This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV
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 08 25.1639 2461277.6639 10.49 23:21:42.30 +50:06:40.6
108.53245 -10.23490 galactic And Second-epoch detections are separated by 1.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.4335+50.1053 | 23:21:42.30 +50:06:40.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:42.30 +50:06:40.6: 15.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:42.30 +50:06:40.6: 14.71 +/- 99.00 upperlimit
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 08 25.1639* 23 21 42.30 +50 06 40.6 10.5 U And 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 J350.4335+50.1053,2461277.6639,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.4335+50.1053 20260825.1639 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 14.22 23:56:48.29 +50:59:51.1
114.22590 -10.94838 galactic Cas Second-epoch detections are separated by 7.3" 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 | target | 23:56:48.29 +50:59:51.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:56:48.29 +50:59:51.1: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:56:48.29 +50:59:51.1: 15.10 +/- 99.00 upperlimit
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 08 25.1639* 23 56 48.29 +50 59 51.1 14.2 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,2461277.6639,14.22,0.05,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 20260825.1639 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 14.11 23:38:48.31 +53:36:52.0
112.17936 -7.73411 galactic Cas Second-epoch detections are separated by 6.8" 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 J354.7014+53.6234 | 23:38:48.31 +53:36:52.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:48.31 +53:36:52.0: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:48.31 +53:36:52.0: 15.04 +/- 99.00 upperlimit
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 08 25.1639* 23 38 48.31 +53 36 52.0 14.1 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 J354.7014+53.6234,2461277.6639,14.11,0.05,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
ATO J354.7014+53.6234 20260825.1639 14.11CV 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 08 25.1639 2461277.6639 14.23 23:30:20.83 +50:22:17.8
109.94577 -10.44427 galactic And Second-epoch detections are separated by 3.0" 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 | 23:30:20.83 +50:22:17.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:20.83 +50:22:17.8: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:20.83 +50:22:17.8: 14.93 +/- 99.00 upperlimit
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 08 25.1639* 23 30 20.83 +50 22 17.8 14.2 U And 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,2461277.6639,14.23,0.05,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
target 20260825.1639 14.23CV 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 08 25.1639 2461277.6639 14.30 23:28:11.69 +53:34:43.9
110.65369 -7.29673 galactic Cas Second-epoch detections are separated by 6.6" 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 | 23:28:11.69 +53:34:43.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:11.69 +53:34:43.9: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:11.69 +53:34:43.9: 14.97 +/- 99.00 upperlimit
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 08 25.1639* 23 28 11.69 +53 34 43.9 14.3 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,2461277.6639,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 14.25 00:09:00.35 +54:34:36.3
116.74959 -7.78486 galactic Cas Second-epoch detections are separated by 3.6" 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 420202179853871616 | 00:08:56.23 +54:34:32.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:00.35 +54:34:36.3: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:00.35 +54:34:36.3: 15.06 +/- 99.00 upperlimit
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 08 25.1639* 00 09 00.35 +54 34 36.3 14.2 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 420202179853871616,2461277.6639,14.25,0.05,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 420202179853871616 20260825.1639 14.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 14.15 23:16:48.67 +56:44:39.5
110.19258 -3.76864 galactic Cas Second-epoch detections are separated by 3.9" 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 | 23:16:48.67 +56:44:39.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:16:48.67 +56:44:39.5: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:16:48.67 +56:44:39.5: 14.82 +/- 99.00 upperlimit
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 08 25.1639* 23 16 48.67 +56 44 39.5 14.2 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,2461277.6639,14.15,0.05,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 20260825.1639 14.15CV 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 08 25.1639 2461277.6639 14.05 23:50:57.87 +53:34:45.9
113.93047 -8.23211 galactic Cas Second-epoch detections are separated by 2.5" 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 | 23:50:57.87 +53:34:45.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:50:57.87 +53:34:45.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:50:57.87 +53:34:45.9: 15.06 +/- 99.00 upperlimit
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 08 25.1639* 23 50 57.87 +53 34 45.9 14.1 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,2461277.6639,14.05,0.05,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 20260825.1639 14.05CV 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 08 25.1639 2461277.6639 14.29 23:52:43.77 +51:16:38.3
113.65456 -10.53384 galactic Cas Second-epoch detections are separated by 3.7" 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 | 23:52:43.77 +51:16:38.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:52:43.77 +51:16:38.3: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:52:43.77 +51:16:38.3: 14.98 +/- 99.00 upperlimit
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 08 25.1639* 23 52 43.77 +51 16 38.3 14.3 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,2461277.6639,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.88 23:17:17.74 +56:04:19.7
110.01465 -4.42041 galactic Cas Second-epoch detections are separated by 7.3" 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 | 23:17:17.74 +56:04:19.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:17.74 +56:04:19.7: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:17.74 +56:04:19.7: 14.84 +/- 99.00 upperlimit
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 08 25.1639* 23 17 17.74 +56 04 19.7 13.9 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,2461277.6639,13.88,0.05,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 20260825.1639 13.88CV 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 08 25.1639 2461277.6639 14.09 00:15:17.00 +51:40:37.0
117.24041 -10.79482 galactic Cas Second-epoch detections are separated by 4.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:15:17.00 +51:40:37.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:15:17.00 +51:40:37.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:15:17.00 +51:40:37.0: 14.97 +/- 99.00 upperlimit
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 08 25.1639* 00 15 17.00 +51 40 37.0 14.1 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,2461277.6639,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.93 23:27:25.43 +56:44:43.8
111.56505 -4.26065 galactic Cas Second-epoch detections are separated by 4.3" 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 | 23:27:25.43 +56:44:43.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:25.43 +56:44:43.8: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:25.43 +56:44:43.8: 14.98 +/- 99.00 upperlimit
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 08 25.1639* 23 27 25.43 +56 44 43.8 13.9 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,2461277.6639,13.93,0.05,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 20260825.1639 13.93CV 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 08 25.1639 2461277.6639 13.97 23:35:37.60 +51:04:21.3
110.97102 -10.03007 galactic Cas Second-epoch detections are separated by 2.9" and 5.4 pix
The object was found in VSX15" Gaia DR3 1944740133410439296
Type: ROT
# Max. Min./Amp. JD0 Period
16.000 G 16.050 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:37.60 +51:04:21.3: 15.64 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:37.60 +51:04:21.3: 14.98 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.64 +/- 0.36
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 08 25.1639* 23 35 37.60 +51 04 21.3 14.0 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 1944740133410439296,2461277.6639,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944740133410439296 20260825.1639 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 14.01 23:34:07.22 +54:09:29.1
111.67095 -7.01452 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 | 23:34:07.22 +54:09:29.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:07.22 +54:09:29.1: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:07.22 +54:09:29.1: 15.05 +/- 99.00 upperlimit
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 08 25.1639* 23 34 07.22 +54 09 29.1 14.0 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,2461277.6639,14.01,0.05,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 20260825.1639 14.01CV 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 08 25.1639 2461277.6639 13.93 23:57:55.58 +50:00:11.9
114.18839 -11.95780 galactic Cas Second-epoch detections are separated by 8.6" 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 | target | 23:57:55.58 +50:00:11.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:55.58 +50:00:11.9: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:55.58 +50:00:11.9: 15.04 +/- 99.00 upperlimit
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 08 25.1639* 23 57 55.58 +50 00 11.9 13.9 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,2461277.6639,13.93,0.05,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 20260825.1639 13.93CV 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 08 25.1639 2461277.6639 13.86 23:42:53.84 +54:25:05.1
112.98317 -7.12436 galactic Cas Second-epoch detections are separated by 5.3" 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 | 23:42:53.84 +54:25:05.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:53.84 +54:25:05.1: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:53.84 +54:25:05.1: 14.98 +/- 99.00 upperlimit
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 08 25.1639* 23 42 53.84 +54 25 05.1 13.9 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,2461277.6639,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.82 23:24:41.24 +50:39:38.4
109.17601 -9.87954 galactic And Second-epoch detections are separated by 6.9" 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 | target | 23:24:41.24 +50:39:38.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:41.24 +50:39:38.4: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:41.24 +50:39:38.4: 14.91 +/- 99.00 upperlimit
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 08 25.1639* 23 24 41.24 +50 39 38.4 13.8 U And 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,2461277.6639,13.82,0.05,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 20260825.1639 13.82CV 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 08 25.1639 2461277.6639 13.79 23:41:49.04 +51:06:39.5
111.92941 -10.26742 galactic Cas Second-epoch detections are separated by 0.4" 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 | 23:41:49.04 +51:06:39.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:41:49.04 +51:06:39.5: 15.60 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:41:49.04 +51:06:39.5: 15.03 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.60 +/- 0.34
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 08 25.1639* 23 41 49.04 +51 06 39.5 13.8 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,2461277.6639,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.95 00:13:01.82 +53:50:13.6
117.21877 -8.60805 galactic Cas Second-epoch detections are separated by 6.1" 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 | 00:13:01.82 +53:50:13.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:13:01.82 +53:50:13.6: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:13:01.82 +53:50:13.6: 15.02 +/- 99.00 upperlimit
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 08 25.1639* 00 13 01.82 +53 50 13.6 13.9 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,2461277.6639,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.95CV 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 08 25.1639 2461277.6639 13.95 23:19:54.07 +49:51:21.3
108.16576 -10.37321 galactic And Second-epoch detections are separated by 3.1" and 4.9 pix
The object was found in VSX 8" Gaia DR3 1991159482809413504
Type: E
# Max. Min./Amp. JD0 Period
19.220 G 20.150 G 0.427519000000
ATTENTION: measured mag 13.95 is 5.3 mag brighter than the VSX record maximum brightness 19.22 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:54.07 +49:51:21.3: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:54.07 +49:51:21.3: 14.87 +/- 99.00 upperlimit
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 08 25.1639* 23 19 54.07 +49 51 21.3 13.9 U And 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 1991159482809413504,2461277.6639,13.95,0.05,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 1991159482809413504 20260825.1639 13.95CV 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 08 25.1639 2461277.6639 13.91 00:00:34.95 +51:13:14.6
114.86367 -10.85260 galactic Cas Second-epoch detections are separated by 8.3" 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 | 00:00:34.95 +51:13:14.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:00:34.95 +51:13:14.6: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:00:34.95 +51:13:14.6: 14.99 +/- 99.00 upperlimit
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 08 25.1639* 00 00 34.95 +51 13 14.6 13.9 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,2461277.6639,13.91,0.05,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 20260825.1639 13.91CV 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 08 25.1639 2461277.6639 13.82 23:15:45.90 +55:44:41.8
109.69594 -4.64871 galactic Cas Second-epoch detections are separated by 4.9" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J231540.50+554438.8 | 23:15:40.49 +55:44:38.8 (Gaia DR3) | SR (local) | 330.000000000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:45.90 +55:44:41.8: 14.73 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:45.90 +55:44:41.8: 14.76 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.73 +/- 0.19
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 08 25.1639* 23 15 45.90 +55 44 41.8 13.8 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
ASASSN-V J231540.50+554438.8,2461277.6639,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J231540.50+554438.8 20260825.1639 13.82CV 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 08 25.1639 2461277.6639 13.71 00:07:48.32 +54:40:28.6
116.59329 -7.65926 galactic Cas Second-epoch detections are separated by 6.9" 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 | ATO J001.9645+54.6665 | 00:07:48.32 +54:40:28.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:48.32 +54:40:28.6: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:48.32 +54:40:28.6: 15.09 +/- 99.00 upperlimit
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 08 25.1639* 00 07 48.32 +54 40 28.6 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.9645+54.6665,2461277.6639,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.9645+54.6665 20260825.1639 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.85 23:26:51.06 +50:20:13.9
109.39744 -10.29845 galactic And Second-epoch detections are separated by 7.6" 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 | target | 23:26:51.06 +50:20:13.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:51.06 +50:20:13.9: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:51.06 +50:20:13.9: 14.90 +/- 99.00 upperlimit
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 08 25.1639* 23 26 51.06 +50 20 13.9 13.8 U And 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,2461277.6639,13.85,0.05,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
target 20260825.1639 13.85CV 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 08 25.1639 2461277.6639 13.63 23:45:29.04 +54:37:38.2
113.40309 -7.01967 galactic Cas Second-epoch detections are separated by 3.3" 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 | 23:45:29.04 +54:37:38.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:29.04 +54:37:38.2: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:29.04 +54:37:38.2: 15.00 +/- 99.00 upperlimit
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 08 25.1639* 23 45 29.04 +54 37 38.2 13.6 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,2461277.6639,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.72 23:30:42.20 +58:00:40.6
112.38354 -3.19745 galactic Cas Second-epoch detections are separated by 3.2" 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 | 23:30:42.20 +58:00:40.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:42.20 +58:00:40.6: 15.01 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:42.20 +58:00:40.6: 14.87 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.01 +/- 0.24
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 08 25.1639* 23 30 42.20 +58 00 40.6 13.7 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,2461277.6639,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.72CV 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 08 25.1639 2461277.6639 13.59 00:05:33.49 +50:54:12.9
115.58440 -11.31247 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 | target | 00:05:33.49 +50:54:12.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:33.49 +50:54:12.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:33.49 +50:54:12.9: 15.06 +/- 99.00 upperlimit
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 08 25.1639* 00 05 33.49 +50 54 12.9 13.6 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,2461277.6639,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.79 23:58:27.57 +52:16:04.1
114.75285 -9.76060 galactic Cas Second-epoch detections are separated by 3.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:58:27.57 +52:16:04.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:27.57 +52:16:04.1: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:27.57 +52:16:04.1: 15.06 +/- 99.00 upperlimit
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 08 25.1639* 23 58 27.57 +52 16 04.1 13.8 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,2461277.6639,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.78 23:22:41.95 +50:08:56.4
108.69768 -10.25417 galactic And Second-epoch detections are separated by 2.3" 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 | target | 23:22:41.95 +50:08:56.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:41.95 +50:08:56.4: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:41.95 +50:08:56.4: 14.94 +/- 99.00 upperlimit
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 08 25.1639* 23 22 41.95 +50 08 56.4 13.8 U And 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,2461277.6639,13.78,0.05,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
target 20260825.1639 13.78CV 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 08 25.1639 2461277.6639 13.63 00:23:12.05 +56:00:07.1
118.96475 -6.65212 galactic Cas Second-epoch detections are separated by 8.6" 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 | 00:23:12.05 +56:00:07.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:23:12.05 +56:00:07.1: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:23:12.05 +56:00:07.1: 15.08 +/- 99.00 upperlimit
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 08 25.1639* 00 23 12.05 +56 00 07.1 13.6 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,2461277.6639,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.59 23:46:33.71 +53:16:40.3
113.21356 -8.36533 galactic Cas Second-epoch detections are separated by 4.7" 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 | 23:46:33.71 +53:16:40.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:46:33.71 +53:16:40.3: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:46:33.71 +53:16:40.3: 15.10 +/- 99.00 upperlimit
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 08 25.1639* 23 46 33.71 +53 16 40.3 13.6 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,2461277.6639,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.51 23:30:32.83 +54:53:57.6
111.39986 -6.15104 galactic Cas Second-epoch detections are separated by 7.6" 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 J352.6420+54.9068 | 23:30:32.83 +54:53:57.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:32.83 +54:53:57.6: 14.88 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:32.83 +54:53:57.6: 14.92 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.88 +/- 0.20
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 08 25.1639* 23 30 32.83 +54 53 57.6 13.5 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 J352.6420+54.9068,2461277.6639,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.6420+54.9068 20260825.1639 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.52 23:20:43.46 +52:15:31.1
109.13877 -8.16691 galactic And Second-epoch detections are separated by 2.6" 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 | 23:20:43.46 +52:15:31.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:43.46 +52:15:31.1: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:43.46 +52:15:31.1: 14.90 +/- 99.00 upperlimit
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 08 25.1639* 23 20 43.46 +52 15 31.1 13.5 U And 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,2461277.6639,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.70 00:09:31.08 +51:50:03.3
116.36791 -10.50243 galactic Cas Second-epoch detections are separated by 1.3" 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 | ATO J002.3863+51.8376 | 00:09:33.37 +51:50:27.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:31.08 +51:50:03.3: 15.04 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:31.08 +51:50:03.3: 15.05 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.04 +/- 0.21
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 08 25.1639* 00 09 31.08 +51 50 03.3 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.3863+51.8376,2461277.6639,13.70,0.05,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
ATO J002.3863+51.8376 20260825.1639 13.70CV 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 08 25.1639 2461277.6639 13.67 00:27:15.89 +53:26:57.0
119.28981 -9.25155 galactic Cas Second-epoch detections are separated by 8.0" 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 | 00:27:15.89 +53:26:57.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:27:15.89 +53:26:57.0: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:27:15.89 +53:26:57.0: 14.95 +/- 99.00 upperlimit
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 08 25.1639* 00 27 15.89 +53 26 57.0 13.7 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,2461277.6639,13.67,0.05,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 20260825.1639 13.67CV 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 08 25.1639 2461277.6639 13.55 23:18:13.31 +54:31:38.2
109.58740 -5.91135 galactic Cas Second-epoch detections are separated by 1.4" 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 | Gaia DR3 1996038776119496320 | 23:18:16.38 +54:31:18.4 (Gaia DR3) | E (local) | 3.188420000000 (local) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:13.31 +54:31:38.2: 14.96 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:13.31 +54:31:38.2: 14.85 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.96 +/- 0.24
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 08 25.1639* 23 18 13.31 +54 31 38.2 13.6 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 1996038776119496320,2461277.6639,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996038776119496320 20260825.1639 13.55CV 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 08 25.1639 2461277.6639 13.35 23:29:05.88 +57:56:19.4
112.15836 -3.20034 galactic Cas 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 | target | 23:29:05.88 +57:56:19.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:05.88 +57:56:19.4: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:29:05.88 +57:56:19.4: 14.86 +/- 99.00 upperlimit
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 08 25.1639* 23 29 05.88 +57 56 19.4 13.3 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,2461277.6639,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.47 00:05:06.43 +54:30:24.1
116.17531 -7.75612 galactic Cas Second-epoch detections are separated by 8.9" 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 | target | 00:05:06.43 +54:30:24.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:06.43 +54:30:24.1: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:06.43 +54:30:24.1: 15.09 +/- 99.00 upperlimit
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 08 25.1639* 00 05 06.43 +54 30 24.1 13.5 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
target,2461277.6639,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.38 23:18:16.98 +54:09:21.5
109.46360 -6.26177 galactic Cas Second-epoch detections are separated by 4.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:18:16.98 +54:09:21.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:16.98 +54:09:21.5: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:16.98 +54:09:21.5: 14.86 +/- 99.00 upperlimit
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 08 25.1639* 23 18 16.98 +54 09 21.5 13.4 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,2461277.6639,13.38,0.05,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 20260825.1639 13.38CV 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 08 25.1639 2461277.6639 13.14 23:38:15.75 +56:01:37.7
112.78441 -5.39617 galactic Cas Second-epoch detections are separated by 6.6" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:38:15.75 +56:01:37.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:15.75 +56:01:37.7: 14.82 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:15.75 +56:01:37.7: 14.77 +/- 0.31 detection
Forced photometry reference-image weighted average: 14.80 +/- 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 08 25.1639* 23 38 15.75 +56 01 37.7 13.1 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,2461277.6639,13.14,0.05,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
target 20260825.1639 13.14CV 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 08 25.1639 2461277.6639 13.31 23:37:51.41 +51:51:10.9
111.53728 -9.38338 galactic Cas Second-epoch detections are separated by 1.9" 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 | target | 23:37:51.41 +51:51:10.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:51.41 +51:51:10.9: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:51.41 +51:51:10.9: 15.02 +/- 99.00 upperlimit
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 08 25.1639* 23 37 51.41 +51 51 10.9 13.3 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,2461277.6639,13.31,0.05,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 20260825.1639 13.31CV 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 08 25.1639 2461277.6639 13.15 23:20:45.72 +54:32:02.1
109.93688 -6.03390 galactic Cas Second-epoch detections are separated by 0.8" and 4.5 pix
The object was found in VSX14" ZTF J232047.31+543158.6
Type: BY
# Max. Min./Amp. JD0 Period
15.968 r Y 0.061 r 2458249.97550 1.204554300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:45.72 +54:32:02.1: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:45.72 +54:32:02.1: 14.96 +/- 99.00 upperlimit
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 08 25.1639* 23 20 45.72 +54 32 02.1 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J232047.31+543158.6,2461277.6639,13.15,0.05,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 J232047.31+543158.6 20260825.1639 13.15CV 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 08 25.1639 2461277.6639 13.09 23:39:45.45 +51:01:20.1
111.58842 -10.26393 galactic Cas Second-epoch detections are separated by 2.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:39:45.45 +51:01:20.1 (user input) | T | P | (position from user input) J-Ks=0.548+/-0.222 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:45.45 +51:01:20.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:45.45 +51:01:20.1: 15.03 +/- 99.00 upperlimit
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 08 25.1639* 23 39 45.45 +51 01 20.1 13.1 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,2461277.6639,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.04 23:12:56.89 +55:27:53.2
109.22147 -4.76329 galactic Cas Second-epoch detections are separated by 5.9" and 5.1 pix
The object was found in VSX 7" ZTF J231256.89+552746.2
Type: BY
# Max. Min./Amp. JD0 Period
17.664 r Y 0.059 r 2458312.92640 0.895689800000
ATTENTION: measured mag 13.04 is 4.6 mag brighter than the VSX record maximum brightness 17.61 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:56.89 +55:27:53.2: 14.90 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:56.89 +55:27:53.2: 14.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.90 +/- 0.22
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 08 25.1639* 23 12 56.89 +55 27 53.2 13.0 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 J231256.89+552746.2,2461277.6639,13.04,0.05,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
ZTF J231256.89+552746.2 20260825.1639 13.04CV 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 08 25.1639 2461277.6639 12.89 23:27:48.29 +56:18:33.6
111.47530 -4.69076 galactic Cas Second-epoch detections are separated by 1.5" 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 | ATO J351.9448+56.3109 | 23:27:48.29 +56:18:33.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:48.29 +56:18:33.6: 15.49 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:48.29 +56:18:33.6: 14.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.49 +/- 0.35
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 08 25.1639* 23 27 48.29 +56 18 33.6 12.9 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
ATO J351.9448+56.3109,2461277.6639,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.9448+56.3109 20260825.1639 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 12.82 23:42:00.50 +51:29:24.8
112.06263 -9.91033 galactic Cas Second-epoch detections are separated by 3.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:42:00.50 +51:29:24.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:00.50 +51:29:24.8: 15.53 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:00.50 +51:29:24.8: 15.12 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.53 +/- 0.31
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 08 25.1639* 23 42 00.50 +51 29 24.8 12.8 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,2461277.6639,12.82,0.05,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 20260825.1639 12.82CV 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 08 25.1639 2461277.6639 12.86 23:21:10.64 +55:53:37.8
110.46239 -4.77724 galactic Cas Second-epoch detections are separated by 4.1" and 4.6 pix
The object was found in VSX22" ZTF J232111.75+555357.2
Type: EW
# Max. Min./Amp. JD0 Period
17.487 r Y 0.217 r 2458273.92520 0.421857800000
ATTENTION: measured mag 12.86 is 4.4 mag brighter than the VSX record maximum brightness 17.27 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:10.64 +55:53:37.8: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:10.64 +55:53:37.8: 14.86 +/- 99.00 upperlimit
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 08 25.1639* 23 21 10.64 +55 53 37.8 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J232111.75+555357.2,2461277.6639,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J232111.75+555357.2 20260825.1639 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 12.88 00:07:16.49 +51:00:10.5
115.87367 -11.26260 galactic Cas Second-epoch detections are separated by 1.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:07:16.49 +51:00:10.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:16.49 +51:00:10.5: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:16.49 +51:00:10.5: 14.98 +/- 99.00 upperlimit
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 08 25.1639* 00 07 16.49 +51 00 10.5 12.9 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,2461277.6639,12.88,0.05,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 20260825.1639 12.88CV 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 08 25.1639 2461277.6639 12.51 23:27:18.08 +56:40:25.9
111.52609 -4.32314 galactic Cas Second-epoch detections are separated by 4.6" 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 | 23:27:18.08 +56:40:25.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:18.08 +56:40:25.9: 15.31 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:18.08 +56:40:25.9: 14.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.31 +/- 0.29
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 08 25.1639* 23 27 18.08 +56 40 25.9 12.5 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
target,2461277.6639,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 12.43 23:32:09.66 +52:54:18.0
111.01060 -8.12199 galactic Cas Second-epoch detections are separated by 2.2" 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 | 23:32:09.66 +52:54:18.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:09.66 +52:54:18.0: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:09.66 +52:54:18.0: 14.93 +/- 99.00 upperlimit
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 08 25.1639* 23 32 09.66 +52 54 18.0 12.4 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,2461277.6639,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 12.36 23:59:24.38 +50:35:23.0
114.54873 -11.43317 galactic Cas Second-epoch detections are separated by 5.9" 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 | 23:59:24.38 +50:35:23.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:59:24.38 +50:35:23.0: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:59:24.38 +50:35:23.0: 15.09 +/- 99.00 upperlimit
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 08 25.1639* 23 59 24.38 +50 35 23.0 12.4 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,2461277.6639,12.36,0.05,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 20260825.1639 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 12.42 23:12:58.95 +56:18:50.6
109.54266 -3.97670 galactic Cas Second-epoch detections are separated by 6.4" 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 | ATO J348.2419+56.3061 | 23:12:58.95 +56:18:50.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:58.95 +56:18:50.6: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:58.95 +56:18:50.6: 14.86 +/- 99.00 upperlimit
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 08 25.1639* 23 12 58.95 +56 18 50.6 12.4 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 J348.2419+56.3061,2461277.6639,12.42,0.05,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 J348.2419+56.3061 20260825.1639 12.42CV 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 08 25.1639 2461277.6639 12.60 23:20:03.66 +49:30:57.1
108.06871 -10.70063 galactic And Second-epoch detections are separated by 4.6" 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 | 23:20:03.66 +49:30:57.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:03.66 +49:30:57.1: 15.13 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:03.66 +49:30:57.1: 14.83 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.13 +/- 0.27
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 08 25.1639* 23 20 03.66 +49 30 57.1 12.6 U And 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,2461277.6639,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 12.68 23:14:48.20 +54:45:40.1
109.20832 -5.51516 galactic Cas Second-epoch detections are separated by 7.0" and 4.8 pix
The object was found in VSX25" ZTF J231450.86+544548.4
Type: BY
# Max. Min./Amp. JD0 Period
15.938 r Y 0.040 r 2458373.80570 1.259359400000
ATTENTION: measured mag 12.68 is 3.2 mag brighter than the VSX record maximum brightness 15.90 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:14:48.20 +54:45:40.1: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:48.20 +54:45:40.1: 14.88 +/- 99.00 upperlimit
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 08 25.1639* 23 14 48.20 +54 45 40.1 12.7 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 J231450.86+544548.4,2461277.6639,12.68,0.05,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
ZTF J231450.86+544548.4 20260825.1639 12.68CV 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 08 25.1639 2461277.6639 13.07 23:12:49.57 +57:05:36.5
109.81298 -3.24515 galactic Cas Second-epoch detections are separated by 8.1" 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 | 23:12:49.57 +57:05:36.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:49.57 +57:05:36.5: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:49.57 +57:05:36.5: 14.84 +/- 99.00 upperlimit
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 08 25.1639* 23 12 49.57 +57 05 36.5 13.1 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,2461277.6639,13.07,0.05,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 20260825.1639 13.07CV 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 08 25.1639 2461277.6639 13.48 23:30:53.65 +49:58:04.2
109.90192 -10.85519 galactic And Second-epoch detections are separated by 0.9" 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 | target | 23:30:53.65 +49:58:04.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:53.65 +49:58:04.2: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:53.65 +49:58:04.2: 14.89 +/- 99.00 upperlimit
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 08 25.1639* 23 30 53.65 +49 58 04.2 13.5 U And 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,2461277.6639,13.48,0.05,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 20260825.1639 13.48CV 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 08 25.1639 2461277.6639 13.56 00:26:59.42 +51:56:16.5
119.10092 -10.75189 galactic Cas Second-epoch detections are separated by 6.0" 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 | 00:26:59.42 +51:56:16.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:26:59.42 +51:56:16.5: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:26:59.42 +51:56:16.5: 14.98 +/- 99.00 upperlimit
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 08 25.1639* 00 26 59.42 +51 56 16.5 13.6 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,2461277.6639,13.56,0.05,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 20260825.1639 13.56CV 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 08 25.1639 2461277.6639 13.57 23:21:44.42 +54:27:02.2
110.04231 -6.16090 galactic Cas Second-epoch detections are separated by 4.3" 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 | ATO J350.4458+54.4444 | 23:21:44.42 +54:27:02.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:44.42 +54:27:02.2: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:44.42 +54:27:02.2: 14.93 +/- 99.00 upperlimit
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 08 25.1639* 23 21 44.42 +54 27 02.2 13.6 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 J350.4458+54.4444,2461277.6639,13.57,0.05,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 J350.4458+54.4444 20260825.1639 13.57CV 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 08 25.1639 2461277.6639 13.51 23:33:08.76 +51:57:12.2
110.86333 -9.07430 galactic Cas Second-epoch detections are separated by 4.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.2771+51.9458 | 23:33:08.76 +51:57:12.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:08.76 +51:57:12.2: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:08.76 +51:57:12.2: 14.99 +/- 99.00 upperlimit
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 08 25.1639* 23 33 08.76 +51 57 12.2 13.5 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 J353.2771+51.9458,2461277.6639,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.2771+51.9458 20260825.1639 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.68 00:09:04.74 +51:43:27.8
116.28130 -10.59954 galactic Cas Second-epoch detections are separated by 5.0" 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 | target | 00:09:04.74 +51:43:27.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:04.74 +51:43:27.8: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:04.74 +51:43:27.8: 15.04 +/- 99.00 upperlimit
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 08 25.1639* 00 09 04.74 +51 43 27.8 13.7 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,2461277.6639,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 13.68CV 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 08 25.1639 2461277.6639 13.69 23:50:03.14 +53:38:14.1
113.81145 -8.14395 galactic Cas Second-epoch detections are separated by 6.7" 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 | 23:50:03.14 +53:38:14.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:50:03.14 +53:38:14.1: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:50:03.14 +53:38:14.1: 15.02 +/- 99.00 upperlimit
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 08 25.1639* 23 50 03.14 +53 38 14.1 13.7 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,2461277.6639,13.69,0.05,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
target 20260825.1639 13.69CV 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 08 25.1639 2461277.6639 13.65 23:49:49.46 +52:31:08.4
113.50779 -9.22170 galactic Cas Second-epoch detections are separated by 3.1" 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 | 23:49:49.46 +52:31:08.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:49:49.46 +52:31:08.4: 15.40 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:49:49.46 +52:31:08.4: 15.06 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.40 +/- 0.29
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 08 25.1639* 23 49 49.46 +52 31 08.4 13.7 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,2461277.6639,13.65,0.05,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 20260825.1639 13.65CV 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 08 25.1639 2461277.6639 13.86 23:48:51.31 +52:53:33.2
113.45475 -8.82377 galactic Cas Second-epoch detections are separated by 3.8" 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 | ATO J357.2195+52.8965 | 23:48:52.47 +52:54:03.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:51.31 +52:53:33.2: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:51.31 +52:53:33.2: 15.13 +/- 99.00 upperlimit
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 08 25.1639* 23 48 51.31 +52 53 33.2 13.9 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
ATO J357.2195+52.8965,2461277.6639,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.2195+52.8965 20260825.1639 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.87 00:05:10.88 +52:08:38.1
115.75400 -10.08199 galactic Cas Second-epoch detections are separated by 4.3" 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 | 00:05:10.88 +52:08:38.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:10.88 +52:08:38.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:10.88 +52:08:38.1: 15.04 +/- 99.00 upperlimit
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 08 25.1639* 00 05 10.88 +52 08 38.1 13.9 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,2461277.6639,13.87,0.05,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
target 20260825.1639 13.87CV 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 08 25.1639 2461277.6639 13.86 23:51:09.98 +51:25:55.4
113.44974 -10.32664 galactic Cas Second-epoch detections are separated by 6.6" 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 J357.7886+51.4251 | 23:51:09.98 +51:25:55.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:51:09.98 +51:25:55.4: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:51:09.98 +51:25:55.4: 14.94 +/- 99.00 upperlimit
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 08 25.1639* 23 51 09.98 +51 25 55.4 13.9 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
ATO J357.7886+51.4251,2461277.6639,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.7886+51.4251 20260825.1639 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 13.82 23:38:04.29 +55:46:00.3
112.68509 -5.63854 galactic Cas Second-epoch detections are separated by 0.5" 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 1997565031399061248 | 23:38:05.88 +55:46:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:04.29 +55:46:00.3: 15.05 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:04.29 +55:46:00.3: 14.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.05 +/- 0.23
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 08 25.1639* 23 38 04.29 +55 46 00.3 13.8 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 1997565031399061248,2461277.6639,13.82,0.05,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 1997565031399061248 20260825.1639 13.82CV 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 08 25.1639 2461277.6639 13.71 23:33:19.74 +56:17:53.3
112.20318 -4.93790 galactic Cas Second-epoch detections are separated by 3.7" 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 J353.3179+56.3052 | 23:33:19.74 +56:17:53.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:19.74 +56:17:53.3: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:19.74 +56:17:53.3: 15.00 +/- 99.00 upperlimit
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 08 25.1639* 23 33 19.74 +56 17 53.3 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.3179+56.3052,2461277.6639,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.3179+56.3052 20260825.1639 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 14.22 23:37:16.12 +51:29:31.0
111.34400 -9.70332 galactic Cas Second-epoch detections are separated by 3.8" 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 | 23:37:16.12 +51:29:31.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:16.12 +51:29:31.0: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:16.12 +51:29:31.0: 15.05 +/- 99.00 upperlimit
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 08 25.1639* 23 37 16.12 +51 29 31.0 14.2 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,2461277.6639,14.22,0.05,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 20260825.1639 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 14.33 23:37:52.68 +50:22:58.9
111.11463 -10.79326 galactic And Second-epoch detections are separated by 2.4" 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 | target | 23:37:52.68 +50:22:58.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:52.68 +50:22:58.9: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:52.68 +50:22:58.9: 14.97 +/- 99.00 upperlimit
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 08 25.1639* 23 37 52.68 +50 22 58.9 14.3 U And 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,2461277.6639,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 25.1639 2461277.6639 14.35 23:42:14.30 +53:13:15.9
112.56747 -8.25243 galactic Cas Second-epoch detections are separated by 5.6" 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 | 23:42:14.30 +53:13:15.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:14.30 +53:13:15.9: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:14.30 +53:13:15.9: 15.06 +/- 99.00 upperlimit
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 08 25.1639* 23 42 14.30 +53 13 15.9 14.3 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,2461277.6639,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.1639 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461239.82421699 18.07.2026 07:46:42.348 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
First image: 2461239.82421699 18.07.2026 07:46:42.348 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Last image: 2461277.66419177 25.08.2026 03:56:16.169 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.76
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: 5 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 12791
Objects passed selection criteria: 12788
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 15490.5
Average stars matched: 15351 (99.0994 %)
Memory usage VmPeak: 245504 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 24 23:03:54 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: 2461239.82421699 18.07.2026 07:46:42.348 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
First image: 2461239.82421699 18.07.2026 07:46:42.348 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Last image: 2461277.66419177 25.08.2026 03:56:16.169 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 246
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
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: 62 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 113172
Objects passed selection criteria: 112969
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 111842
Average stars matched: 109742 (98.1221 %)
Memory usage VmPeak: 518180 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 24 23:07:35 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.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: 2461277.66368813
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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.062 +54:00:02.05 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Image size: 927.0'x616.5' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:06.812 +54:04:03.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.062 +54:00:02.05
Second-epoch image center 00:00:06.812 +54:04:03.85
Angular distance between the image centers 0.0686 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Image size: 927.1'x616.5' 15.5(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:10.170 +54:04:03.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.062 +54:00:02.05
Second-epoch image center 00:00:10.170 +54:04:03.40
Angular distance between the image centers 0.0706 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 00:00:06.812 +54:04:03.85
Second-epoch second image center 00:00:10.170 +54:04:03.40
Angular distance between the image centers 0.00821 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits &> /tmp/tmp.R3Wgo3YnPE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits &> /tmp/tmp.HxfVhuD6M0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits &> /tmp/tmp.Tu8psIkQaD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits &> /tmp/tmp.JFDCoJLkEi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits and wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits and wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits and wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 33669 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.3600 to 15.3869 deg, Dec +47.7769 to +59.3470 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 345.3600 to 15.3869 deg, Dec 47.7769 to 59.3470 deg
Loaded 26243 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): 16959 out of 18283 total matches.
Matched with Tycho-2 18283 out of 33669 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.677900
a=0.000000 b=1.000000 c=22.677900
From vast_summary.log: estimated ref. image limiting mag.: -7.76
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.92
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.92
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 33669 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.3600 to 15.3869 deg, Dec +47.7769 to +59.3470 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 345.3600 to 15.3869 deg, Dec 47.7769 to 59.3470 deg
Loaded 26243 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): 16959 out of 18283 total matches.
Matched with Tycho-2 18283 out of 33669 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits (aperture=7.3)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 14903 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 344.8488 to 14.8386 deg, Dec +48.0248 to +59.2553 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 344.8488 to 14.8386 deg, Dec 48.0248 to 59.2553 deg
Loaded 25721 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): 11593 out of 12074 total matches.
Matched with Tycho-2 12074 out of 14903 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
3.5 pix Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
2.3 pix Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Limiting magnitude estimates:
14.9 mag. Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
14.3 mag. Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
14.2 mag. fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
14.2 mag. fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.R3Wgo3YnPE (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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits' -> 'wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2621, bad_region=6655, passed=33669
Got 33669 stars (including 24831 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
util/solve_plate_with_UCAC5 got 33669 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
RA wraps around 0/360 boundary: field RA 345.3600 through 0 to 15.3869, gap 15.3869 to 345.3600
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.8 to 59.3)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 4904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 28540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3592 through 0 to 15.3870, gap 15.3870 to 345.3592
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.8 to 59.3)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 28540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 28540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4904 stars left (next iteration limit 5394)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits N_match=4904 sigma_overall_arcsec=0.398 sigma_q1_arcsec=0.441 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.363 sigma_q4_arcsec=0.358 n_q1=1555 n_q2=802 n_q3=1643 n_q4=904 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits -region wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.HxfVhuD6M0 (6) ############
Parsing command line arguments...
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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits' -> 'wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1092, bad_region=2856, passed=14903
Got 14903 stars (including 11103 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat
util/solve_plate_with_UCAC5 got 14903 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8488 through 0 to 14.8386, gap 14.8386 to 344.8488
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 4904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 12704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8478 through 0 to 14.8387, gap 14.8387 to 344.8478
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 12704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 12704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4902 stars left (next iteration limit 5394)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits N_match=4902 sigma_overall_arcsec=0.528 sigma_q1_arcsec=0.495 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.586 sigma_q4_arcsec=0.534 n_q1=1550 n_q2=795 n_q3=1659 n_q4=898 worst_quadrant_to_overall_ratio=1.109
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits -region wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Tu8psIkQaD (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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1031, bad_region=2751, passed=14406
Got 14406 stars (including 10764 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat
util/solve_plate_with_UCAC5 got 14406 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.0'
Seting catalog search parameters based on the expected field of view 927.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012875 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010300 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0813 through 0 to 14.9386, gap 14.9386 to 345.0813
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3510 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2190 matched stars entering correct_measured_positions(), 2426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2056 matched stars entering correct_measured_positions(), 12161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.78"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0800 through 0 to 14.9577, gap 14.9577 to 345.0800
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3614 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2477 matched stars entering correct_measured_positions(), 12161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.08"
Accuracy estimation diagnostic: 2411 matched stars entering correct_measured_positions(), 12221 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.92"
Excluding outliers - 2411 stars left (next iteration limit 2261)
SIP_REFIT: SIP order 2 trial: matched=2411 robust_rms=26.556 arcsec worst_quadrant_rms=29.179 arcsec
SIP_REFIT: SIP order 3 trial: matched=2411 robust_rms=25.702 arcsec worst_quadrant_rms=29.752 arcsec
SIP_REFIT: SIP order 5 trial: matched=2411 robust_rms=22.989 arcsec worst_quadrant_rms=29.277 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2411 robust_rms_before=32.402 arcsec robust_rms_before_corrected=19.270 arcsec robust_rms_after=26.556 arcsec worst_quadrant_rms_before=24.346 worst_quadrant_rms_after=29.179
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.346 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits N_match=2411 sigma_overall_arcsec=13.753 sigma_q1_arcsec=29.159 sigma_q2_arcsec=28.015 sigma_q3_arcsec=7.243 sigma_q4_arcsec=5.321 n_q1=540 n_q2=267 n_q3=945 n_q4=659 worst_quadrant_to_overall_ratio=2.120
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.JFDCoJLkEi (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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1032, bad_region=2742, passed=14306
Got 14306 stars (including 10673 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat
util/solve_plate_with_UCAC5 got 14306 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.1'
Seting catalog search parameters based on the expected field of view 927.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012876 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010301 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0815 through 0 to 14.9394, gap 14.9394 to 345.0815
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3509 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2210 matched stars entering correct_measured_positions(), 2448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.11"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2076 matched stars entering correct_measured_positions(), 12053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0803 through 0 to 14.9584, gap 14.9584 to 345.0803
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3637 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2477 matched stars entering correct_measured_positions(), 12053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.95"
Accuracy estimation diagnostic: 2416 matched stars entering correct_measured_positions(), 12088 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.93"
Excluding outliers - 2416 stars left (next iteration limit 2283)
SIP_REFIT: SIP order 2 trial: matched=2416 robust_rms=26.450 arcsec worst_quadrant_rms=29.135 arcsec
SIP_REFIT: SIP order 3 trial: matched=2416 robust_rms=25.779 arcsec worst_quadrant_rms=29.487 arcsec
SIP_REFIT: SIP order 5 trial: matched=2416 robust_rms=23.024 arcsec worst_quadrant_rms=29.536 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2416 robust_rms_before=32.453 arcsec robust_rms_before_corrected=19.397 arcsec robust_rms_after=26.450 arcsec worst_quadrant_rms_before=24.432 worst_quadrant_rms_after=29.135
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.432 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits N_match=2416 sigma_overall_arcsec=13.522 sigma_q1_arcsec=28.887 sigma_q2_arcsec=26.685 sigma_q3_arcsec=7.431 sigma_q4_arcsec=4.930 n_q1=546 n_q2=273 n_q3=936 n_q4=661 worst_quadrant_to_overall_ratio=2.136
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits'
Saving the final (post-refit) wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits'
Saving the final (post-refit) wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits'
Saving the final (post-refit) wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits sigma_overall=0.398 worst_q_ratio=1.108
ref2=Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits sigma_overall=0.528 worst_q_ratio=1.109
new1=fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits sigma_overall=13.753 worst_q_ratio=2.120
new2=fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits sigma_overall=13.522 worst_q_ratio=2.136
reference average sigma_overall=0.463 worst_q_ratio=1.1085
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits) flagged: sigma=13.753 (ref avg 0.463), ratio=2.120 (ref avg 1.1085), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/lib/make_outxyls_for_astrometric_calibration found 13852 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out627626.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out627626.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 24.1633 (3.11894e+10), 7 match, 0 conflict, 20 distractors, 24 index.
RA,Dec = (0.0256278,54.0661), pixel scale 5.9323 arcsec/pix.
Hit/miss: Hit/miss: ---++----+----+-+---+-----+(best)-------+-----------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out627626.solved to indicate this.
Field: out627626.xyls
Field center: (RA,Dec) = (0.027006, 54.066909) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:06.481, +54:04:00.874).
Field size: 15.6095 x 10.4362 degrees
Field rotation angle: up is 3.53585 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits' -> 'fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Aug 24 23:06 fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
-rw-r--r-- 1 apache apache 8.5K Aug 24 23:06 out627626.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits (fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out627626.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out627626.axy"...
Only searching for solutions within 15.45 degrees of RA,Dec (0.0283833,54.0677)
log-odds ratio 24.1633 (3.11894e+10), 7 match, 0 conflict, 20 distractors, 24 index.
RA,Dec = (0.0256278,54.0661), pixel scale 5.9323 arcsec/pix.
Hit/miss: Hit/miss: ---++----+----+-+---+-----+(best)-------+-----------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out627626.solved to indicate this.
Field: out627626.xyls
Field center: (RA,Dec) = (0.027006, 54.066909) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:06.481, +54:04:00.874).
Field size: 15.6095 x 10.4362 degrees
Field rotation angle: up is 3.53585 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Aug 24 23:06 fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
-rw-r--r-- 1 apache apache 8.5K Aug 24 23:06 out627626.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat from image00003.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Image size: 927.0'x616.5' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:06.812 +54:04:03.85 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 14406 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/correct_sextractor_wcs_catalog_usingxy2sky628015.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1031, bad_region=2751, passed=14406
Got 14406 stars (including 10764 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat
util/solve_plate_with_UCAC5 got 14406 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.0'
Seting catalog search parameters based on the expected field of view 927.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012875 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010300 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0813 through 0 to 14.9386, gap 14.9386 to 345.0813
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3510 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2190 matched stars entering correct_measured_positions(), 2426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2056 matched stars entering correct_measured_positions(), 12161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.78"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0800 through 0 to 14.9577, gap 14.9577 to 345.0800
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3614 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2477 matched stars entering correct_measured_positions(), 12161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.08"
Accuracy estimation diagnostic: 2411 matched stars entering correct_measured_positions(), 12221 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.92"
Excluding outliers - 2411 stars left (next iteration limit 2261)
SIP_REFIT: SIP order 2 trial: matched=2411 robust_rms=26.556 arcsec worst_quadrant_rms=29.179 arcsec
SIP_REFIT: SIP order 3 trial: matched=2411 robust_rms=25.702 arcsec worst_quadrant_rms=29.752 arcsec
SIP_REFIT: SIP order 5 trial: matched=2411 robust_rms=22.989 arcsec worst_quadrant_rms=29.277 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2411 robust_rms_before=32.402 arcsec robust_rms_before_corrected=19.270 arcsec robust_rms_after=26.556 arcsec worst_quadrant_rms_before=24.346 worst_quadrant_rms_after=29.179
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.346 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits N_match=2411 sigma_overall_arcsec=13.753 sigma_q1_arcsec=29.159 sigma_q2_arcsec=28.015 sigma_q3_arcsec=7.243 sigma_q4_arcsec=5.321 n_q1=540 n_q2=267 n_q3=945 n_q4=659 worst_quadrant_to_overall_ratio=2.120
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits): sigma 13.753->13.753, ratio 2.120->2.120; reverting to order 3
WCS_QUALITY_RETRY: 2nd new image (fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits) flagged: sigma=13.522 (ref avg 0.463), ratio=2.136 (ref avg 1.1085), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/lib/make_outxyls_for_astrometric_calibration found 13750 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out628247.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out628247.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 25.2395 (9.14909e+10), 7 match, 0 conflict, 20 distractors, 24 index.
RA,Dec = (0.0396189,54.066), pixel scale 5.93236 arcsec/pix.
Hit/miss: Hit/miss: ----++---+--+---+---+-----+(best)-------+-----------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out628247.solved to indicate this.
Field: out628247.xyls
Field center: (RA,Dec) = (0.040997, 54.066782) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:09.839, +54:04:00.416).
Field size: 15.6099 x 10.4363 degrees
Field rotation angle: up is 3.52812 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits' -> 'fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Aug 24 23:06 fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
-rw-r--r-- 1 apache apache 8.5K Aug 24 23:06 out628247.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits (fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out628247.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out628247.axy"...
Only searching for solutions within 15.4517 degrees of RA,Dec (0.042375,54.0676)
log-odds ratio 25.2395 (9.14909e+10), 7 match, 0 conflict, 20 distractors, 24 index.
RA,Dec = (0.0396189,54.066), pixel scale 5.93236 arcsec/pix.
Hit/miss: Hit/miss: ----++---+--+---+---+-----+(best)-------+-----------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out628247.solved to indicate this.
Field: out628247.xyls
Field center: (RA,Dec) = (0.040997, 54.066782) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:09.839, +54:04:00.416).
Field size: 15.6099 x 10.4363 degrees
Field rotation angle: up is 3.52812 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Aug 24 23:06 fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
-rw-r--r-- 1 apache apache 8.5K Aug 24 23:06 out628247.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat from image00004.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Image size: 927.1'x616.5' 15.5(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:10.170 +54:04:03.40 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 14306 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/correct_sextractor_wcs_catalog_usingxy2sky628650.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1032, bad_region=2742, passed=14306
Got 14306 stars (including 10673 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat
util/solve_plate_with_UCAC5 got 14306 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.1'
Seting catalog search parameters based on the expected field of view 927.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012876 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010301 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0815 through 0 to 14.9394, gap 14.9394 to 345.0815
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3509 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2210 matched stars entering correct_measured_positions(), 2448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.11"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2076 matched stars entering correct_measured_positions(), 12053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0803 through 0 to 14.9584, gap 14.9584 to 345.0803
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3637 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2477 matched stars entering correct_measured_positions(), 12053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.95"
Accuracy estimation diagnostic: 2416 matched stars entering correct_measured_positions(), 12088 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.93"
Excluding outliers - 2416 stars left (next iteration limit 2283)
SIP_REFIT: SIP order 2 trial: matched=2416 robust_rms=26.450 arcsec worst_quadrant_rms=29.135 arcsec
SIP_REFIT: SIP order 3 trial: matched=2416 robust_rms=25.779 arcsec worst_quadrant_rms=29.487 arcsec
SIP_REFIT: SIP order 5 trial: matched=2416 robust_rms=23.024 arcsec worst_quadrant_rms=29.536 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2416 robust_rms_before=32.453 arcsec robust_rms_before_corrected=19.397 arcsec robust_rms_after=26.450 arcsec worst_quadrant_rms_before=24.432 worst_quadrant_rms_after=29.135
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.432 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits N_match=2416 sigma_overall_arcsec=13.522 sigma_q1_arcsec=28.887 sigma_q2_arcsec=26.685 sigma_q3_arcsec=7.431 sigma_q4_arcsec=4.930 n_q1=546 n_q2=273 n_q3=936 n_q4=661 worst_quadrant_to_overall_ratio=2.136
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 2nd new image (fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits): sigma 13.522->13.522, ratio 2.136->2.136; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=13.753 -- 29.70x the reference average (0.463); plate solution may be of low accuracy
WARNING: 2nd new image has sigma_overall_arcsec=13.522 -- 29.21x the reference average (0.463); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246_astrometric_residuals.png (4904 matched stars from wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111_astrometric_residuals.png (4902 matched stars from wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096_astrometric_residuals.png (2411 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 11.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097_astrometric_residuals.png (2416 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 11.49 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:42.30 +50:06:40.6: 15.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:42.30 +50:06:40.6: 14.71 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out50514.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 50514_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 50514_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50524_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 50524_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 00:15:50.08 +57:32:36.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 16s
Prepared the HTML report for the field Cas-04-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 ####
23:21:42.30 +50:06:40.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.062 +54:00:02.05 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Image size: 927.0'x616.5' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:06.812 +54:04:03.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.062 +54:00:02.05
Second-epoch image center 00:00:06.812 +54:04:03.85
Angular distance between the image centers 0.0686 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Image size: 927.1'x616.5' 15.5(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:10.170 +54:04:03.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.062 +54:00:02.05
Second-epoch image center 00:00:10.170 +54:04:03.40
Angular distance between the image centers 0.0706 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 00:00:06.812 +54:04:03.85
Second-epoch second image center 00:00:10.170 +54:04:03.40
Angular distance between the image centers 0.00821 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits &> /tmp/tmp.WtKD05bopd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits &> /tmp/tmp.Q373p1qvDV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits &> /tmp/tmp.cP9kzdh9QK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits &> /tmp/tmp.jnGfKMPoo5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits and wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits and wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits and wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 173088 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.3601 to 15.3872 deg, Dec +47.7472 to +59.3472 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 345.3601 to 15.3872 deg, Dec 47.7472 to 59.3472 deg
Loaded 26306 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): 14017 out of 18860 total matches.
Matched with Tycho-2 18860 out of 173088 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.590200
a=0.000000 b=1.000000 c=22.590200
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 173088 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.3601 to 15.3872 deg, Dec +47.7472 to +59.3472 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 345.3601 to 15.3872 deg, Dec 47.7472 to 59.3472 deg
Loaded 26306 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): 14017 out of 18860 total matches.
Matched with Tycho-2 18860 out of 173088 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits (aperture=6.1)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 122631 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 344.8488 to 14.8386 deg, Dec +47.9552 to +59.2699 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 344.8488 to 14.8386 deg, Dec 47.9552 to 59.2699 deg
Loaded 25870 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): 15872 out of 18918 total matches.
Matched with Tycho-2 18918 out of 122631 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 208 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
3.3 pix Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
2.1 pix Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
2.2 pix fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
2.2 pix fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Limiting magnitude estimates:
15.0 mag. Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
14.5 mag. Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
14.4 mag. fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
14.4 mag. fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.WtKD05bopd (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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.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-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits' -> 'wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=24691, bad_region=28985, passed=173052
Got 173052 stars (including 122564 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
util/solve_plate_with_UCAC5 got 173052 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
RA wraps around 0/360 boundary: field RA 345.3601 through 0 to 15.3872, gap 15.3872 to 345.3601
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 4916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 150954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3595 through 0 to 15.3874, gap 15.3874 to 345.3595
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 150954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 150954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4916 stars left (next iteration limit 5407)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits N_match=4916 sigma_overall_arcsec=0.384 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.384 sigma_q3_arcsec=0.346 sigma_q4_arcsec=0.350 n_q1=1555 n_q2=812 n_q3=1627 n_q4=922 worst_quadrant_to_overall_ratio=1.167
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits -region wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Q373p1qvDV (6) ############
Parsing command line arguments...
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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.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-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits' -> 'wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=11094, bad_region=15504, passed=122612
Got 122612 stars (including 97170 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat
util/solve_plate_with_UCAC5 got 122612 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8488 through 0 to 14.8386, gap 14.8386 to 344.8488
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 4916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 111480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8482 through 0 to 14.8387, gap 14.8387 to 344.8482
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 111480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 111480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4915 stars left (next iteration limit 5407)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits N_match=4915 sigma_overall_arcsec=0.511 sigma_q1_arcsec=0.492 sigma_q2_arcsec=0.440 sigma_q3_arcsec=0.574 sigma_q4_arcsec=0.515 n_q1=1598 n_q2=785 n_q3=1561 n_q4=971 worst_quadrant_to_overall_ratio=1.121
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits -region wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.cP9kzdh9QK (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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=9919, bad_region=13321, passed=113350
Got 113350 stars (including 91332 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat
util/solve_plate_with_UCAC5 got 113350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.0'
Seting catalog search parameters based on the expected field of view 927.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012875 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010300 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0547 through 0 to 15.0212, gap 15.0212 to 345.0547
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3502 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2193 matched stars entering correct_measured_positions(), 2426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.93"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2048 matched stars entering correct_measured_positions(), 102893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0534 through 0 to 15.0417, gap 15.0417 to 345.0534
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3587 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2480 matched stars entering correct_measured_positions(), 102894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.40"
Accuracy estimation diagnostic: 2422 matched stars entering correct_measured_positions(), 103043 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.76"
Excluding outliers - 2422 stars left (next iteration limit 2252)
SIP_REFIT: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=2422 robust_rms=26.241 arcsec worst_quadrant_rms=28.520 arcsec
SIP_REFIT: SIP order 3 trial: matched=2422 robust_rms=25.180 arcsec worst_quadrant_rms=29.950 arcsec
SIP_REFIT: SIP order 5 trial: matched=2422 robust_rms=22.710 arcsec worst_quadrant_rms=29.217 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2422 robust_rms_before=32.417 arcsec robust_rms_before_corrected=19.012 arcsec robust_rms_after=26.241 arcsec worst_quadrant_rms_before=24.033 worst_quadrant_rms_after=28.520
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.033 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits N_match=2422 sigma_overall_arcsec=12.898 sigma_q1_arcsec=29.253 sigma_q2_arcsec=26.636 sigma_q3_arcsec=6.582 sigma_q4_arcsec=4.927 n_q1=571 n_q2=277 n_q3=904 n_q4=670 worst_quadrant_to_overall_ratio=2.268
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.jnGfKMPoo5 (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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=9821, bad_region=13417, passed=112357
Got 112357 stars (including 90362 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat
util/solve_plate_with_UCAC5 got 112357 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.1'
Seting catalog search parameters based on the expected field of view 927.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012876 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010301 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0645 through 0 to 15.0256, gap 15.0256 to 345.0645
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3494 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2185 matched stars entering correct_measured_positions(), 2440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.97"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2058 matched stars entering correct_measured_positions(), 101937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.16"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0633 through 0 to 15.0467, gap 15.0467 to 345.0633
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3612 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2511 matched stars entering correct_measured_positions(), 101937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.19"
Accuracy estimation diagnostic: 2460 matched stars entering correct_measured_positions(), 102031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.55"
Excluding outliers - 2460 stars left (next iteration limit 2263)
SIP_REFIT: wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=2460 robust_rms=25.879 arcsec worst_quadrant_rms=28.699 arcsec
SIP_REFIT: SIP order 3 trial: matched=2460 robust_rms=24.826 arcsec worst_quadrant_rms=29.636 arcsec
SIP_REFIT: SIP order 5 trial: matched=2460 robust_rms=22.507 arcsec worst_quadrant_rms=29.140 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2460 robust_rms_before=32.934 arcsec robust_rms_before_corrected=18.956 arcsec robust_rms_after=25.879 arcsec worst_quadrant_rms_before=24.112 worst_quadrant_rms_after=28.699
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.112 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits N_match=2460 sigma_overall_arcsec=12.061 sigma_q1_arcsec=29.155 sigma_q2_arcsec=27.692 sigma_q3_arcsec=6.818 sigma_q4_arcsec=4.745 n_q1=579 n_q2=272 n_q3=907 n_q4=702 worst_quadrant_to_overall_ratio=2.417
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-55-32_20.00sec_0.00C_LIGHT_0096.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.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_2026-08-24_CI_Cas-04-Q2b1x1_230135_TTUQ2b1x1_567265_v8KcvnMV/wcs_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:59:20.27 +56:34:35.6: 14.25 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:10:16.89 +56:50:56.7: 13.55 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:11.69 +53:34:43.9: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:20.83 +50:22:17.8: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:09.34 +52:44:37.3: 14.22 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:48.31 +53:36:52.0: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:56:48.29 +50:59:51.1: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:20.83 +50:22:17.8: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:09.34 +52:44:37.3: 14.48 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:59:20.27 +56:34:35.6: 15.07 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:11.69 +53:34:43.9: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:10:16.89 +56:50:56.7: 14.34 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:48.31 +53:36:52.0: 15.04 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.26 +/- 0.10
Forced photometry reference-image weighted average: 13.61 +/- 0.05
Forced photometry reference-image weighted average: 14.31 +/- 0.10
Forced photometry filter REJECTED candidate at 23:36:09.34 +52:44:37.3: ref_mag=14.26 +/- 0.10 new_mean_mag=14.2416 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:10:16.89 +56:50:56.7: ref_mag=13.61 +/- 0.05 new_mean_mag=14.0353 delta=-0.42 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:59:20.27 +56:34:35.6: ref_mag=14.31 +/- 0.10 new_mean_mag=14.1150 delta=0.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:56:48.29 +50:59:51.1: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:00.35 +54:34:36.3: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:57.28 +55:44:19.7: 13.53 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:16:48.67 +56:44:39.5: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:00.35 +54:34:36.3: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:57.28 +55:44:19.7: 13.89 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.05
Forced photometry filter REJECTED candidate at 23:48:57.28 +55:44:19.7: ref_mag=13.58 +/- 0.05 new_mean_mag=14.1772 delta=-0.60 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:16:48.67 +56:44:39.5: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:56:08.62 +54:25:46.6: 13.84 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:53.47 +56:52:26.5: 13.56 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:50:57.87 +53:34:45.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:56:08.62 +54:25:46.6: 14.14 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.06
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:53.47 +56:52:26.5: 13.72 +/- 0.11 detection
Forced photometry filter REJECTED candidate at 23:56:08.62 +54:25:46.6: ref_mag=13.89 +/- 0.06 new_mean_mag=14.0728 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.60 +/- 0.05
Forced photometry filter REJECTED candidate at 23:48:53.47 +56:52:26.5: ref_mag=13.60 +/- 0.05 new_mean_mag=13.8452 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:50:58.57 +55:52:06.1: 13.85 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:50:57.87 +53:34:45.9: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:50:58.57 +55:52:06.1: 14.46 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.07
Forced photometry filter REJECTED candidate at 23:50:58.57 +55:52:06.1: ref_mag=13.91 +/- 0.07 new_mean_mag=14.1071 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:52:43.77 +51:16:38.3: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:52:43.77 +51:16:38.3: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:59:56.29 +54:25:44.0: 13.79 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:17.74 +56:04:19.7: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:59:56.29 +54:25:44.0: 14.08 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.06
Forced photometry filter REJECTED candidate at 23:59:56.29 +54:25:44.0: ref_mag=13.84 +/- 0.06 new_mean_mag=14.1220 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:17.74 +56:04:19.7: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:53:57.80 +53:13:27.7: 13.44 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:53:57.80 +53:13:27.7: 13.99 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.05
Forced photometry filter REJECTED candidate at 23:53:57.80 +53:13:27.7: ref_mag=13.49 +/- 0.05 new_mean_mag=14.0606 delta=-0.57 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:15:17.00 +51:40:37.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:15:17.00 +51:40:37.0: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:56:14.87 +55:22:34.2: 13.54 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:56:14.87 +55:22:34.2: 13.70 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Forced photometry filter REJECTED candidate at 23:56:14.87 +55:22:34.2: ref_mag=13.57 +/- 0.04 new_mean_mag=13.8577 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:22.56 +55:42:27.7: 12.41 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:22.56 +55:42:27.7: 12.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.02
Forced photometry filter REJECTED candidate at 23:26:22.56 +55:42:27.7: ref_mag=12.46 +/- 0.02 new_mean_mag=13.9929 delta=-1.53 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:25.43 +56:44:43.8: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:25.43 +56:44:43.8: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:03:08.41 +50:52:37.6: 14.94 +/- 0.17 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:03:08.41 +50:52:37.6: 15.06 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.94 +/- 0.17
Forced photometry filter REJECTED candidate at 00:03:08.41 +50:52:37.6: ref_mag=14.94 +/- 0.17 new_mean_mag=14.0845 delta=0.85 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:37.60 +51:04:21.3: 15.64 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:37.60 +51:04:21.3: 14.98 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.64 +/- 0.36
Forced photometry filter KEPT candidate at 23:35:37.60 +51:04:21.3: ref_mag=15.64 +/- 0.36 new_mean_mag=13.9742 delta=1.66 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:07.22 +54:09:29.1: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:53.90 +56:58:13.9: 13.83 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:53.90 +56:58:13.9: 13.88 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.07
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:07.22 +54:09:29.1: 15.05 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:45:53.90 +56:58:13.9: ref_mag=13.84 +/- 0.07 new_mean_mag=13.9791 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:55.60 +52:52:54.9: 12.37 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:52:01.56 +58:17:48.2: 13.31 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:02.50 +54:32:47.6: 13.91 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:55.60 +52:52:54.9: 12.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.02
Forced photometry filter REJECTED candidate at 23:30:55.60 +52:52:54.9: ref_mag=12.43 +/- 0.02 new_mean_mag=13.8191 delta=-1.39 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:52:01.56 +58:17:48.2: 13.46 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Forced photometry filter REJECTED candidate at 23:52:01.56 +58:17:48.2: ref_mag=13.34 +/- 0.04 new_mean_mag=13.6752 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:02.50 +54:32:47.6: 14.19 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.06
Forced photometry filter REJECTED candidate at 23:58:02.50 +54:32:47.6: ref_mag=13.95 +/- 0.06 new_mean_mag=14.0273 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:13:12.30 +58:10:33.5: 13.52 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:55.58 +50:00:11.9: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:13:12.30 +58:10:33.5: 13.62 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.05
Forced photometry filter REJECTED candidate at 00:13:12.30 +58:10:33.5: ref_mag=13.54 +/- 0.05 new_mean_mag=13.9254 delta=-0.38 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:55.58 +50:00:11.9: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:53.84 +54:25:05.1: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:53:27.95 +56:05:37.8: 13.53 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:41.24 +50:39:38.4: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:54:51.62 +55:45:26.0: 13.46 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:53.84 +54:25:05.1: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:53:27.95 +56:05:37.8: 13.92 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.05
Forced photometry filter REJECTED candidate at 23:53:27.95 +56:05:37.8: ref_mag=13.59 +/- 0.05 new_mean_mag=13.8400 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:41:49.04 +51:06:39.5: 15.60 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:41.24 +50:39:38.4: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:54:51.62 +55:45:26.0: 13.54 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Forced photometry filter REJECTED candidate at 23:54:51.62 +55:45:26.0: ref_mag=13.48 +/- 0.04 new_mean_mag=13.9943 delta=-0.52 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:41:49.04 +51:06:39.5: 15.03 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.60 +/- 0.34
Forced photometry filter KEPT candidate at 23:41:49.04 +51:06:39.5: ref_mag=15.60 +/- 0.34 new_mean_mag=13.7707 delta=1.82 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:20.79 +54:05:10.8: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:13:01.82 +53:50:13.6: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:20.79 +54:05:10.8: 12.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry filter REJECTED candidate at 23:58:20.79 +54:05:10.8: ref_mag=12.62 +/- 0.02 new_mean_mag=13.9692 delta=-1.35 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:13:01.82 +53:50:13.6: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:29.26 +56:49:05.4: 13.25 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:54.07 +49:51:21.3: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:29.26 +56:49:05.4: 13.40 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.05
Forced photometry filter REJECTED candidate at 23:57:29.26 +56:49:05.4: ref_mag=13.30 +/- 0.05 new_mean_mag=13.6781 delta=-0.38 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:54.07 +49:51:21.3: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:15.71 +56:00:21.2: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:15.71 +56:00:21.2: 13.32 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Forced photometry filter REJECTED candidate at 23:48:15.71 +56:00:21.2: ref_mag=13.17 +/- 0.03 new_mean_mag=13.7262 delta=-0.55 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:00:34.95 +51:13:14.6: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:10.63 +58:01:34.7: 13.59 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:00:34.95 +51:13:14.6: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:10.63 +58:01:34.7: 13.90 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.05
Forced photometry filter REJECTED candidate at 23:36:10.63 +58:01:34.7: ref_mag=13.64 +/- 0.05 new_mean_mag=13.7467 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:17.43 +54:23:31.1: 13.43 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:17.43 +54:23:31.1: 13.66 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Forced photometry filter REJECTED candidate at 23:57:17.43 +54:23:31.1: ref_mag=13.47 +/- 0.04 new_mean_mag=13.8679 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:49:32.70 +55:08:08.3: 13.66 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:49:32.70 +55:08:08.3: 14.11 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.05
Forced photometry filter REJECTED candidate at 23:49:32.70 +55:08:08.3: ref_mag=13.71 +/- 0.05 new_mean_mag=13.8326 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:02.53 +54:13:44.5: 13.32 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:02.53 +54:13:44.5: 13.56 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.04
Forced photometry filter REJECTED candidate at 23:58:02.53 +54:13:44.5: ref_mag=13.36 +/- 0.04 new_mean_mag=13.5584 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:45.90 +55:44:41.8: 14.73 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:59:24.33 +55:24:56.7: 13.39 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:45.90 +55:44:41.8: 14.76 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.73 +/- 0.19
Forced photometry filter KEPT candidate at 23:15:45.90 +55:44:41.8: ref_mag=14.73 +/- 0.19 new_mean_mag=13.8248 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:59:24.33 +55:24:56.7: 13.52 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.04
Forced photometry filter REJECTED candidate at 23:59:24.33 +55:24:56.7: ref_mag=13.41 +/- 0.04 new_mean_mag=13.7181 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:48.32 +54:40:28.6: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:48.32 +54:40:28.6: 15.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:51.06 +50:20:13.9: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:51.06 +50:20:13.9: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:41:22.93 +57:23:24.1: 13.23 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:29.04 +54:37:38.2: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:41:22.93 +57:23:24.1: 13.50 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.04
Forced photometry filter REJECTED candidate at 23:41:22.93 +57:23:24.1: ref_mag=13.28 +/- 0.04 new_mean_mag=13.7015 delta=-0.42 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:29.04 +54:37:38.2: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:03:28.92 +57:18:39.4: 13.13 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:03:28.92 +57:18:39.4: 13.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Forced photometry filter REJECTED candidate at 00:03:28.92 +57:18:39.4: ref_mag=13.18 +/- 0.03 new_mean_mag=13.6123 delta=-0.43 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:42.20 +58:00:40.6: 15.01 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:42.20 +58:00:40.6: 14.87 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.01 +/- 0.24
Forced photometry filter KEPT candidate at 23:30:42.20 +58:00:40.6: ref_mag=15.01 +/- 0.24 new_mean_mag=13.7159 delta=1.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:33.49 +50:54:12.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:33.49 +50:54:12.9: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:27.57 +52:16:04.1: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:27.57 +52:16:04.1: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:41.95 +50:08:56.4: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:41.95 +50:08:56.4: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:50.17 +57:10:37.8: 12.65 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:50.17 +57:10:37.8: 12.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry filter REJECTED candidate at 23:38:50.17 +57:10:37.8: ref_mag=12.68 +/- 0.02 new_mean_mag=13.5423 delta=-0.86 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:23:12.05 +56:00:07.1: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:46:33.71 +53:16:40.3: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:23:12.05 +56:00:07.1: 15.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:46:33.71 +53:16:40.3: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:32.83 +54:53:57.6: 14.88 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:32.83 +54:53:57.6: 14.92 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.88 +/- 0.20
Forced photometry filter KEPT candidate at 23:30:32.83 +54:53:57.6: ref_mag=14.88 +/- 0.20 new_mean_mag=13.4976 delta=1.38 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:43.46 +52:15:31.1: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:43.46 +52:15:31.1: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:31.08 +51:50:03.3: 15.04 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:31.08 +51:50:03.3: 15.05 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.04 +/- 0.21
Forced photometry filter KEPT candidate at 00:09:31.08 +51:50:03.3: ref_mag=15.04 +/- 0.21 new_mean_mag=13.6662 delta=1.37 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:49:54.36 +55:54:36.3: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:49:54.36 +55:54:36.3: 13.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Forced photometry filter REJECTED candidate at 23:49:54.36 +55:54:36.3: ref_mag=13.10 +/- 0.03 new_mean_mag=13.5676 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:27:15.89 +53:26:57.0: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:13.31 +54:31:38.2: 14.96 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:27:15.89 +53:26:57.0: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:13.31 +54:31:38.2: 14.85 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.96 +/- 0.24
Forced photometry filter KEPT candidate at 23:18:13.31 +54:31:38.2: ref_mag=14.96 +/- 0.24 new_mean_mag=13.5489 delta=1.41 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:41.59 +54:06:31.8: 14.43 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:41.59 +54:06:31.8: 14.42 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.12
Forced photometry filter REJECTED candidate at 23:27:41.59 +54:06:31.8: ref_mag=14.43 +/- 0.12 new_mean_mag=13.5293 delta=0.90 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:58.53 +55:22:27.7: 12.84 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:05.88 +57:56:19.4: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:58.53 +55:22:27.7: 13.61 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:06.43 +54:30:24.1: 15.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.89 +/- 0.03
Forced photometry filter REJECTED candidate at 23:57:58.53 +55:22:27.7: ref_mag=12.89 +/- 0.03 new_mean_mag=13.5427 delta=-0.65 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:29:05.88 +57:56:19.4: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:06.43 +54:30:24.1: 15.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:16.98 +54:09:21.5: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:34.53 +56:42:25.9: 12.09 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:16.98 +54:09:21.5: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:34.53 +56:42:25.9: 13.27 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.02
Forced photometry filter REJECTED candidate at 23:32:34.53 +56:42:25.9: ref_mag=12.13 +/- 0.02 new_mean_mag=13.4560 delta=-1.33 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:08:58.81 +54:18:07.5: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:47:47.07 +57:09:49.3: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:08:58.81 +54:18:07.5: 13.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Forced photometry filter REJECTED candidate at 00:08:58.81 +54:18:07.5: ref_mag=13.18 +/- 0.03 new_mean_mag=13.4266 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:47:47.07 +57:09:49.3: 12.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Forced photometry filter REJECTED candidate at 23:47:47.07 +57:09:49.3: ref_mag=12.85 +/- 0.03 new_mean_mag=13.3971 delta=-0.54 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:15.75 +56:01:37.7: 14.82 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:51.41 +51:51:10.9: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:15.75 +56:01:37.7: 14.77 +/- 0.31 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.16
Forced photometry filter KEPT candidate at 23:38:15.75 +56:01:37.7: ref_mag=14.80 +/- 0.16 new_mean_mag=13.0812 delta=1.72 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:45.72 +54:32:02.1: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:51.41 +51:51:10.9: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:45.72 +54:32:02.1: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:56:56.02 +58:18:44.8: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:56:56.02 +58:18:44.8: 13.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.03
Forced photometry filter REJECTED candidate at 23:56:56.02 +58:18:44.8: ref_mag=12.88 +/- 0.03 new_mean_mag=13.2223 delta=-0.35 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:44.14 +52:38:24.8: 12.72 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:44.14 +52:38:24.8: 13.31 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.03
Forced photometry filter REJECTED candidate at 23:20:44.14 +52:38:24.8: ref_mag=12.78 +/- 0.03 new_mean_mag=12.9877 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:42.73 +57:16:04.9: 12.40 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:42.73 +57:16:04.9: 12.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Forced photometry filter REJECTED candidate at 23:39:42.73 +57:16:04.9: ref_mag=12.45 +/- 0.02 new_mean_mag=12.9979 delta=-0.55 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:45.45 +51:01:20.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:56.89 +55:27:53.2: 14.90 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:45.45 +51:01:20.1: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:56.89 +55:27:53.2: 14.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.90 +/- 0.22
Forced photometry filter KEPT candidate at 23:12:56.89 +55:27:53.2: ref_mag=14.90 +/- 0.22 new_mean_mag=13.0362 delta=1.86 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:22:59.41 +53:53:10.9: 12.89 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:48.29 +56:18:33.6: 15.49 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:22:59.41 +53:53:10.9: 13.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.03
Forced photometry filter REJECTED candidate at 00:22:59.41 +53:53:10.9: ref_mag=12.93 +/- 0.03 new_mean_mag=12.9605 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:48.29 +56:18:33.6: 14.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.49 +/- 0.35
Forced photometry filter KEPT candidate at 23:27:48.29 +56:18:33.6: ref_mag=15.49 +/- 0.35 new_mean_mag=12.8930 delta=2.60 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:00.50 +51:29:24.8: 15.53 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:00.50 +51:29:24.8: 15.12 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.53 +/- 0.31
Forced photometry filter KEPT candidate at 23:42:00.50 +51:29:24.8: ref_mag=15.53 +/- 0.31 new_mean_mag=12.7913 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:10.64 +55:53:37.8: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:10.64 +55:53:37.8: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:56:30.84 +56:44:23.7: 12.49 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:56:30.84 +56:44:23.7: 12.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.03
Forced photometry filter REJECTED candidate at 23:56:30.84 +56:44:23.7: ref_mag=12.56 +/- 0.03 new_mean_mag=12.8442 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:16.49 +51:00:10.5: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:16.49 +51:00:10.5: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:18.08 +56:40:25.9: 15.31 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:18.08 +56:40:25.9: 14.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.31 +/- 0.29
Forced photometry filter KEPT candidate at 23:27:18.08 +56:40:25.9: ref_mag=15.31 +/- 0.29 new_mean_mag=12.5041 delta=2.81 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:54:49.11 +55:06:22.2: 11.86 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:54:49.11 +55:06:22.2: 12.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter REJECTED candidate at 23:54:49.11 +55:06:22.2: ref_mag=11.90 +/- 0.01 new_mean_mag=12.3645 delta=-0.46 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:09.66 +52:54:18.0: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:09.66 +52:54:18.0: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:03:24.36 +55:40:55.8: 10.89 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:03:24.36 +55:40:55.8: 11.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.01
Forced photometry filter REJECTED candidate at 00:03:24.36 +55:40:55.8: ref_mag=10.93 +/- 0.01 new_mean_mag=11.6946 delta=-0.76 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:59:24.38 +50:35:23.0: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:59:24.38 +50:35:23.0: 15.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:58.95 +56:18:50.6: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:58.95 +56:18:50.6: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:03.66 +49:30:57.1: 15.13 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:03.66 +49:30:57.1: 14.83 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.13 +/- 0.27
Forced photometry filter KEPT candidate at 23:20:03.66 +49:30:57.1: ref_mag=15.13 +/- 0.27 new_mean_mag=12.5720 delta=2.56 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:14:48.20 +54:45:40.1: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:48.20 +54:45:40.1: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:49.57 +57:05:36.5: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:49.57 +57:05:36.5: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:53:37.56 +56:59:07.4: 12.87 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:53:37.56 +56:59:07.4: 12.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.03
Forced photometry filter REJECTED candidate at 23:53:37.56 +56:59:07.4: ref_mag=12.86 +/- 0.03 new_mean_mag=12.9948 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:27.99 +57:57:27.1: 13.51 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:27.99 +57:57:27.1: 13.23 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.05
Forced photometry filter REJECTED candidate at 23:30:27.99 +57:57:27.1: ref_mag=13.43 +/- 0.05 new_mean_mag=13.1651 delta=0.26 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:53.65 +49:58:04.2: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:26:59.42 +51:56:16.5: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:53.65 +49:58:04.2: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:26:59.42 +51:56:16.5: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:44.42 +54:27:02.2: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:44.42 +54:27:02.2: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:08.76 +51:57:12.2: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:08.76 +51:57:12.2: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:04.74 +51:43:27.8: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:04.74 +51:43:27.8: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:50:03.14 +53:38:14.1: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:50:03.14 +53:38:14.1: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:58.78 +56:58:22.9: 13.36 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:58.78 +56:58:22.9: 13.59 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.05
Forced photometry filter REJECTED candidate at 23:58:58.78 +56:58:22.9: ref_mag=13.40 +/- 0.05 new_mean_mag=13.6765 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:13.73 +57:42:57.7: 13.54 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:49.67 +57:56:19.8: 13.51 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:13.73 +57:42:57.7: 13.74 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.05
Forced photometry filter REJECTED candidate at 23:48:13.73 +57:42:57.7: ref_mag=13.58 +/- 0.05 new_mean_mag=13.6932 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:49.67 +57:56:19.8: 13.84 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.05
Forced photometry filter REJECTED candidate at 23:48:49.67 +57:56:19.8: ref_mag=13.56 +/- 0.05 new_mean_mag=13.7748 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:49:49.46 +52:31:08.4: 15.40 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:41:00.12 +56:50:57.5: 13.51 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:49:49.46 +52:31:08.4: 15.06 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.40 +/- 0.29
Forced photometry filter KEPT candidate at 23:49:49.46 +52:31:08.4: ref_mag=15.40 +/- 0.29 new_mean_mag=13.6409 delta=1.76 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:41:00.12 +56:50:57.5: 13.71 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.05
Forced photometry filter REJECTED candidate at 23:41:00.12 +56:50:57.5: ref_mag=13.55 +/- 0.05 new_mean_mag=13.6552 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:51.31 +52:53:33.2: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:10.88 +52:08:38.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:51.31 +52:53:33.2: 15.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:10.88 +52:08:38.1: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:03:27.70 +55:39:38.7: 13.43 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:03:27.70 +55:39:38.7: 13.51 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.05
Forced photometry filter REJECTED candidate at 00:03:27.70 +55:39:38.7: ref_mag=13.45 +/- 0.05 new_mean_mag=13.7525 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:51:09.98 +51:25:55.4: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:51:09.98 +51:25:55.4: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:02.40 +58:05:55.6: 13.44 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:02.40 +58:05:55.6: 14.03 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.05
Forced photometry filter REJECTED candidate at 23:45:02.40 +58:05:55.6: ref_mag=13.50 +/- 0.05 new_mean_mag=13.8103 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:54.22 +56:41:21.5: 14.26 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:04.29 +55:46:00.3: 15.05 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:19.74 +56:17:53.3: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:54.22 +56:41:21.5: 13.75 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.14
Forced photometry filter REJECTED candidate at 23:57:54.22 +56:41:21.5: ref_mag=13.93 +/- 0.14 new_mean_mag=13.9892 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:04.29 +55:46:00.3: 14.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.05 +/- 0.23
Forced photometry filter KEPT candidate at 23:38:04.29 +55:46:00.3: ref_mag=15.05 +/- 0.23 new_mean_mag=13.8183 delta=1.24 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:19.74 +56:17:53.3: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:14.58 +51:03:06.3: 11.59 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:14.58 +51:03:06.3: 13.26 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.01
Forced photometry filter REJECTED candidate at 23:30:14.58 +51:03:06.3: ref_mag=11.61 +/- 0.01 new_mean_mag=14.0676 delta=-2.46 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:19.19 +58:00:13.8: 14.04 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:19.19 +58:00:13.8: 14.22 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.08
Forced photometry filter REJECTED candidate at 23:45:19.19 +58:00:13.8: ref_mag=14.07 +/- 0.08 new_mean_mag=14.1212 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:16.12 +51:29:31.0: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:16.12 +51:29:31.0: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:05.12 +57:14:03.1: 13.93 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:05.12 +57:14:03.1: 13.79 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.07
Forced photometry filter REJECTED candidate at 23:45:05.12 +57:14:03.1: ref_mag=13.89 +/- 0.07 new_mean_mag=14.2501 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:52.68 +50:22:58.9: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:52.68 +50:22:58.9: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:54:13.79 +54:55:36.1: 14.41 +/- 0.11 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:54:13.79 +54:55:36.1: 14.19 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.09
Forced photometry filter REJECTED candidate at 23:54:13.79 +54:55:36.1: ref_mag=14.33 +/- 0.09 new_mean_mag=14.0398 delta=0.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:14.30 +53:13:15.9: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:14.30 +53:13:15.9: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:50:07.17 +56:25:12.8: 14.52 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:50:07.17 +56:25:12.8: 14.55 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.12
Forced photometry filter REJECTED candidate at 23:50:07.17 +56:25:12.8: ref_mag=14.52 +/- 0.12 new_mean_mag=14.2184 delta=0.30 (need > 0.90)
Adding exclusion_list_local.txt__out189568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190594.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 120s
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: 43s
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Considering the candidate 189553_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189553_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189557_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189557_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 189562_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189562_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189563_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189563_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 189568_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189568_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189571_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189571_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189576_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189576_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 00:00:20.63 +54:28:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189582_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189582_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189587_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189587_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189590_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189590_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189599_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189599_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 189607_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189607_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 189613_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189613_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 189614_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189614_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189622_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189622_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189623_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189623_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189625_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189625_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189629_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189629_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 189633_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189633_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189644_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189644_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189645_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189645_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189657_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189657_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 189662_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189662_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189665_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189665_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189666_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189666_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189672_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189672_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 189678_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189678_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189687_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189687_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189703_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189703_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 189704_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189704_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189705_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189705_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189706_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189706_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189716_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189716_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189722_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189722_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189725_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189725_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 189732_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189732_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189738_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189738_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189749_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189749_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 189752_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189752_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189756_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189756_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189757_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189757_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189759_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189759_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189769_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189769_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189771_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189771_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 00:01:58.46 +54:26:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189773_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189773_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189774_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189774_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189775_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189775_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189776_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189776_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189777_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189777_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189780_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189780_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 189782_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189782_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189789_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189789_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189790_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189790_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 23:41:29.37 +57:44:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189798_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189798_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189799_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189799_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189800_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189800_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189803_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189803_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 189807_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189807_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 189814_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189814_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189816_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189816_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189817_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189817_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189836_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189836_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189839_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189839_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189843_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189843_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189844_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189844_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189848_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189848_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 189852_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189852_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189854_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189854_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 189858_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189858_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189859_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189859_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189865_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189865_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189866_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189866_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 189868_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189868_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189870_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189870_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189871_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189871_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 189873_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189873_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189874_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189874_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 189878_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189878_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 189880_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189880_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189884_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189884_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 189885_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189885_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189887_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189887_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189890_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189890_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 23:56:21.70 +55:07:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189892_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189892_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189894_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189894_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189897_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189897_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 189904_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189904_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 189905_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189905_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 189910_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189910_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 189911_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189911_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189912_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189912_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (35.0") between the two second-epoch detections
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Considering the candidate 189915_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189915_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189923_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189923_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189925_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189925_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 189927_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189927_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189928_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189928_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189937_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189937_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 189944_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189944_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189945_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189945_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 189947_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189947_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189951_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189951_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (33.7") between the two second-epoch detections
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Considering the candidate 189952_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189952_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 189953_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189953_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 189955_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189955_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189956_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189956_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189961_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189961_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189962_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189962_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189965_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189965_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189966_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189966_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189967_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189967_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 189969_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189969_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 189975_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189975_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 23:57:13.26 +56:39:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189977_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189977_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 189979_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189979_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 189982_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189982_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 189983_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189983_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 189985_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189985_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 189986_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 189986_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 00:24:08.95 +57:10:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189990_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189990_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189996_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 189996_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190000_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190000_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 190001_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190001_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 00:09:58.18 +56:18:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190013_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190013_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 190017_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190017_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 190019_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190019_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
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Considering the candidate 190021_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190021_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190025_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190025_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 190029_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190029_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190031_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190031_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190032_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190032_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 00:03:55.24 +55:04:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190034_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190034_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190035_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190035_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 190037_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190037_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190038_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190038_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 190039_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190039_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 190046_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190046_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190053_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190053_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190055_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190055_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 00:02:52.87 +55:52:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190058_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190058_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190059_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190059_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190061_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190061_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 190064_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190064_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 190072_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190072_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190074_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190074_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 190115_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190115_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 190118_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190118_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190122_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190122_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (29.8") between the two second-epoch detections
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Considering the candidate 190123_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190123_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 23:42:05.18 +57:16:08.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190128_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190128_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190137_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190137_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 190142_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190142_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190144_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190144_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 190146_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190146_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
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Considering the candidate 190152_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190152_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190167_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190167_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 190171_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190171_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 190180_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190180_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190181_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190181_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 00:05:42.81 +58:17:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190182_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190182_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 190197_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190197_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
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Considering the candidate 190199_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190199_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 190200_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190200_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (46.0") between the two second-epoch detections
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Considering the candidate 190205_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190205_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 23:42:25.22 +56:49:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190208_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190208_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 190225_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190225_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 190237_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190237_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190244_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190244_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190247_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190247_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 190249_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190249_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 190262_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190262_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190265_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190265_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190267_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190267_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 23:41:17.06 +57:32:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190284_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190284_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190285_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190285_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190296_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190296_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190300_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190300_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190304_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190304_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190317_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190317_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190323_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190323_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190329_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190329_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190333_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190333_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190334_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190334_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190338_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190338_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190350_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190350_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190360_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190360_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190393_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190393_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190395_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190395_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190396_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190396_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190403_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190403_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190448_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190448_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190449_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190449_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190464_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190464_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190467_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190467_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190493_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190493_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190497_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190497_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190520_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190520_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190529_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190529_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190537_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190537_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190541_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190541_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190583_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190583_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190585_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190585_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190594_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
Preparing report for the candidate 190594_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190597_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190597_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190600_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190600_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190618_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 190618_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170697_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 170697_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 00:15:50.89 +57:32:39.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140319_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 140319_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16337_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097
The candidate 16337_fd_Cas-04-Q2b1x1_2026-08-24_22-56-16_20.00sec_-0.00C_LIGHT_0097 did not pass the final checks
**** FOUND 23:21:42.41 +50:06:42.9 in the exclusion list exclusion_list_local.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-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:21:42.30 +50:06:40.6
23:56:48.29 +50:59:51.1
23:38:48.31 +53:36:52.0
23:30:20.83 +50:22:17.8
23:28:11.69 +53:34:43.9
00:09:00.35 +54:34:36.3
23:16:48.67 +56:44:39.5
23:50:57.87 +53:34:45.9
23:52:43.77 +51:16:38.3
23:17:17.74 +56:04:19.7
00:15:17.00 +51:40:37.0
23:27:25.43 +56:44:43.8
23:35:37.60 +51:04:21.3
23:34:07.22 +54:09:29.1
23:57:55.58 +50:00:11.9
23:42:53.84 +54:25:05.1
23:24:41.24 +50:39:38.4
23:41:49.04 +51:06:39.5
00:13:01.82 +53:50:13.6
23:19:54.07 +49:51:21.3
00:00:34.95 +51:13:14.6
23:15:45.90 +55:44:41.8
00:07:48.32 +54:40:28.6
23:26:51.06 +50:20:13.9
23:45:29.04 +54:37:38.2
23:30:42.20 +58:00:40.6
00:05:33.49 +50:54:12.9
23:58:27.57 +52:16:04.1
23:22:41.95 +50:08:56.4
00:23:12.05 +56:00:07.1
23:46:33.71 +53:16:40.3
23:30:32.83 +54:53:57.6
23:20:43.46 +52:15:31.1
00:09:31.08 +51:50:03.3
00:27:15.89 +53:26:57.0
23:18:13.31 +54:31:38.2
23:29:05.88 +57:56:19.4
00:05:06.43 +54:30:24.1
23:18:16.98 +54:09:21.5
23:38:15.75 +56:01:37.7
23:37:51.41 +51:51:10.9
23:20:45.72 +54:32:02.1
23:39:45.45 +51:01:20.1
23:12:56.89 +55:27:53.2
23:27:48.29 +56:18:33.6
23:42:00.50 +51:29:24.8
23:21:10.64 +55:53:37.8
00:07:16.49 +51:00:10.5
23:27:18.08 +56:40:25.9
23:32:09.66 +52:54:18.0
23:59:24.38 +50:35:23.0
23:12:58.95 +56:18:50.6
23:20:03.66 +49:30:57.1
23:14:48.20 +54:45:40.1
23:12:49.57 +57:05:36.5
23:30:53.65 +49:58:04.2
00:26:59.42 +51:56:16.5
23:21:44.42 +54:27:02.2
23:33:08.76 +51:57:12.2
00:09:04.74 +51:43:27.8
23:50:03.14 +53:38:14.1
23:49:49.46 +52:31:08.4
23:48:51.31 +52:53:33.2
00:05:10.88 +52:08:38.1
23:51:09.98 +51:25:55.4
23:38:04.29 +55:46:00.3
23:33:19.74 +56:17:53.3
23:37:16.12 +51:29:31.0
23:37:52.68 +50:22:58.9
23:42:14.30 +53:13:15.9
########### Completed Cas-04-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 ####
23:21:42.30 +50:06:40.6
23:56:48.29 +50:59:51.1
23:38:48.31 +53:36:52.0
23:30:20.83 +50:22:17.8
23:28:11.69 +53:34:43.9
00:09:00.35 +54:34:36.3
23:16:48.67 +56:44:39.5
23:50:57.87 +53:34:45.9
23:52:43.77 +51:16:38.3
23:17:17.74 +56:04:19.7
00:15:17.00 +51:40:37.0
23:27:25.43 +56:44:43.8
23:35:37.60 +51:04:21.3
23:34:07.22 +54:09:29.1
23:57:55.58 +50:00:11.9
23:42:53.84 +54:25:05.1
23:24:41.24 +50:39:38.4
23:41:49.04 +51:06:39.5
00:13:01.82 +53:50:13.6
23:19:54.07 +49:51:21.3
00:00:34.95 +51:13:14.6
23:15:45.90 +55:44:41.8
00:07:48.32 +54:40:28.6
23:26:51.06 +50:20:13.9
23:45:29.04 +54:37:38.2
23:30:42.20 +58:00:40.6
00:05:33.49 +50:54:12.9
23:58:27.57 +52:16:04.1
23:22:41.95 +50:08:56.4
00:23:12.05 +56:00:07.1
23:46:33.71 +53:16:40.3
23:30:32.83 +54:53:57.6
23:20:43.46 +52:15:31.1
00:09:31.08 +51:50:03.3
00:27:15.89 +53:26:57.0
23:18:13.31 +54:31:38.2
23:29:05.88 +57:56:19.4
00:05:06.43 +54:30:24.1
23:18:16.98 +54:09:21.5
23:38:15.75 +56:01:37.7
23:37:51.41 +51:51:10.9
23:20:45.72 +54:32:02.1
23:39:45.45 +51:01:20.1
23:12:56.89 +55:27:53.2
23:27:48.29 +56:18:33.6
23:42:00.50 +51:29:24.8
23:21:10.64 +55:53:37.8
00:07:16.49 +51:00:10.5
23:27:18.08 +56:40:25.9
23:32:09.66 +52:54:18.0
23:59:24.38 +50:35:23.0
23:12:58.95 +56:18:50.6
23:20:03.66 +49:30:57.1
23:14:48.20 +54:45:40.1
23:12:49.57 +57:05:36.5
23:30:53.65 +49:58:04.2
00:26:59.42 +51:56:16.5
23:21:44.42 +54:27:02.2
23:33:08.76 +51:57:12.2
00:09:04.74 +51:43:27.8
23:50:03.14 +53:38:14.1
23:49:49.46 +52:31:08.4
23:48:51.31 +52:53:33.2
00:05:10.88 +52:08:38.1
23:51:09.98 +51:25:55.4
23:38:04.29 +55:46:00.3
23:33:19.74 +56:17:53.3
23:37:16.12 +51:29:31.0
23:37:52.68 +50:22:58.9
23:42:14.30 +53:13:15.9
###################################################################################
23:21:42.30 +50:06:40.6 -- not an asteroid (will add it to exclusion list)
23:56:48.29 +50:59:51.1 -- not an asteroid (will add it to exclusion list)
23:38:48.31 +53:36:52.0 -- not an asteroid (will add it to exclusion list)
23:30:20.83 +50:22:17.8 -- not an asteroid (will add it to exclusion list)
23:28:11.69 +53:34:43.9 -- not an asteroid (will add it to exclusion list)
00:09:00.35 +54:34:36.3 -- not an asteroid (will add it to exclusion list)
23:16:48.67 +56:44:39.5 -- not an asteroid (will add it to exclusion list)
23:50:57.87 +53:34:45.9 -- not an asteroid (will add it to exclusion list)
23:52:43.77 +51:16:38.3 -- not an asteroid (will add it to exclusion list)
23:17:17.74 +56:04:19.7 -- not an asteroid (will add it to exclusion list)
00:15:17.00 +51:40:37.0 -- not an asteroid (will add it to exclusion list)
23:27:25.43 +56:44:43.8 -- not an asteroid (will add it to exclusion list)
23:35:37.60 +51:04:21.3 -- not an asteroid (will add it to exclusion list)
23:34:07.22 +54:09:29.1 -- not an asteroid (will add it to exclusion list)
23:57:55.58 +50:00:11.9 -- not an asteroid (will add it to exclusion list)
23:42:53.84 +54:25:05.1 -- not an asteroid (will add it to exclusion list)
23:24:41.24 +50:39:38.4 -- not an asteroid (will add it to exclusion list)
23:41:49.04 +51:06:39.5 -- not an asteroid (will add it to exclusion list)
00:13:01.82 +53:50:13.6 -- not an asteroid (will add it to exclusion list)
23:19:54.07 +49:51:21.3 -- not an asteroid (will add it to exclusion list)
00:00:34.95 +51:13:14.6 -- not an asteroid (will add it to exclusion list)
23:15:45.90 +55:44:41.8 -- not an asteroid (will add it to exclusion list)
00:07:48.32 +54:40:28.6 -- not an asteroid (will add it to exclusion list)
23:26:51.06 +50:20:13.9 -- not an asteroid (will add it to exclusion list)
23:45:29.04 +54:37:38.2 -- not an asteroid (will add it to exclusion list)
23:30:42.20 +58:00:40.6 -- not an asteroid (will add it to exclusion list)
00:05:33.49 +50:54:12.9 -- not an asteroid (will add it to exclusion list)
23:58:27.57 +52:16:04.1 -- not an asteroid (will add it to exclusion list)
23:22:41.95 +50:08:56.4 -- not an asteroid (will add it to exclusion list)
00:23:12.05 +56:00:07.1 -- not an asteroid (will add it to exclusion list)
23:46:33.71 +53:16:40.3 -- not an asteroid (will add it to exclusion list)
23:30:32.83 +54:53:57.6 -- not an asteroid (will add it to exclusion list)
23:20:43.46 +52:15:31.1 -- not an asteroid (will add it to exclusion list)
00:09:31.08 +51:50:03.3 -- not an asteroid (will add it to exclusion list)
00:27:15.89 +53:26:57.0 -- not an asteroid (will add it to exclusion list)
23:18:13.31 +54:31:38.2 -- not an asteroid (will add it to exclusion list)
23:29:05.88 +57:56:19.4 -- not an asteroid (will add it to exclusion list)
00:05:06.43 +54:30:24.1 -- not an asteroid (will add it to exclusion list)
23:18:16.98 +54:09:21.5 -- not an asteroid (will add it to exclusion list)
23:38:15.75 +56:01:37.7 -- not an asteroid (will add it to exclusion list)
23:37:51.41 +51:51:10.9 -- not an asteroid (will add it to exclusion list)
23:20:45.72 +54:32:02.1 -- not an asteroid (will add it to exclusion list)
23:39:45.45 +51:01:20.1 -- not an asteroid (will add it to exclusion list)
23:12:56.89 +55:27:53.2 -- not an asteroid (will add it to exclusion list)
23:27:48.29 +56:18:33.6 -- not an asteroid (will add it to exclusion list)
23:42:00.50 +51:29:24.8 -- not an asteroid (will add it to exclusion list)
23:21:10.64 +55:53:37.8 -- not an asteroid (will add it to exclusion list)
00:07:16.49 +51:00:10.5 -- not an asteroid (will add it to exclusion list)
23:27:18.08 +56:40:25.9 -- not an asteroid (will add it to exclusion list)
23:32:09.66 +52:54:18.0 -- not an asteroid (will add it to exclusion list)
23:59:24.38 +50:35:23.0 -- not an asteroid (will add it to exclusion list)
23:12:58.95 +56:18:50.6 -- not an asteroid (will add it to exclusion list)
23:20:03.66 +49:30:57.1 -- not an asteroid (will add it to exclusion list)
23:14:48.20 +54:45:40.1 -- not an asteroid (will add it to exclusion list)
23:12:49.57 +57:05:36.5 -- not an asteroid (will add it to exclusion list)
23:30:53.65 +49:58:04.2 -- not an asteroid (will add it to exclusion list)
00:26:59.42 +51:56:16.5 -- not an asteroid (will add it to exclusion list)
23:21:44.42 +54:27:02.2 -- not an asteroid (will add it to exclusion list)
23:33:08.76 +51:57:12.2 -- not an asteroid (will add it to exclusion list)
00:09:04.74 +51:43:27.8 -- not an asteroid (will add it to exclusion list)
23:50:03.14 +53:38:14.1 -- not an asteroid (will add it to exclusion list)
23:49:49.46 +52:31:08.4 -- not an asteroid (will add it to exclusion list)
23:48:51.31 +52:53:33.2 -- not an asteroid (will add it to exclusion list)
00:05:10.88 +52:08:38.1 -- not an asteroid (will add it to exclusion list)
23:51:09.98 +51:25:55.4 -- not an asteroid (will add it to exclusion list)
23:38:04.29 +55:46:00.3 -- not an asteroid (will add it to exclusion list)
23:33:19.74 +56:17:53.3 -- not an asteroid (will add it to exclusion list)
23:37:16.12 +51:29:31.0 -- not an asteroid (will add it to exclusion list)
23:37:52.68 +50:22:58.9 -- not an asteroid (will add it to exclusion list)
23:42:14.30 +53:13:15.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:34.95 +51:13:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:06.43 +54:30:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:10.88 +52:08:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:33.49 +50:54:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:16.49 +51:00:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:48.32 +54:40:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:00.35 +54:34:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:04.74 +51:43:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:31.08 +51:50:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:01.82 +53:50:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:17.00 +51:40:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:12.05 +56:00:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:59.42 +51:56:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:15.89 +53:26:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:49.57 +57:05:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:56.89 +55:27:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:58.95 +56:18:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:48.20 +54:45:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:45.90 +55:44:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:48.67 +56:44:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:17.74 +56:04:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:13.31 +54:31:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:16.98 +54:09:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:54.07 +49:51:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:03.66 +49:30:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:43.46 +52:15:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:45.72 +54:32:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:10.64 +55:53:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:42.30 +50:06:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:44.42 +54:27:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:41.95 +50:08:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:41.24 +50:39:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:51.06 +50:20:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:18.08 +56:40:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:25.43 +56:44:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:48.29 +56:18:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:11.69 +53:34:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:05.88 +57:56:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:20.83 +50:22:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:32.83 +54:53:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:42.20 +58:00:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:53.65 +49:58:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:09.66 +52:54:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:08.76 +51:57:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:19.74 +56:17:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:07.22 +54:09:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:37.60 +51:04:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:16.12 +51:29:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:51.41 +51:51:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:52.68 +50:22:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:04.29 +55:46:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:15.75 +56:01:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:48.31 +53:36:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:45.45 +51:01:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:49.04 +51:06:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:00.50 +51:29:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:14.30 +53:13:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:53.84 +54:25:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:29.04 +54:37:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:33.71 +53:16:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:51.31 +52:53:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:49.46 +52:31:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:03.14 +53:38:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:57.87 +53:34:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:09.98 +51:25:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:43.77 +51:16:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:48.29 +50:59:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:55.58 +50:00:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:27.57 +52:16:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:24.38 +50:35:23.0 -- 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)
00:00:34.95 +51:13:14.6 -- not a known variable star
00:05:06.43 +54:30:24.1 -- not a known variable star
00:05:10.88 +52:08:38.1 -- not a known variable star
00:05:33.49 +50:54:12.9 -- not a known variable star
00:07:16.49 +51:00:10.5 -- not a known variable star
00:07:48.32 +54:40:28.6 -- not a known variable star
00:09:00.35 +54:34:36.3 -- not a known variable star
00:09:04.74 +51:43:27.8 -- not a known variable star
00:09:31.08 +51:50:03.3 -- not a known variable star
00:13:01.82 +53:50:13.6 -- not a known variable star
00:15:17.00 +51:40:37.0 -- not a known variable star
00:23:12.05 +56:00:07.1 -- not a known variable star
00:26:59.42 +51:56:16.5 -- not a known variable star
00:27:15.89 +53:26:57.0 -- not a known variable star
23:12:49.57 +57:05:36.5 -- not a known variable star
23:12:56.89 +55:27:53.2 -- a known variable star
23:12:58.95 +56:18:50.6 -- not a known variable star
23:14:48.20 +54:45:40.1 -- a known variable star
23:15:45.90 +55:44:41.8 -- not a known variable star
23:16:48.67 +56:44:39.5 -- not a known variable star
23:17:17.74 +56:04:19.7 -- not a known variable star
23:18:13.31 +54:31:38.2 -- not a known variable star
23:18:16.98 +54:09:21.5 -- not a known variable star
23:19:54.07 +49:51:21.3 -- a known variable star
23:20:03.66 +49:30:57.1 -- not a known variable star
23:20:43.46 +52:15:31.1 -- not a known variable star
23:20:45.72 +54:32:02.1 -- a known variable star
23:21:10.64 +55:53:37.8 -- a known variable star
23:21:42.30 +50:06:40.6 -- not a known variable star
23:21:44.42 +54:27:02.2 -- not a known variable star
23:22:41.95 +50:08:56.4 -- not a known variable star
23:24:41.24 +50:39:38.4 -- not a known variable star
23:26:51.06 +50:20:13.9 -- not a known variable star
23:27:18.08 +56:40:25.9 -- not a known variable star
23:27:25.43 +56:44:43.8 -- not a known variable star
23:27:48.29 +56:18:33.6 -- not a known variable star
23:28:11.69 +53:34:43.9 -- not a known variable star
23:29:05.88 +57:56:19.4 -- not a known variable star
23:30:20.83 +50:22:17.8 -- not a known variable star
23:30:32.83 +54:53:57.6 -- not a known variable star
23:30:42.20 +58:00:40.6 -- not a known variable star
23:30:53.65 +49:58:04.2 -- not a known variable star
23:32:09.66 +52:54:18.0 -- not a known variable star
23:33:08.76 +51:57:12.2 -- not a known variable star
23:33:19.74 +56:17:53.3 -- not a known variable star
23:34:07.22 +54:09:29.1 -- not a known variable star
23:35:37.60 +51:04:21.3 -- a known variable star
23:37:16.12 +51:29:31.0 -- not a known variable star
23:37:51.41 +51:51:10.9 -- not a known variable star
23:37:52.68 +50:22:58.9 -- not a known variable star
23:38:04.29 +55:46:00.3 -- not a known variable star
23:38:15.75 +56:01:37.7 -- not a known variable star
23:38:48.31 +53:36:52.0 -- not a known variable star
23:39:45.45 +51:01:20.1 -- not a known variable star
23:41:49.04 +51:06:39.5 -- not a known variable star
23:42:00.50 +51:29:24.8 -- not a known variable star
23:42:14.30 +53:13:15.9 -- not a known variable star
23:42:53.84 +54:25:05.1 -- not a known variable star
23:45:29.04 +54:37:38.2 -- not a known variable star
23:46:33.71 +53:16:40.3 -- not a known variable star
23:48:51.31 +52:53:33.2 -- not a known variable star
23:49:49.46 +52:31:08.4 -- not a known variable star
23:50:03.14 +53:38:14.1 -- not a known variable star
23:50:57.87 +53:34:45.9 -- not a known variable star
23:51:09.98 +51:25:55.4 -- not a known variable star
23:52:43.77 +51:16:38.3 -- not a known variable star
23:56:48.29 +50:59:51.1 -- not a known variable star
23:57:55.58 +50:00:11.9 -- not a known variable star
23:58:27.57 +52:16:04.1 -- not a known variable star
23:59:24.38 +50:35:23.0 -- not a known variable star
Found 64 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
70 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 70 (excluding asteroids and hot pixels, 64 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)2461277.66368813 -observatory V36
10:07:10.41 +13:27:39.3 Mercury (-1.9mag)
12:58:58.45 -09:03:01.0 Venus (-4.5mag)
06:37:46.69 +23:35:03.9 Mars (1.3mag)
08:57:56.38 +17:43:19.5 Jupiter (-1.8mag)
00:54:22.10 +02:58:00.4 Saturn (0.5mag)
04:13:12.98 +21:00:46.7 Uranus (5.7mag)
00:14:54.54 +00:04:42.9 Neptune (7.7mag)
20:26:36.25 -23:36:04.9 Pluto (14.5mag)
19:59:28.06 -24:17:02.0 Moon (-11.8mag)
-rw-r--r-- 1 apache apache 363 Aug 24 23:03 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461277.66368813:
08:57:58.68 +17:43:10.3 Io (6.1mag)
08:57:51.64 +17:43:42.6 Europa (6.3mag)
08:57:49.62 +17:43:50.2 Ganymede (5.6mag)
08:58:03.09 +17:42:51.5 Callisto (6.9mag)
08:55:25.83 +17:52:59.2 Himalia (15.7mag)
08:57:54.42 +17:43:28.9 Thebe (16.6mag)
08:55:05.70 +17:48:23.9 Elara (17.7mag)
09:02:02.69 +17:15:27.8 Pasiphae (17.9mag)
08:59:57.71 +17:57:37.0 Carme (19.0mag)
00:54:08.78 +02:58:10.2 Titan (8.4mag)
00:54:17.71 +02:57:47.1 Rhea (9.7mag)
00:54:57.91 +03:00:07.5 Iapetus (11.1mag)
00:54:16.58 +02:58:26.0 Hyperion (14.4mag)
00:53:23.54 +02:49:06.5 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 24 23:04 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461277.66368813:
20:30:17.92 -11:46:33.5 JWST
17:56:38.13 +32:51:26.3 Chandra
22:18:00.98 +56:11:52.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 24 23:03 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461277.66368813 -observatory V36
03:30:45.35 +18:37:19.6 17.5mag P/1996 R2 (Lagerkvist)
18:00:03.44 -34:26:06.7 14.2mag P/2010 H2 (Vales)
07:08:54.28 -69:37:21.2 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:13:41.40 +33:22:25.3 17.7mag C/2017 K2 (PANSTARRS)
04:27:24.78 +43:04:18.5 17.6mag P/2021 N1 (ZTF)
22:24:21.05 +30:06:46.5 17.4mag C/2022 E2 (ATLAS)
06:59:24.08 +26:13:47.3 16.8mag C/2022 N2 (PANSTARRS)
10:37:19.18 +27:44:07.2 17.0mag C/2022 QE78 (ATLAS)
09:40:09.37 +05:17:30.7 18.0mag C/2022 R6 (PANSTARRS)
15:16:30.09 -13:00:19.6 18.0mag P/2023 B1 (PANSTARRS)
20:50:27.19 +63:35:51.6 18.0mag C/2023 H5 (Lemmon)
15:34:51.27 -14:29:07.7 14.6mag C/2023 R1 (PANSTARRS)
08:26:04.79 +32:09:18.1 15.6mag C/2024 E1 (Wierzchos)
15:05:41.66 +15:28:29.6 17.8mag C/2024 G6 (ATLAS)
18:44:05.50 +43:29:00.5 13.7mag C/2024 J3 (ATLAS)
20:45:10.62 +49:41:21.6 17.5mag C/2024 R4 (PANSTARRS)
05:27:40.42 -12:54:27.3 15.3mag C/2024 T5 (ATLAS)
07:06:02.83 +21:05:02.2 17.9mag C/2025 J1 (Borisov)
10:57:29.14 +19:45:25.0 17.0mag C/2025 V2 (Rankin)
13:09:25.10 +01:08:37.8 16.9mag C/2025 Y1 (ATLAS)
16:14:19.58 +75:56:13.0 16.4mag C/2026 A2 (Bok)
03:09:43.80 +46:20:48.3 17.3mag C/2026 B2 (Sun-Gao)
12:01:20.23 +10:10:37.7 17.4mag A/2026 E1
22:14:55.66 -33:01:24.4 7.2mag 10P/Tempel
11:39:31.44 -04:30:54.7 16.3mag 29P/Schwassmann-Wachmann
11:42:05.02 -00:53:10.3 17.4mag 63P/Wild
00:50:41.44 -06:15:36.6 15.4mag 65P/Gunn
06:12:44.00 +20:06:07.7 13.7mag 78P/Gehrels
20:23:46.45 -25:14:31.1 17.4mag 84P/Giclas
03:13:31.44 +14:39:18.7 17.0mag 88P/Howell
08:36:58.88 +25:08:28.6 16.5mag 93P/Lovas
04:56:09.27 +23:31:02.6 17.2mag 112P/Urata-Niijima
06:51:28.45 +27:46:22.8 16.0mag 114P/Wiseman-Skiff
09:58:07.09 +23:32:59.8 14.9mag 123P/West-Hartley
12:18:23.03 -16:38:18.4 17.3mag 124P/Mrkos
06:00:33.89 +20:58:33.7 16.0mag 128P/Shoemaker-Holt
06:56:23.17 +17:54:55.1 17.9mag 131P/Mueller
23:58:32.67 +02:59:53.9 17.4mag 139P/Vaisala-Oterma
03:05:37.70 -18:30:38.5 12.6mag 161P/Hartley-IRAS
08:12:36.55 +38:05:27.3 16.1mag 162P/Siding Spring
10:37:18.35 +26:07:44.2 12.3mag 169P/NEAT
03:10:02.60 +09:17:23.6 17.6mag 220P/McNaught
20:16:07.75 -51:25:44.6 18.0mag 259P/Garradd
04:11:20.38 +31:51:55.5 15.3mag 260P/McNaught
07:55:22.88 +36:53:27.4 17.3mag 295P/LINEAR
15:17:35.46 +01:14:12.0 17.8mag 391P/Kowalski
09:16:13.68 +17:31:27.9 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.3K Aug 24 23:03 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
-rw-r--r-- 1 apache apache 190K Aug 24 23:03 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:33:55.780 -21:38:59.14 AT 2026xqa 2026-08-03.18 18.0148
21:55:59.445 +07:05:12.88 AT 2026xpz 2026-08-05.35 19.863
16:45:38.067 +72:51:22.66 AT 2026xpy 2026-08-05.91 20.09
16:42:36.347 +57:19:39.63 AT 2026xpx 2026-08-05.92 19.14
11:49:41.968 +31:31:29.11 AT 2026xpw 2026-01-27.50 20.88
09:24:00.803 +39:35:33.95 AT 2026xpv 2026-01-19.40 20.33
12:49:17.559 +46:39:17.78 AT 2026xpu 2026-01-19.61 21.02
09:21:30.163 +36:17:37.77 AT 2026xpt 2026-01-19.40 20.66
07:49:07.955 +40:36:24.67 AT 2026xps 2026-01-18.38 20.96
13:27:11.570 +33:26:06.06 AT 2026xpr 2026-01-17.59 20.66
12:35:40.338 +14:59:49.24 AT 2026xpq 2026-01-17.53 20.38
13:05:21.770 +10:09:12.94 AT 2026xpp 2026-01-16.58 20.11
10:23:27.739 +49:29:35.53 AT 2026xpo 2026-01-14.60 21.05
01:23:04.564 +12:23:08.97 AT 2026xpn 2026-07-29.54 20.19
16:47:23.438 +66:28:39.91 AT 2026xpm 2026-08-05.89 19.92
23:34:35.589 +29:43:01.68 AT 2026xpl 2026-07-27.51 20.27
20:31:23.535 -10:54:59.72 AT 2026xpk 2026-08-03.43 20.33
10:34:15.921 +52:45:00.65 AT 2026xpj 2026-01-14.61 20.82
10:40:15.540 -22:57:09.71 AT 2026xpi 2026-01-27.59 20.18
09:44:54.064 -01:47:07.25 AT 2026xph 2026-02-14.42 20.93
-rw-r--r-- 1 apache apache 87K Aug 24 23:03 tns_transients_list.txt
