8 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
Gaia DR3 518077479449762560,2461176.8930,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518077479449762560 20260516.3930 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.34 01:54:30.03 +61:41:17.3
130.33577 -0.27374 galactic Cas Second-epoch detections are separated by 7.6" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 508336046943897984 | 01:54:27.53 +61:41:33.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1955ApJS....2..123F LF 5 +61 179
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:30.03 +61:41:17.3: 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 01:54:30.03 +61:41:17.3: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 54 30.03 +61 41 17.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508336046943897984,2461176.8930,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508336046943897984 20260516.3930 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 16.3930 2461176.8930 11.26 02:03:41.87 +58:47:26.2
132.18932 -2.77628 galactic Per Second-epoch detections are separated by 1.0" and 4.4 pix
The object was found in VSX 2" Gaia DR3 507016151955253248
Type: ROT
# Max. Min./Amp. JD0 Period
13.920 G 13.940 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:41.87 +58:47:26.2: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:41.87 +58:47:26.2: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 05 16.3930* 02 03 41.87 +58 47 26.2 11.3 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 507016151955253248,2461176.8930,11.26,0.05,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 507016151955253248 20260516.3930 11.26CV 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 05 16.3930 2461176.8930 11.83 01:39:27.12 +60:45:14.4
128.76583 -1.57274 galactic Cas Second-epoch detections are separated by 0.3" 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 | target | 01:39:27.12 +60:45:14.4 (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 01:39:27.12 +60:45:14.4: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:27.12 +60:45:14.4: 14.91 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 16.3930* 01 39 27.12 +60 45 14.4 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461176.8930,11.83,0.05,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
target 20260516.3930 11.83CV 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
## 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: 2461176.89327637 16.05.2026 09:26:09.078 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 20 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): 25672
Objects passed selection criteria: 25533
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: 18088.2
Average stars matched: 16584.5 (91.6866 %)
Memory usage VmPeak: 128288 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat May 16 08:22:49 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: 2461176.89327637 16.05.2026 09:26:09.078 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 207
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: 141 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): 186061
Objects passed selection criteria: 185601
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 139298
Average stars matched: 128117 (91.9728 %)
Memory usage VmPeak: 2000196 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat May 16 08:30:59 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.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: 2461176.89275073
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.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: 01:42:54.593 +61:59:00.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:54.593 +61:59:00.78
Angular distance between the image centers 0.0507 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
Image size: 938.8'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:54.964 +61:59:27.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:54.964 +61:59:27.60
Angular distance between the image centers 0.0517 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:54.593 +61:59:00.78
Second-epoch second image center 01:42:54.964 +61:59:27.60
Angular distance between the image centers 0.00749 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.jGCJ7xmbzw
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.6ZEbK0QWpu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits &> /tmp/tmp.r9sR7VdrU7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits &> /tmp/tmp.pgfrnjktXd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929150
a=0.000000 b=1.000000 c=22.929150
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.8)
Read 31681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.0659 to 45.7628 deg, Dec +55.3336 to +67.4023 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.0659 to 45.7628 deg, Dec 55.3336 to 67.4023 deg
Loaded 26179 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 14497 out of 16269 total matches.
Matched with Tycho-2 16269 out of 31681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.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
14.4 mag. fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
14.4 mag. fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jGCJ7xmbzw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 266 matched stars entering correct_measured_positions(), 9996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 337 matched stars entering correct_measured_positions(), 10041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.88"
Excluding outliers - 331 stars left (next iteration limit 292)
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.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6ZEbK0QWpu (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
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.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.r9sR7VdrU7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1283, passed=15922
Got 15922 stars (including 14627 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat
util/solve_plate_with_UCAC5 got 15922 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 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: 974 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 15605 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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 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(), 15608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 15608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 973 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_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits N_match=973 sigma_overall_arcsec=0.657 sigma_q1_arcsec=0.621 sigma_q2_arcsec=0.584 sigma_q3_arcsec=0.840 sigma_q4_arcsec=0.764 n_q1=265 n_q2=321 n_q3=225 n_q4=162 worst_quadrant_to_overall_ratio=1.278
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.pgfrnjktXd (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1312, passed=15907
Got 15907 stars (including 14588 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat
util/solve_plate_with_UCAC5 got 15907 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (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: 976 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 15612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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: 975 matched stars entering correct_measured_positions(), 15611 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 15611 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 975 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits N_match=975 sigma_overall_arcsec=0.681 sigma_q1_arcsec=0.598 sigma_q2_arcsec=0.641 sigma_q3_arcsec=0.718 sigma_q4_arcsec=0.740 n_q1=261 n_q2=322 n_q3=230 n_q4=162 worst_quadrant_to_overall_ratio=1.086
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=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_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits sigma_overall=0.657 worst_q_ratio=1.278
new2=fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits sigma_overall=0.681 worst_q_ratio=1.086
reference average sigma_overall=4.067 worst_q_ratio=2.6855
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: 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.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: 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.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295_astrometric_residuals.png (973 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296_astrometric_residuals.png (975 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:34.22 +62:59:14.3: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:34.22 +62:59:14.3: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter REJECTED candidate at 01:44:34.22 +62:59:14.3: ref_mag=12.12 +/- 0.01 new_mean_mag=12.0462 delta=0.08 (need > 0.90)
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 51606_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 51606_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:13:07.40 +58:04:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55227_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 55227_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:11:03.56 +57:20:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55709_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 55709_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 08339_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:20:32.59 +62:32:01.9 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_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits exists and is non-empty
wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.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: 01:42:54.593 +61:59:00.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:54.593 +61:59:00.78
Angular distance between the image centers 0.0507 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
Image size: 938.8'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:54.964 +61:59:27.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:54.964 +61:59:27.60
Angular distance between the image centers 0.0517 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:54.593 +61:59:00.78
Second-epoch second image center 01:42:54.964 +61:59:27.60
Angular distance between the image centers 0.00749 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.QC6j446vMA
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.za6EbsHV4n
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits &> /tmp/tmp.5JoQXUHWwf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits &> /tmp/tmp.sMcWYvcJyM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.035150
a=0.000000 b=1.000000 c=20.035150
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.76
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 222556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9526 to 45.5655 deg, Dec +55.3232 to +67.4437 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9526 to 45.5655 deg, Dec 55.3232 to 67.4437 deg
Loaded 26242 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 114 out of 143 total matches.
Matched with Tycho-2 143 out of 222556 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=4.4)
Read 218998 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 6.9707 to 45.8168 deg, Dec +55.3262 to +67.4140 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 6.9707 to 45.8168 deg, Dec 55.3262 to 67.4140 deg
Loaded 26295 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10859 out of 16691 total matches.
Matched with Tycho-2 16691 out of 218998 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 176 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_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
2.2 pix fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.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
11.7 mag. fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
11.8 mag. fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
All-image limiting magnitude estimate: 11.7 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QC6j446vMA (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=35398, passed=222522
Got 222522 stars (including 186791 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 222522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 275 matched stars entering correct_measured_positions(), 212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 264 matched stars entering correct_measured_positions(), 49591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 434 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 49636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.64"
Accuracy estimation diagnostic: 344 matched stars entering correct_measured_positions(), 64908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.78"
Excluding outliers - 344 stars left (next iteration limit 290)
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.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.za6EbsHV4n (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=35098, passed=218974
Got 218974 stars (including 183551 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 218974 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 209116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
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.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5JoQXUHWwf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=12292, passed=118145
Got 118145 stars (including 105721 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat
util/solve_plate_with_UCAC5 got 118145 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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 116384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 116385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 116300 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 969 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits N_match=969 sigma_overall_arcsec=0.666 sigma_q1_arcsec=0.569 sigma_q2_arcsec=0.581 sigma_q3_arcsec=0.831 sigma_q4_arcsec=0.700 n_q1=268 n_q2=322 n_q3=205 n_q4=174 worst_quadrant_to_overall_ratio=1.248
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.sMcWYvcJyM (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=12734, passed=120089
Got 120089 stars (including 107204 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat
util/solve_plate_with_UCAC5 got 120089 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 118427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 118427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 118427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 971 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits N_match=971 sigma_overall_arcsec=0.670 sigma_q1_arcsec=0.621 sigma_q2_arcsec=0.607 sigma_q3_arcsec=0.706 sigma_q4_arcsec=0.763 n_q1=270 n_q2=322 n_q3=206 n_q4=173 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-25-23_20.00sec_-0.00C_LIGHT_0295.fits
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-16_CI_Cas-03-Q2b1x1_062841_TTUQ2b1x1_3527350_BqSk9HAU/wcs_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296.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 01:49:53.19 +63:40:48.9: 12.16 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:27.79 +63:24:10.7: 12.83 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:01.08 +60:10:49.8: 12.56 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:23.59 +59:20:12.7: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:24.69 +58:01:36.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:09.06 +64:21:26.0: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:00.79 +59:33:43.7: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:33.02 +60:44:43.0: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:35.65 +63:20:53.0: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:36.33 +64:06:19.9: 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 01:37:23.59 +59:20:12.7: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Forced photometry filter KEPT candidate at 01:37:23.59 +59:20:12.7: ref_mag=14.00 +/- 0.05 new_mean_mag=11.2003 delta=2.80 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:53.19 +63:40:48.9: 13.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:09.06 +64:21:26.0: 13.71 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:00.79 +59:33:43.7: 14.20 +/- 0.07 detection
Forced photometry filter KEPT candidate at 01:49:53.19 +63:40:48.9: ref_mag=13.69 +/- 0.04 new_mean_mag=11.3589 delta=2.33 (need > 0.90)
Forced photometry reference-image weighted average: 13.71 +/- 0.05
Forced photometry filter KEPT candidate at 01:42:09.06 +64:21:26.0: ref_mag=13.71 +/- 0.05 new_mean_mag=11.2992 delta=2.41 (need > 0.90)
Forced photometry reference-image weighted average: 14.20 +/- 0.07
Forced photometry filter KEPT candidate at 01:25:00.79 +59:33:43.7: ref_mag=14.20 +/- 0.07 new_mean_mag=11.3889 delta=2.81 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:27.79 +63:24:10.7: 14.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Forced photometry filter KEPT candidate at 01:44:27.79 +63:24:10.7: ref_mag=14.00 +/- 0.05 new_mean_mag=11.3547 delta=2.65 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:35.65 +63:20:53.0: 14.43 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.07
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:01.08 +60:10:49.8: 13.98 +/- 0.06 detection
Forced photometry filter KEPT candidate at 01:20:35.65 +63:20:53.0: ref_mag=14.43 +/- 0.07 new_mean_mag=11.5411 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 01:22:33.02 +60:44:43.0: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.06
Forced photometry filter KEPT candidate at 01:30:01.08 +60:10:49.8: ref_mag=13.84 +/- 0.06 new_mean_mag=11.0763 delta=2.76 (need > 0.90)
Forced photometry reference-image weighted average: 14.13 +/- 0.06
Forced photometry filter KEPT candidate at 01:22:33.02 +60:44:43.0: ref_mag=14.13 +/- 0.06 new_mean_mag=11.2148 delta=2.91 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:36.33 +64:06:19.9: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.06
Forced photometry filter KEPT candidate at 01:46:36.33 +64:06:19.9: ref_mag=14.16 +/- 0.06 new_mean_mag=11.3956 delta=2.76 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:24.69 +58:01:36.0: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.05
Forced photometry filter KEPT candidate at 01:09:24.69 +58:01:36.0: ref_mag=13.65 +/- 0.05 new_mean_mag=11.0120 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 01:56:31.39 +58:17:39.4: 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 01:56:31.39 +58:17:39.4: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter KEPT candidate at 01:56:31.39 +58:17:39.4: ref_mag=13.68 +/- 0.04 new_mean_mag=10.9061 delta=2.77 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:36.00 +57:49:40.9: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:36.00 +57:49:40.9: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Forced photometry filter KEPT candidate at 01:17:36.00 +57:49:40.9: ref_mag=13.78 +/- 0.04 new_mean_mag=11.1643 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 01:24:54.87 +59:41:46.9: 12.93 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:10.42 +58:09:35.8: 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 01:24:54.87 +59:41:46.9: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry filter KEPT candidate at 01:24:54.87 +59:41:46.9: ref_mag=13.91 +/- 0.05 new_mean_mag=10.9956 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:10.42 +58:09:35.8: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Forced photometry filter KEPT candidate at 01:09:10.42 +58:09:35.8: ref_mag=13.92 +/- 0.05 new_mean_mag=10.9248 delta=2.99 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:27.53 +58:28:39.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:27.53 +58:28:39.1: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter KEPT candidate at 01:47:27.53 +58:28:39.1: ref_mag=13.81 +/- 0.04 new_mean_mag=11.0459 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 01:26:05.65 +59:01:14.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:21.61 +64:35:17.0: 12.82 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.65 +59:01:14.9: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.06
Forced photometry filter KEPT candidate at 01:26:05.65 +59:01:14.9: ref_mag=13.92 +/- 0.06 new_mean_mag=11.0664 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 01:43:27.18 +58:38:07.4: 12.75 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:21.61 +64:35:17.0: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry filter KEPT candidate at 01:09:21.61 +64:35:17.0: ref_mag=13.59 +/- 0.04 new_mean_mag=10.8971 delta=2.69 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:06.36 +59:00:32.7: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:27.18 +58:38:07.4: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry filter KEPT candidate at 01:43:27.18 +58:38:07.4: ref_mag=13.60 +/- 0.04 new_mean_mag=10.8429 delta=2.76 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:06.36 +59:00:32.7: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter KEPT candidate at 02:00:06.36 +59:00:32.7: ref_mag=13.49 +/- 0.03 new_mean_mag=11.0829 delta=2.40 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:13.06 +59:33:47.0: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:13.06 +59:33:47.0: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Forced photometry filter KEPT candidate at 01:06:13.06 +59:33:47.0: ref_mag=13.55 +/- 0.04 new_mean_mag=11.0393 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 01:54:45.35 +57:45:52.5: 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 01:54:45.35 +57:45:52.5: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Forced photometry filter KEPT candidate at 01:54:45.35 +57:45:52.5: ref_mag=13.69 +/- 0.05 new_mean_mag=10.9060 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 01:40:18.08 +61:21:06.8: 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 01:40:18.08 +61:21:06.8: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter KEPT candidate at 01:40:18.08 +61:21:06.8: ref_mag=13.81 +/- 0.04 new_mean_mag=10.9281 delta=2.88 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:11.63 +59:17:23.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:11.63 +59:17:23.8: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.05
Forced photometry filter KEPT candidate at 01:10:11.63 +59:17:23.8: ref_mag=13.78 +/- 0.05 new_mean_mag=10.9523 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 01:10:02.85 +57:48:13.3: 12.96 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:02.85 +57:48:13.3: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.06
Forced photometry filter KEPT candidate at 01:10:02.85 +57:48:13.3: ref_mag=13.86 +/- 0.06 new_mean_mag=11.0125 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 02:00:46.33 +57:54:00.7: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:46.33 +57:54:00.7: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Forced photometry filter KEPT candidate at 02:00:46.33 +57:54:00.7: ref_mag=13.80 +/- 0.05 new_mean_mag=10.9146 delta=2.89 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:25.53 +59:48:03.7: 12.47 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:59.62 +61:28:38.0: 13.02 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:25.53 +59:48:03.7: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry filter KEPT candidate at 01:08:25.53 +59:48:03.7: ref_mag=13.73 +/- 0.04 new_mean_mag=10.9840 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:59.62 +61:28:38.0: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter KEPT candidate at 01:06:59.62 +61:28:38.0: ref_mag=13.49 +/- 0.03 new_mean_mag=10.9456 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 02:07:25.37 +57:54:58.4: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:25.37 +57:54:58.4: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Forced photometry filter KEPT candidate at 02:07:25.37 +57:54:58.4: ref_mag=13.46 +/- 0.04 new_mean_mag=10.7735 delta=2.69 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.16 +59:59:18.2: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:47.02 +58:37:57.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:44.87 +57:55:09.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.16 +59:59:18.2: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter KEPT candidate at 01:07:39.16 +59:59:18.2: ref_mag=13.75 +/- 0.04 new_mean_mag=10.8356 delta=2.92 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:47.02 +58:37:57.5: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.07
Forced photometry filter KEPT candidate at 01:51:47.02 +58:37:57.5: ref_mag=13.89 +/- 0.07 new_mean_mag=10.9176 delta=2.97 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:44.87 +57:55:09.3: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Forced photometry filter KEPT candidate at 01:20:44.87 +57:55:09.3: ref_mag=13.34 +/- 0.03 new_mean_mag=10.6506 delta=2.69 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:45.72 +61:46:39.2: 12.53 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:45.72 +61:46:39.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Forced photometry filter KEPT candidate at 01:09:45.72 +61:46:39.2: ref_mag=13.06 +/- 0.03 new_mean_mag=10.7177 delta=2.34 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:38.62 +59:41:40.1: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:38.62 +59:41:40.1: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.04
Forced photometry filter KEPT candidate at 01:26:38.62 +59:41:40.1: ref_mag=13.42 +/- 0.04 new_mean_mag=10.7537 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 01:13:44.70 +57:24:51.1: 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 01:13:44.70 +57:24:51.1: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter KEPT candidate at 01:13:44.70 +57:24:51.1: ref_mag=13.48 +/- 0.03 new_mean_mag=10.6657 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 01:37:09.87 +58:51:06.9: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:09.87 +58:51:06.9: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry filter KEPT candidate at 01:37:09.87 +58:51:06.9: ref_mag=13.38 +/- 0.03 new_mean_mag=10.6226 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 01:33:10.34 +60:37:30.6: 7.58 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:10.34 +60:37:30.6: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 7.85 +/- 0.01
Forced photometry filter REJECTED candidate at 01:33:10.34 +60:37:30.6: ref_mag=7.85 +/- 0.01 new_mean_mag=10.5450 delta=-2.70 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:05:14.69 +63:02:38.1: 13.00 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:05:14.69 +63:02:38.1: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 02:05:14.69 +63:02:38.1: ref_mag=13.35 +/- 0.03 new_mean_mag=10.6458 delta=2.70 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:23.07 +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 01:31:23.07 +59:33:42.9: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter KEPT candidate at 01:31:23.07 +59:33:42.9: ref_mag=13.27 +/- 0.03 new_mean_mag=10.5485 delta=2.72 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:46.02 +58:12:06.9: 12.57 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:46.02 +58:12:06.9: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter KEPT candidate at 01:09:46.02 +58:12:06.9: ref_mag=13.12 +/- 0.03 new_mean_mag=10.3868 delta=2.73 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:55.22 +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 01:46:55.22 +59:54:51.7: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 01:46:55.22 +59:54:51.7: ref_mag=12.67 +/- 0.01 new_mean_mag=10.1406 delta=2.53 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:53:47.13 +60:15:59.7: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:53:47.13 +60:15:59.7: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter KEPT candidate at 01:53:47.13 +60:15:59.7: ref_mag=12.54 +/- 0.01 new_mean_mag=9.9325 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 01:20:24.33 +59:10:24.8: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:43.82 +60:47:34.5: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:24.33 +59:10:24.8: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:43.82 +60:47:34.5: 12.14 +/- 0.01 detection
Forced photometry filter KEPT candidate at 01:20:24.33 +59:10:24.8: ref_mag=12.31 +/- 0.01 new_mean_mag=9.6117 delta=2.70 (need > 0.90)
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter KEPT candidate at 01:30:43.82 +60:47:34.5: ref_mag=12.14 +/- 0.01 new_mean_mag=9.5334 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 01:09:00.88 +60:12:40.3: 9.42 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:27.99 +58:11:23.3: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:00.88 +60:12:40.3: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.04 +/- 0.01
Forced photometry filter REJECTED candidate at 01:09:00.88 +60:12:40.3: ref_mag=10.04 +/- 0.01 new_mean_mag=10.4153 delta=-0.37 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:27.99 +58:11:23.3: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Forced photometry filter KEPT candidate at 01:18:27.99 +58:11:23.3: ref_mag=13.11 +/- 0.03 new_mean_mag=10.4072 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 01:09:09.36 +61:37:28.7: 13.09 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:09.36 +61:37:28.7: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter KEPT candidate at 01:09:09.36 +61:37:28.7: ref_mag=13.33 +/- 0.03 new_mean_mag=10.6514 delta=2.68 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.40 +60:07:33.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.40 +60:07:33.6: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.04
Forced photometry filter KEPT candidate at 01:46:38.40 +60:07:33.6: ref_mag=13.40 +/- 0.04 new_mean_mag=10.5174 delta=2.88 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:05.36 +57:15:17.9: 10.10 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:05.36 +57:15:17.9: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.01 +/- 0.02
Forced photometry filter REJECTED candidate at 01:09:05.36 +57:15:17.9: ref_mag=11.01 +/- 0.02 new_mean_mag=10.5152 delta=0.50 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:04:00.85 +58:29:06.4: 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 02:04:00.85 +58:29:06.4: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.05
Forced photometry filter KEPT candidate at 02:04:00.85 +58:29:06.4: ref_mag=13.81 +/- 0.05 new_mean_mag=10.8450 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 01:39:36.32 +60:53:52.2: 9.82 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:36.32 +60:53:52.2: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 10.99 +/- 0.03
Forced photometry filter REJECTED candidate at 01:39:36.32 +60:53:52.2: ref_mag=10.99 +/- 0.03 new_mean_mag=10.8306 delta=0.16 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:35.78 +59:32:43.9: 12.77 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:35.78 +59:32:43.9: 14.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.07
Forced photometry filter KEPT candidate at 01:24:35.78 +59:32:43.9: ref_mag=13.98 +/- 0.07 new_mean_mag=10.9447 delta=3.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:33.90 +63:37:10.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:05.50 +59:57:20.8: 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 01:59:33.90 +63:37:10.1: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Forced photometry filter KEPT candidate at 01:59:33.90 +63:37:10.1: ref_mag=13.92 +/- 0.05 new_mean_mag=10.9782 delta=2.94 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:05.50 +59:57:20.8: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Forced photometry filter KEPT candidate at 01:56:05.50 +59:57:20.8: ref_mag=13.77 +/- 0.04 new_mean_mag=10.8142 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 01:44:03.15 +61:54:45.7: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:32.65 +62:45:43.1: 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 01:44:03.15 +61:54:45.7: 13.95 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.12
Forced photometry filter KEPT candidate at 01:44:03.15 +61:54:45.7: ref_mag=13.95 +/- 0.12 new_mean_mag=10.9104 delta=3.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:32.65 +62:45:43.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Forced photometry filter KEPT candidate at 02:20:32.65 +62:45:43.1: ref_mag=13.95 +/- 0.05 new_mean_mag=10.9930 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 01:22:11.00 +59:09:03.3: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:11.00 +59:09:03.3: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.05
Forced photometry filter KEPT candidate at 01:22:11.00 +59:09:03.3: ref_mag=13.74 +/- 0.05 new_mean_mag=10.8859 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 01:41:34.20 +59:13:56.8: 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 01:41:34.20 +59:13:56.8: 14.08 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.07
Forced photometry filter KEPT candidate at 01:41:34.20 +59:13:56.8: ref_mag=14.08 +/- 0.07 new_mean_mag=11.0663 delta=3.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.61 +57:26:30.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.61 +57:26:30.6: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Forced photometry filter KEPT candidate at 01:09:22.61 +57:26:30.6: ref_mag=13.90 +/- 0.05 new_mean_mag=10.9854 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 01:21:55.47 +63:45:20.5: 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 01:21:55.47 +63:45:20.5: 14.29 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.07
Forced photometry filter KEPT candidate at 01:21:55.47 +63:45:20.5: ref_mag=14.29 +/- 0.07 new_mean_mag=11.1668 delta=3.13 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:32.82 +59:40:06.6: 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 02:00:32.82 +59:40:06.6: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.05
Forced photometry filter KEPT candidate at 02:00:32.82 +59:40:06.6: ref_mag=12.84 +/- 0.05 new_mean_mag=11.1099 delta=1.73 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:55.26 +59:33:31.1: 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 01:52:55.26 +59:33:31.1: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.07
Forced photometry filter KEPT candidate at 01:52:55.26 +59:33:31.1: ref_mag=14.06 +/- 0.07 new_mean_mag=11.0671 delta=2.99 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:17.61 +63:24:25.5: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:17.61 +63:24:25.5: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.06
Forced photometry filter KEPT candidate at 01:42:17.61 +63:24:25.5: ref_mag=14.03 +/- 0.06 new_mean_mag=11.1061 delta=2.93 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:51.84 +60:56:00.1: 12.23 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:51.84 +60:56:00.1: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.06
Forced photometry filter KEPT candidate at 01:36:51.84 +60:56:00.1: ref_mag=13.78 +/- 0.06 new_mean_mag=11.1834 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 01:58:04.23 +59:07:28.4: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:04.23 +59:07:28.4: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry filter KEPT candidate at 01:58:04.23 +59:07:28.4: ref_mag=13.91 +/- 0.05 new_mean_mag=11.2327 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 01:51:40.21 +60:56:16.1: 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 01:51:40.21 +60:56:16.1: 14.12 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.07
Forced photometry filter KEPT candidate at 01:51:40.21 +60:56:16.1: ref_mag=14.12 +/- 0.07 new_mean_mag=11.3495 delta=2.77 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:06.50 +64:35:47.8: 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 02:01:06.50 +64:35:47.8: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.06
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:30.03 +61:41:17.3: 13.29 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 02:01:06.50 +64:35:47.8: ref_mag=14.18 +/- 0.06 new_mean_mag=11.3555 delta=2.82 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:30.03 +61:41:17.3: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Forced photometry filter KEPT candidate at 01:54:30.03 +61:41:17.3: ref_mag=13.83 +/- 0.04 new_mean_mag=11.3368 delta=2.50 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:50.89 +61:52:51.1: 11.37 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:50.89 +61:52:51.1: 14.64 +/- 0.29 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.15
Forced photometry filter REJECTED candidate at 01:43:50.89 +61:52:51.1: ref_mag=12.23 +/- 0.15 new_mean_mag=11.4817 delta=0.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:41.87 +58:47:26.2: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:41.87 +58:47:26.2: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.06
Forced photometry filter KEPT candidate at 02:03:41.87 +58:47:26.2: ref_mag=13.95 +/- 0.06 new_mean_mag=11.2116 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:29.98 +60:37:07.2: 10.44 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:29.98 +60:37:07.2: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.02
Forced photometry filter REJECTED candidate at 01:44:29.98 +60:37:07.2: ref_mag=10.91 +/- 0.02 new_mean_mag=11.4776 delta=-0.57 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:27.12 +60:45:14.4: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:27.12 +60:45:14.4: 14.91 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.16
Forced photometry filter KEPT candidate at 01:39:27.12 +60:45:14.4: ref_mag=14.91 +/- 0.16 new_mean_mag=11.8328 delta=3.07 (need > 0.90)
Adding exclusion_list_local.txt__out247639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247719.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__out247728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247737.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__out247744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out261562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out265769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out266889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out267634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out268607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out269902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out271600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out272215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out272469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out272844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out274036.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 115s
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: 48s
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Considering the candidate 247639_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247639_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247640_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247640_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247645_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247645_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247651_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247651_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247658_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247658_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247663_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247663_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247672_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247672_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247675_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247675_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247684_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247684_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247685_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247685_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247686_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247686_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247688_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247688_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247689_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247689_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247692_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247692_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247696_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247696_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247707_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247707_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:30:06.49 +61:51:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247708_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247708_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:50:44.74 +58:00:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247719_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247719_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247722_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247722_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247724_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247724_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247726_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247726_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247728_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247728_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247732_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247732_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247733_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247733_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247734_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247734_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247736_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247736_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247737_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247737_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247739_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247739_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:14:01.35 +57:40:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247740_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247740_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247741_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247741_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247742_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247742_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247744_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247744_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247746_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247746_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247749_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247749_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247756_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247756_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:58:54.89 +58:10:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247757_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247757_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247758_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247758_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247762_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247762_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:39:24.01 +58:23:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247769_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247769_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
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Considering the candidate 247771_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247771_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247775_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247775_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:07:34.95 +57:33:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247778_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247778_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247782_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247782_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247785_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247785_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:19:23.96 +58:26:39.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247788_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247788_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247790_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247790_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247794_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247794_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:10:37.48 +57:22:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247795_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247795_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:25:15.33 +64:40:35.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247796_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247796_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:07:34.10 +60:52:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247799_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247799_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:03:21.60 +57:48:47.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247802_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247802_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:14:45.30 +60:30:05.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247803_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247803_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247807_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247807_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:07:07.92 +57:44:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247809_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247809_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247811_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247811_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:43:59.06 +61:55:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247814_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247814_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:55:14.53 +59:32:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247817_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247817_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:15:16.77 +57:28:05.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247818_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247818_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247819_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 247819_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247829_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247829_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:13:07.21 +58:04:49.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247831_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 247831_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:32:40.10 +63:11:28.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251458_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 251458_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:44:01.94 +61:53:56.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252494_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 252494_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:38:00.39 +57:56:45.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253373_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 253373_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:19:11.01 +58:20:30.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253456_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 253456_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:26:41.04 +60:46:46.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 255374_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 255374_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:58:16.26 +59:38:59.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256586_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 256586_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:46:33.52 +61:16:46.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 256850_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 256850_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:43:53.07 +61:53:16.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257172_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 257172_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:20:10.89 +58:12:10.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257582_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 257582_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:44:17.59 +61:53:15.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258212_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 258212_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:16:08.69 +58:49:39.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258222_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 258222_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:19:12.23 +65:35:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258274_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 258274_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:29:33.89 +63:19:25.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258353_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 258353_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:15:58.90 +63:12:26.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258436_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 258436_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:11:22.90 +61:21:06.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258818_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 258818_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:44:32.26 +58:45:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 258903_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 258903_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:04:26.63 +65:05:52.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259639_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 259639_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:02:54.73 +64:24:59.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 259791_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 259791_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:00:36.70 +58:30:23.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260331_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 260331_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:16:05.04 +58:49:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260610_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 260610_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:33:23.07 +57:44:23.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260680_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 260680_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:35:50.51 +61:27:35.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 260761_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 260761_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:16:36.14 +64:57:47.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261096_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 261096_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:13:30.14 +58:34:25.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261266_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 261266_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:11:50.45 +59:02:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261363_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 261363_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261436_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 261436_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:02:54.01 +60:15:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261562_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 261562_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261824_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 261824_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:19:03.73 +63:57:43.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261830_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 261830_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:13:35.95 +57:52:31.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 261999_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 261999_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:16:02.28 +58:49:59.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262033_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 262033_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:52:48.68 +60:28:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262055_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 262055_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:06:23.58 +62:44:06.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262083_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 262083_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:54:19.06 +63:38:05.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262092_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 262092_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262114_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 262114_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:10:23.82 +60:01:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262637_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 262637_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:43:06.92 +58:57:28.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262722_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 262722_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:58:04.17 +57:58:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262909_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 262909_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:31:32.54 +61:02:20.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263115_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 263115_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263206_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 263206_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:44:56.49 +59:46:24.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263282_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 263282_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:10:32.85 +59:59:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263411_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 263411_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263567_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 263567_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:26:35.99 +57:57:39.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263652_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 263652_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:01:36.87 +59:57:23.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263851_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 263851_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:37:13.49 +58:38:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263853_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 263853_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:01:15.10 +59:23:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263878_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 263878_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:42:28.03 +58:17:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263946_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 263946_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:38:33.73 +60:47:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264003_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 264003_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:06:45.41 +59:50:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264038_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 264038_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:17:21.64 +59:22:32.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264197_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 264197_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:16:24.31 +58:04:08.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264283_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 264283_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:44:32.23 +61:36:39.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264483_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 264483_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:37:13.11 +58:38:19.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264548_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 264548_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:16:02.44 +60:36:57.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264872_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 264872_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:54:30.29 +59:06:33.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265052_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265052_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:16:36.97 +64:56:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265131_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265131_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:10:10.12 +59:08:09.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265275_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265275_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:38:06.37 +58:10:42.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265500_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265500_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:48:39.79 +59:09:18.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265529_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265529_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:54:34.65 +59:52:43.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265560_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265560_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:55:21.56 +59:25:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265655_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265655_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:43:12.73 +64:00:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265675_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265675_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:14:00.29 +61:42:02.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265676_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265676_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:38:12.02 +61:01:26.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265769_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 265769_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265795_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265795_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:46:18.32 +60:59:19.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265870_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265870_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265893_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265893_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:14:58.44 +60:30:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265990_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 265990_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:58:04.82 +59:36:38.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266030_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 266030_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:42:55.10 +64:01:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266294_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 266294_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:08:30.46 +58:24:16.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266318_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 266318_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266328_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 266328_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:59:05.89 +59:55:34.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266497_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 266497_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:18:04.19 +65:36:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266730_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 266730_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:27:56.37 +62:46:06.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266855_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 266855_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:43:03.24 +58:57:13.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266889_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 266889_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267305_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 267305_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267492_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 267492_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267634_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 267634_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267775_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 267775_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:03:25.08 +57:50:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267797_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 267797_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:34:42.60 +58:42:16.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268036_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 268036_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268127_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 268127_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:17:01.85 +63:21:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268144_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 268144_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268202_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 268202_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:15:05.46 +64:08:42.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268226_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 268226_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:14:00.50 +59:02:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268275_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 268275_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:27:03.92 +64:43:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268607_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 268607_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269061_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 269061_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:48:34.98 +58:41:31.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269063_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 269063_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:09:18.16 +58:38:30.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269087_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 269087_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269264_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 269264_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269438_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 269438_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:56:25.33 +62:05:30.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269827_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 269827_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 269902_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 269902_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270439_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 270439_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:56:05.61 +60:57:15.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270457_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 270457_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 270808_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 270808_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:54:06.29 +61:05:12.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271348_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 271348_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271600_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 271600_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272215_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 272215_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272469_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 272469_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272540_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 272540_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272563_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 272563_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:47:18.55 +58:31:59.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272844_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 272844_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273559_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 273559_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 274000_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 274000_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 274036_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
Preparing report for the candidate 274036_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153703_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 153703_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:18:22.40 +58:47:11.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 112593_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:21:55.01 +61:20:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 70271_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:20:32.54 +62:32:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 72532_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:45:35.17 +63:07:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 76113_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 02:02:02.11 +62:41:32.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296
The candidate 39378_fd_Cas-03-Q2b1x1_2026-05-16_04-26-09_20.00sec_-0.00C_LIGHT_0296 did not pass the final checks
**** FOUND 01:47:55.49 +64:32:55.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 167s
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 ####
01:25:00.79 +59:33:43.7
01:20:35.65 +63:20:53.0
01:44:27.79 +63:24:10.7
01:49:53.19 +63:40:48.9
01:46:36.33 +64:06:19.9
01:37:23.59 +59:20:12.7
01:09:24.69 +58:01:36.0
01:22:33.02 +60:44:43.0
01:30:01.08 +60:10:49.8
01:42:09.06 +64:21:26.0
01:56:31.39 +58:17:39.4
01:17:36.00 +57:49:40.9
01:24:54.87 +59:41:46.9
01:09:10.42 +58:09:35.8
01:47:27.53 +58:28:39.1
01:26:05.65 +59:01:14.9
01:09:21.61 +64:35:17.0
01:43:27.18 +58:38:07.4
02:00:06.36 +59:00:32.7
01:06:13.06 +59:33:47.0
01:54:45.35 +57:45:52.5
01:40:18.08 +61:21:06.8
01:10:11.63 +59:17:23.8
01:10:02.85 +57:48:13.3
02:00:46.33 +57:54:00.7
01:08:25.53 +59:48:03.7
01:06:59.62 +61:28:38.0
02:07:25.37 +57:54:58.4
01:07:39.16 +59:59:18.2
01:51:47.02 +58:37:57.5
01:20:44.87 +57:55:09.3
01:09:45.72 +61:46:39.2
01:26:38.62 +59:41:40.1
01:13:44.70 +57:24:51.1
01:37:09.87 +58:51:06.9
02:05:14.69 +63:02:38.1
01:31:23.07 +59:33:42.9
01:09:46.02 +58:12:06.9
01:46:55.22 +59:54:51.7
01:53:47.13 +60:15:59.7
01:20:24.33 +59:10:24.8
01:30:43.82 +60:47:34.5
01:18:27.99 +58:11:23.3
01:09:09.36 +61:37:28.7
01:46:38.40 +60:07:33.6
02:04:00.85 +58:29:06.4
01:24:35.78 +59:32:43.9
01:59:33.90 +63:37:10.1
01:56:05.50 +59:57:20.8
01:44:03.15 +61:54:45.7
02:20:32.65 +62:45:43.1
01:22:11.00 +59:09:03.3
01:41:34.20 +59:13:56.8
01:09:22.61 +57:26:30.6
01:21:55.47 +63:45:20.5
02:00:32.82 +59:40:06.6
01:52:55.26 +59:33:31.1
01:42:17.61 +63:24:25.5
01:36:51.84 +60:56:00.1
01:58:04.23 +59:07:28.4
01:51:40.21 +60:56:16.1
02:01:06.50 +64:35:47.8
01:54:30.03 +61:41:17.3
02:03:41.87 +58:47:26.2
01:39:27.12 +60:45:14.4
########### Completed Cas-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:25:00.79 +59:33:43.7
01:20:35.65 +63:20:53.0
01:44:27.79 +63:24:10.7
01:49:53.19 +63:40:48.9
01:46:36.33 +64:06:19.9
01:37:23.59 +59:20:12.7
01:09:24.69 +58:01:36.0
01:22:33.02 +60:44:43.0
01:30:01.08 +60:10:49.8
01:42:09.06 +64:21:26.0
01:56:31.39 +58:17:39.4
01:17:36.00 +57:49:40.9
01:24:54.87 +59:41:46.9
01:09:10.42 +58:09:35.8
01:47:27.53 +58:28:39.1
01:26:05.65 +59:01:14.9
01:09:21.61 +64:35:17.0
01:43:27.18 +58:38:07.4
02:00:06.36 +59:00:32.7
01:06:13.06 +59:33:47.0
01:54:45.35 +57:45:52.5
01:40:18.08 +61:21:06.8
01:10:11.63 +59:17:23.8
01:10:02.85 +57:48:13.3
02:00:46.33 +57:54:00.7
01:08:25.53 +59:48:03.7
01:06:59.62 +61:28:38.0
02:07:25.37 +57:54:58.4
01:07:39.16 +59:59:18.2
01:51:47.02 +58:37:57.5
01:20:44.87 +57:55:09.3
01:09:45.72 +61:46:39.2
01:26:38.62 +59:41:40.1
01:13:44.70 +57:24:51.1
01:37:09.87 +58:51:06.9
02:05:14.69 +63:02:38.1
01:31:23.07 +59:33:42.9
01:09:46.02 +58:12:06.9
01:46:55.22 +59:54:51.7
01:53:47.13 +60:15:59.7
01:20:24.33 +59:10:24.8
01:30:43.82 +60:47:34.5
01:18:27.99 +58:11:23.3
01:09:09.36 +61:37:28.7
01:46:38.40 +60:07:33.6
02:04:00.85 +58:29:06.4
01:24:35.78 +59:32:43.9
01:59:33.90 +63:37:10.1
01:56:05.50 +59:57:20.8
01:44:03.15 +61:54:45.7
02:20:32.65 +62:45:43.1
01:22:11.00 +59:09:03.3
01:41:34.20 +59:13:56.8
01:09:22.61 +57:26:30.6
01:21:55.47 +63:45:20.5
02:00:32.82 +59:40:06.6
01:52:55.26 +59:33:31.1
01:42:17.61 +63:24:25.5
01:36:51.84 +60:56:00.1
01:58:04.23 +59:07:28.4
01:51:40.21 +60:56:16.1
02:01:06.50 +64:35:47.8
01:54:30.03 +61:41:17.3
02:03:41.87 +58:47:26.2
01:39:27.12 +60:45:14.4
###################################################################################
01:25:00.79 +59:33:43.7 -- not an asteroid (will add it to exclusion list)
01:20:35.65 +63:20:53.0 -- not an asteroid (will add it to exclusion list)
01:44:27.79 +63:24:10.7 -- not an asteroid (will add it to exclusion list)
01:49:53.19 +63:40:48.9 -- not an asteroid (will add it to exclusion list)
01:46:36.33 +64:06:19.9 -- not an asteroid (will add it to exclusion list)
01:37:23.59 +59:20:12.7 -- not an asteroid (will add it to exclusion list)
01:09:24.69 +58:01:36.0 -- not an asteroid (will add it to exclusion list)
01:22:33.02 +60:44:43.0 -- not an asteroid (will add it to exclusion list)
01:30:01.08 +60:10:49.8 -- not an asteroid (will add it to exclusion list)
01:42:09.06 +64:21:26.0 -- not an asteroid (will add it to exclusion list)
01:56:31.39 +58:17:39.4 -- not an asteroid (will add it to exclusion list)
01:17:36.00 +57:49:40.9 -- not an asteroid (will add it to exclusion list)
01:24:54.87 +59:41:46.9 -- not an asteroid (will add it to exclusion list)
01:09:10.42 +58:09:35.8 -- not an asteroid (will add it to exclusion list)
01:47:27.53 +58:28:39.1 -- not an asteroid (will add it to exclusion list)
01:26:05.65 +59:01:14.9 -- not an asteroid (will add it to exclusion list)
01:09:21.61 +64:35:17.0 -- not an asteroid (will add it to exclusion list)
01:43:27.18 +58:38:07.4 -- not an asteroid (will add it to exclusion list)
02:00:06.36 +59:00:32.7 -- not an asteroid (will add it to exclusion list)
01:06:13.06 +59:33:47.0 -- not an asteroid (will add it to exclusion list)
01:54:45.35 +57:45:52.5 -- not an asteroid (will add it to exclusion list)
01:40:18.08 +61:21:06.8 -- not an asteroid (will add it to exclusion list)
01:10:11.63 +59:17:23.8 -- not an asteroid (will add it to exclusion list)
01:10:02.85 +57:48:13.3 -- not an asteroid (will add it to exclusion list)
02:00:46.33 +57:54:00.7 -- not an asteroid (will add it to exclusion list)
01:08:25.53 +59:48:03.7 -- not an asteroid (will add it to exclusion list)
01:06:59.62 +61:28:38.0 -- not an asteroid (will add it to exclusion list)
02:07:25.37 +57:54:58.4 -- not an asteroid (will add it to exclusion list)
01:07:39.16 +59:59:18.2 -- not an asteroid (will add it to exclusion list)
01:51:47.02 +58:37:57.5 -- not an asteroid (will add it to exclusion list)
01:20:44.87 +57:55:09.3 -- not an asteroid (will add it to exclusion list)
01:09:45.72 +61:46:39.2 -- not an asteroid (will add it to exclusion list)
01:26:38.62 +59:41:40.1 -- not an asteroid (will add it to exclusion list)
01:13:44.70 +57:24:51.1 -- not an asteroid (will add it to exclusion list)
01:37:09.87 +58:51:06.9 -- not an asteroid (will add it to exclusion list)
02:05:14.69 +63:02:38.1 -- not an asteroid (will add it to exclusion list)
01:31:23.07 +59:33:42.9 -- not an asteroid (will add it to exclusion list)
01:09:46.02 +58:12:06.9 -- not an asteroid (will add it to exclusion list)
01:46:55.22 +59:54:51.7 -- not an asteroid (will add it to exclusion list)
01:53:47.13 +60:15:59.7 -- not an asteroid (will add it to exclusion list)
01:20:24.33 +59:10:24.8 -- not an asteroid (will add it to exclusion list)
01:30:43.82 +60:47:34.5 -- not an asteroid (will add it to exclusion list)
01:18:27.99 +58:11:23.3 -- not an asteroid (will add it to exclusion list)
01:09:09.36 +61:37:28.7 -- not an asteroid (will add it to exclusion list)
01:46:38.40 +60:07:33.6 -- not an asteroid (will add it to exclusion list)
02:04:00.85 +58:29:06.4 -- not an asteroid (will add it to exclusion list)
01:24:35.78 +59:32:43.9 -- not an asteroid (will add it to exclusion list)
01:59:33.90 +63:37:10.1 -- not an asteroid (will add it to exclusion list)
01:56:05.50 +59:57:20.8 -- not an asteroid (will add it to exclusion list)
01:44:03.15 +61:54:45.7 -- not an asteroid (will add it to exclusion list)
02:20:32.65 +62:45:43.1 -- not an asteroid (will add it to exclusion list)
01:22:11.00 +59:09:03.3 -- not an asteroid (will add it to exclusion list)
01:41:34.20 +59:13:56.8 -- not an asteroid (will add it to exclusion list)
01:09:22.61 +57:26:30.6 -- not an asteroid (will add it to exclusion list)
01:21:55.47 +63:45:20.5 -- not an asteroid (will add it to exclusion list)
02:00:32.82 +59:40:06.6 -- not an asteroid (will add it to exclusion list)
01:52:55.26 +59:33:31.1 -- not an asteroid (will add it to exclusion list)
01:42:17.61 +63:24:25.5 -- not an asteroid (will add it to exclusion list)
01:36:51.84 +60:56:00.1 -- not an asteroid (will add it to exclusion list)
01:58:04.23 +59:07:28.4 -- not an asteroid (will add it to exclusion list)
01:51:40.21 +60:56:16.1 -- not an asteroid (will add it to exclusion list)
02:01:06.50 +64:35:47.8 -- not an asteroid (will add it to exclusion list)
01:54:30.03 +61:41:17.3 -- not an asteroid (will add it to exclusion list)
02:03:41.87 +58:47:26.2 -- not an asteroid (will add it to exclusion list)
01:39:27.12 +60:45:14.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:06:13.06 +59:33:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:59.62 +61:28:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.16 +59:59:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:25.53 +59:48:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:09.36 +61:37:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:10.42 +58:09:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:21.61 +64:35:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.61 +57:26:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:24.69 +58:01:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:45.72 +61:46:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:46.02 +58:12:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:02.85 +57:48:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:11.63 +59:17:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:44.70 +57:24:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:36.00 +57:49:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:27.99 +58:11:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:24.33 +59:10:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:35.65 +63:20:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:44.87 +57:55:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:55.47 +63:45:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:11.00 +59:09:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:33.02 +60:44:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:35.78 +59:32:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:54.87 +59:41:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:00.79 +59:33:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.65 +59:01:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:38.62 +59:41:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:01.08 +60:10:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:43.82 +60:47:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:23.07 +59:33:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:51.84 +60:56:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:09.87 +58:51:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:23.59 +59:20:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:27.12 +60:45:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:18.08 +61:21:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:34.20 +59:13:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:09.06 +64:21:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:17.61 +63:24:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:27.18 +58:38:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:03.15 +61:54:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:27.79 +63:24:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:36.33 +64:06:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.40 +60:07:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:55.22 +59:54:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:27.53 +58:28:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:53.19 +63:40:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:40.21 +60:56:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:47.02 +58:37:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:55.26 +59:33:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:47.13 +60:15:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:30.03 +61:41:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:45.35 +57:45:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:05.50 +59:57:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:31.39 +58:17:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:04.23 +59:07:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:33.90 +63:37:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:06.36 +59:00:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:32.82 +59:40:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:46.33 +57:54:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:06.50 +64:35:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:41.87 +58:47:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:00.85 +58:29:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:14.69 +63:02:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:25.37 +57:54:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:32.65 +62:45:43.1 -- 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)
01:06:13.06 +59:33:47.0 -- not a known variable star
01:06:59.62 +61:28:38.0 -- a known variable star
01:07:39.16 +59:59:18.2 -- not a known variable star
01:08:25.53 +59:48:03.7 -- not a known variable star
01:09:09.36 +61:37:28.7 -- a known variable star
01:09:10.42 +58:09:35.8 -- not a known variable star
01:09:21.61 +64:35:17.0 -- not a known variable star
01:09:22.61 +57:26:30.6 -- not a known variable star
01:09:24.69 +58:01:36.0 -- not a known variable star
01:09:45.72 +61:46:39.2 -- not a known variable star
01:09:46.02 +58:12:06.9 -- not a known variable star
01:10:02.85 +57:48:13.3 -- not a known variable star
01:10:11.63 +59:17:23.8 -- not a known variable star
01:13:44.70 +57:24:51.1 -- not a known variable star
01:17:36.00 +57:49:40.9 -- not a known variable star
01:18:27.99 +58:11:23.3 -- not a known variable star
01:20:24.33 +59:10:24.8 -- not a known variable star
01:20:35.65 +63:20:53.0 -- not a known variable star
01:20:44.87 +57:55:09.3 -- not a known variable star
01:21:55.47 +63:45:20.5 -- not a known variable star
01:22:11.00 +59:09:03.3 -- not a known variable star
01:22:33.02 +60:44:43.0 -- not a known variable star
01:24:35.78 +59:32:43.9 -- a known variable star
01:24:54.87 +59:41:46.9 -- not a known variable star
01:25:00.79 +59:33:43.7 -- not a known variable star
01:26:05.65 +59:01:14.9 -- not a known variable star
01:26:38.62 +59:41:40.1 -- a known variable star
01:30:01.08 +60:10:49.8 -- a known variable star
01:30:43.82 +60:47:34.5 -- a known variable star
01:31:23.07 +59:33:42.9 -- not a known variable star
01:36:51.84 +60:56:00.1 -- not a known variable star
01:37:09.87 +58:51:06.9 -- a known variable star
01:37:23.59 +59:20:12.7 -- not a known variable star
01:39:27.12 +60:45:14.4 -- not a known variable star
01:40:18.08 +61:21:06.8 -- not a known variable star
01:41:34.20 +59:13:56.8 -- not a known variable star
01:42:09.06 +64:21:26.0 -- not a known variable star
01:42:17.61 +63:24:25.5 -- not a known variable star
01:43:27.18 +58:38:07.4 -- a known variable star
01:44:03.15 +61:54:45.7 -- not a known variable star
01:44:27.79 +63:24:10.7 -- not a known variable star
01:46:36.33 +64:06:19.9 -- not a known variable star
01:46:38.40 +60:07:33.6 -- not a known variable star
01:46:55.22 +59:54:51.7 -- not a known variable star
01:47:27.53 +58:28:39.1 -- not a known variable star
01:49:53.19 +63:40:48.9 -- not a known variable star
01:51:40.21 +60:56:16.1 -- not a known variable star
01:51:47.02 +58:37:57.5 -- not a known variable star
01:52:55.26 +59:33:31.1 -- a known variable star
01:53:47.13 +60:15:59.7 -- not a known variable star
01:54:30.03 +61:41:17.3 -- not a known variable star
01:54:45.35 +57:45:52.5 -- a known variable star
01:56:05.50 +59:57:20.8 -- not a known variable star
01:56:31.39 +58:17:39.4 -- not a known variable star
01:58:04.23 +59:07:28.4 -- not a known variable star
01:59:33.90 +63:37:10.1 -- not a known variable star
02:00:06.36 +59:00:32.7 -- not a known variable star
02:00:32.82 +59:40:06.6 -- a known variable star
02:00:46.33 +57:54:00.7 -- not a known variable star
02:01:06.50 +64:35:47.8 -- not a known variable star
02:03:41.87 +58:47:26.2 -- a known variable star
02:04:00.85 +58:29:06.4 -- not a known variable star
02:05:14.69 +63:02:38.1 -- a known variable star
02:07:25.37 +57:54:58.4 -- not a known variable star
02:20:32.65 +62:45:43.1 -- a known variable star
Found 51 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
65 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 65 (excluding asteroids and hot pixels, 51 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)2461176.89275073 -observatory V36
03:39:50.89 +20:00:50.4 Mercury (-2.2mag)
05:44:22.45 +24:53:49.0 Venus (-3.9mag)
01:44:03.27 +09:56:26.8 Mars (1.2mag)
07:30:42.04 +22:12:19.5 Jupiter (-1.9mag)
00:41:47.78 +02:05:33.2 Saturn (0.9mag)
03:54:41.28 +20:09:12.1 Uranus (5.8mag)
00:14:21.30 +00:06:21.4 Neptune (7.8mag)
20:34:10.79 -22:57:16.5 Pluto (14.5mag)
03:02:41.62 +21:20:05.2 Moon (-8.3mag)
-rw-r--r-- 1 apache apache 362 May 16 08:22 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461176.89275073:
07:30:47.89 +22:12:06.5 Io (5.9mag)
07:30:37.33 +22:12:29.9 Europa (6.1mag)
07:30:36.24 +22:12:28.7 Ganymede (5.5mag)
07:30:53.11 +22:11:59.6 Callisto (6.7mag)
07:32:23.13 +21:49:55.6 Himalia (15.5mag)
07:30:44.04 +22:12:12.9 Thebe (16.4mag)
07:32:49.68 +22:15:08.5 Elara (17.4mag)
07:31:34.66 +22:36:19.6 Pasiphae (17.6mag)
07:38:10.47 +22:12:33.6 Carme (18.7mag)
00:41:55.06 +02:05:52.8 Titan (8.7mag)
00:41:46.07 +02:05:48.6 Rhea (10.0mag)
00:41:48.00 +02:04:04.4 Iapetus (11.4mag)
00:41:39.99 +02:05:24.7 Hyperion (14.7mag)
00:42:56.22 +02:10:39.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 16 08:22 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461176.89275073:
17:05:44.69 -30:54:33.3 JWST
17:41:01.12 +37:46:11.1 Chandra
09:14:50.24 -52:47:30.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 16 08:22 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461176.89275073 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
13:30:35.52 -28:01:37.0 14.6mag D/1884 O1 (Barnard)
06:20:37.13 +30:52:41.7 15.8mag D/1886 K1 (Brooks)
15:35:17.76 +00:48:16.4 14.8mag D/1895 Q1 (Swift)
05:12:31.04 +24:15:03.4 17.1mag D/1918 W1 (Schorr)
08:19:45.52 +22:38:22.0 17.7mag P/2009 WX51 (Catalina)
18:54:30.33 -30:53:14.2 13.7mag P/2010 H2 (Vales)
05:31:46.90 -68:30:19.0 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:40:59.74 +31:42:02.1 17.4mag C/2017 K2 (PANSTARRS)
17:23:24.32 +13:45:32.5 17.7mag C/2021 G2 (ATLAS)
23:14:48.67 +30:35:45.0 17.2mag C/2022 E2 (ATLAS)
05:05:55.29 +26:43:02.2 16.3mag C/2022 N2 (PANSTARRS)
09:15:13.80 +31:44:18.0 16.5mag C/2022 QE78 (ATLAS)
08:39:45.46 +02:33:42.1 17.5mag C/2022 R6 (PANSTARRS)
18:41:51.83 +20:43:34.6 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:28:36.61 -11:06:54.4 17.5mag P/2023 B1 (PANSTARRS)
08:59:53.18 -07:42:39.2 17.9mag C/2023 F3 (ATLAS)
22:14:27.25 +64:57:38.2 17.7mag C/2023 H5 (Lemmon)
18:37:20.75 -04:51:02.3 13.8mag C/2023 R1 (PANSTARRS)
14:46:43.25 +87:33:44.5 17.9mag C/2023 X2 (Lemmon)
06:42:10.53 +63:43:06.0 17.5mag C/2024 A1 (ATLAS)
06:10:39.79 +25:10:05.9 12.7mag C/2024 E1 (Wierzchos)
15:56:05.33 +10:59:57.8 17.3mag C/2024 G6 (ATLAS)
20:22:35.70 +24:09:25.5 14.2mag C/2024 J3 (ATLAS)
03:55:14.91 -18:17:17.8 16.2mag C/2024 T5 (ATLAS)
05:44:23.46 +38:39:46.8 17.9mag C/2025 J1 (Borisov)
12:01:04.12 +53:22:49.9 16.5mag C/2025 L1 (ATLAS)
05:58:43.63 -09:04:01.9 11.2mag C/2025 R3 (PANSTARRS)
12:43:02.44 +04:24:25.9 17.2mag C/2025 Y1 (ATLAS)
01:15:47.81 +41:26:41.7 15.5mag C/2026 B2 (Sun-Gao)
11:12:31.16 -13:51:41.7 16.1mag A/2026 E1
19:41:18.50 -08:15:23.4 10.0mag 10P/Tempel
14:24:43.86 -00:59:40.1 16.8mag 24P/Schaumasse
10:59:01.93 -00:53:42.2 15.9mag 29P/Schwassmann-Wachmann
10:45:28.90 -02:38:10.3 17.5mag 43P/Wolf-Harrington
02:36:07.89 +22:23:23.1 17.5mag 47P/Ashbrook-Jackson
08:11:33.07 +29:55:11.7 16.9mag 63P/Wild
00:04:48.99 -08:10:47.5 15.7mag 65P/Gunn
05:31:01.26 +29:48:59.6 16.3mag 76P/West-Kohoutek-Ikemura
02:14:50.89 +13:49:28.7 14.0mag 78P/Gehrels
00:27:10.46 -00:41:48.4 15.1mag 88P/Howell
03:41:40.23 +27:26:48.3 15.1mag 93P/Lovas
05:57:46.41 +33:18:48.7 15.9mag 123P/West-Hartley
09:11:52.97 +24:34:50.3 16.4mag 124P/Mrkos
03:21:35.70 +17:27:18.1 16.4mag 128P/Shoemaker-Holt
03:47:57.48 +17:37:06.0 17.6mag 131P/Mueller
04:09:26.05 +19:31:51.4 11.9mag 141P/Machholz
04:12:59.23 +14:33:05.9 11.8mag 141P-A/Machholz
02:54:18.02 +11:04:32.0 10.5mag 141P-D/Machholz
02:40:48.50 -28:18:52.8 17.6mag 161P/Hartley-IRAS
02:29:56.08 +13:39:20.3 14.8mag 162P/SidingSpring
17:09:19.42 -10:18:07.7 16.2mag 235P/LINEAR
06:42:37.55 +35:54:50.4 17.2mag 240P/NEAT
07:58:10.11 -02:34:35.0 18.0mag 242P/Spahr
23:33:29.79 -11:26:34.6 17.0mag 260P/McNaught
03:05:44.16 +27:47:12.3 17.7mag 295P/LINEAR
15:27:11.16 +08:18:42.8 17.4mag 391P/Kowalski
07:50:25.20 +21:11:57.0 17.8mag 450P/LONEOS
06:22:54.87 +43:13:01.6 17.7mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 16 08:22 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
01:13:11.60 -33:25:16.10 2026-05-13.41 16.8
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
01:13:11.60 -33:25:16.10 2026-05-13.41 16.8
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
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -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
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
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
-rw-r--r-- 1 apache apache 188K May 16 08:22 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:39:12.700 +26:22:45.94 AT 2026mbn 2026-05-07.91 20.01
08:43:14.046 -12:27:44.01 AT 2026mbm 2026-05-11.01 19.298
08:06:58.636 +12:14:42.48 AT 2026mbl 2026-05-10.98 19.209
08:03:49.724 +08:46:23.51 AT 2026mbk 2026-05-10.98 18.791
16:11:41.710 -24:03:58.63 AT 2026mbj 2026-05-10.33 20.1009
15:07:09.944 +22:57:46.48 AT 2026mbi 2026-05-07.31 20.6241
13:42:19.773 +47:03:00.78 AT 2026mbh 2026-04-17.32 20.8541
11:49:00.086 +08:01:50.77 AT 2026mbg 2026-05-11.28 19.6199
11:23:16.401 +78:54:34.59 AT 2026mbf 2026-03-12.27 20.0252
18:51:53.437 -14:24:27.20 AT 2026mbe 2026-05-09.50 18.22
19:57:19.177 +14:53:10.19 AT 2026mbd 2026-05-07.47 18
16:40:52.672 -01:10:17.77 SN 2026mbc 2026-05-02.42 17.55
17:06:12.819 -16:40:54.28 AT 2026mbb 2026-02-06.56 19.5689
16:57:35.331 +21:47:47.40 AT 2026mba 2026-05-07.43 20.53
06:29:52.132 +51:37:24.24 AT 2026maz 2026-05-06.25 20.11
14:24:27.954 +49:06:41.65 AT 2026may 2026-05-06.42 20.89
08:12:26.744 -14:34:02.26 AT 2026max 2026-05-08.26 19.55
08:26:21.218 -19:09:53.70 AT 2026maw 2026-05-08.26 20.81
14:10:04.550 -06:02:36.44 AT 2026mav 2026-05-07.48 20.04
11:50:36.810 -33:08:06.10 AT 2026mau 2026-04-27.58 19.6
-rw-r--r-- 1 apache apache 30K May 16 08:22 tns_transients_list.txt
