This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq
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 07 18.1794 2461239.6794 12.44 23:44:16.80 +51:40:48.6
112.45910 -9.82078 galactic Cas Second-epoch detections are separated by 1.1" and 8.1 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 | 23:44:16.80 +51:40:48.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:16.80 +51:40:48.6: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:16.80 +51:40:48.6: 13.62 +/- 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 07 18.1794* 23 44 16.80 +51 40 48.6 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
target,2461239.6794,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260718.1794 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.30 23:46:15.15 +52:45:10.8
113.03425 -8.86152 galactic Cas Second-epoch detections are separated by 1.1" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1945363281626831488 | 23:46:14.29 +52:44:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:15.15 +52:45:10.8: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:15.15 +52:45:10.8: 13.66 +/- 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 07 18.1794* 23 46 15.15 +52 45 10.8 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1945363281626831488,2461239.6794,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1945363281626831488 20260718.1794 12.30CV 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 07 18.1794 2461239.6794 12.47 23:44:58.72 +55:01:33.5
113.43476 -6.61561 galactic Cas Second-epoch detections are separated by 1.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1994621157730571648 | 23:45:03.10 +55:01:45.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.323+/-0.041 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:58.72 +55:01:33.5: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:58.72 +55:01:33.5: 13.63 +/- 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 07 18.1794* 23 44 58.72 +55 01 33.5 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
Gaia DR3 1994621157730571648,2461239.6794,12.47,0.05,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
Gaia DR3 1994621157730571648 20260718.1794 12.47CV 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 07 18.1794 2461239.6794 12.59 23:34:37.78 +53:35:38.7
111.57490 -7.57546 galactic Cas Second-epoch detections are separated by 0.7" and 7.9 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 | 23:34:37.78 +53:35:38.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:37.78 +53:35:38.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:37.78 +53:35:38.7: 13.43 +/- 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 07 18.1794* 23 34 37.78 +53 35 38.7 12.6 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,2461239.6794,12.59,0.05,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 20260718.1794 12.59CV 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 07 18.1794 2461239.6794 12.52 23:35:32.87 +56:05:53.8
112.44014 -5.21979 galactic Cas Second-epoch detections are separated by 0.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1997696118100411136 | 23:35:33.21 +56:05:13.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.321+/-0.044 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:32.87 +56:05:53.8: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:32.87 +56:05:53.8: 13.44 +/- 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 07 18.1794* 23 35 32.87 +56 05 53.8 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
Gaia DR3 1997696118100411136,2461239.6794,12.52,0.05,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
Gaia DR3 1997696118100411136 20260718.1794 12.52CV 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 07 18.1794 2461239.6794 12.41 23:49:20.24 +55:31:33.7
114.16467 -6.28507 galactic Cas Second-epoch detections are separated by 1.4" and 7.8 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 | 23:49:20.24 +55:31:33.7 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.039 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:20.24 +55:31:33.7: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:20.24 +55:31:33.7: 13.40 +/- 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 07 18.1794* 23 49 20.24 +55 31 33.7 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,2461239.6794,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.20 00:04:12.88 +55:36:14.5
116.24975 -6.65385 galactic Cas Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:04:12.88 +55:36:14.5 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:12.88 +55:36:14.5: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:12.88 +55:36:14.5: 13.60 +/- 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 07 18.1794* 00 04 12.88 +55 36 14.5 12.2 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,2461239.6794,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260718.1794 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.24 23:37:17.74 +55:33:07.6
112.51859 -5.81346 galactic Cas Second-epoch detections are separated by 1.4" and 8.0 pix
The object was found in VSX 2" Gaia DR3 1997558095031557632
Type: ROT
# Max. Min./Amp. JD0 Period
13.950 G 13.980 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:17.74 +55:33:07.6: 13.20 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:17.74 +55:33:07.6: 13.08 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.1794* 23 37 17.74 +55 33 07.6 12.2 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 1997558095031557632,2461239.6794,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997558095031557632 20260718.1794 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.36 23:36:49.02 +56:55:01.8
112.84515 -4.48605 galactic Cas Second-epoch detections are separated by 2.7" and 8.3 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 J354.1988+56.9151 | 23:36:49.02 +56:55:01.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:49.02 +56:55:01.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:49.02 +56:55:01.8: 13.45 +/- 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 07 18.1794* 23 36 49.02 +56 55 01.8 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 J354.1988+56.9151,2461239.6794,12.36,0.05,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
ATO J354.1988+56.9151 20260718.1794 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 07 18.1794 2461239.6794 12.19 23:46:36.44 +54:09:45.1
113.44426 -7.51065 galactic Cas Second-epoch detections are separated by 0.3" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1993760759825454336 | 23:46:40.25 +54:09:29.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:36.44 +54:09:45.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:36.44 +54:09:45.1: 13.61 +/- 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 07 18.1794* 23 46 36.44 +54 09 45.1 12.2 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 1993760759825454336,2461239.6794,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993760759825454336 20260718.1794 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.46 23:16:56.98 +52:55:46.6
108.83663 -7.33676 galactic And Second-epoch detections are separated by 0.9" and 8.1 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 | 23:16:56.98 +52:55:46.6 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:56.98 +52:55:46.6: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:56.98 +52:55:46.6: 13.58 +/- 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 07 18.1794* 23 16 56.98 +52 55 46.6 12.5 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,2461239.6794,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.24 23:35:20.02 +54:55:24.7
112.06712 -6.33479 galactic Cas Second-epoch detections are separated by 1.5" and 7.7 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 J353.8332+54.9240 | 23:35:22.33 +54:55:14.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.229+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:20.02 +54:55:24.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:20.02 +54:55:24.7: 13.63 +/- 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 07 18.1794* 23 35 20.02 +54 55 24.7 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.8332+54.9240,2461239.6794,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.8332+54.9240 20260718.1794 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.29 23:27:40.51 +53:59:08.7
110.71143 -6.88664 galactic Cas Second-epoch detections are separated by 1.6" and 7.8 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 J351.9157+53.9893 | 23:27:40.25 +53:58:51.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:40.51 +53:59:08.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:40.51 +53:59:08.7: 13.50 +/- 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 07 18.1794* 23 27 40.51 +53 59 08.7 12.3 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
ATO J351.9157+53.9893,2461239.6794,12.29,0.05,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
ATO J351.9157+53.9893 20260718.1794 12.29CV 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 07 18.1794 2461239.6794 11.95 00:15:17.99 +53:07:48.6
117.45251 -9.35668 galactic Cas Second-epoch detections are separated by 0.8" and 7.6 pix
The object was found in VSX18" Gaia DR3 419243891056810368
Type: ROT
# Max. Min./Amp. JD0 Period
12.930 G 13.020 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:17.99 +53:07:48.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:17.99 +53:07:48.6: 13.73 +/- 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 07 18.1794* 00 15 17.99 +53 07 48.6 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419243891056810368,2461239.6794,11.95,0.05,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 419243891056810368 20260718.1794 11.95CV 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 07 18.1794 2461239.6794 12.12 00:00:21.26 +53:34:11.0
115.30372 -8.54373 galactic Cas Second-epoch detections are separated by 1.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:00:21.26 +53:34:11.0 (user input) | T | P | (position from user input) J-Ks=0.609+/-0.032 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:21.26 +53:34:11.0: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:21.26 +53:34:11.0: 13.69 +/- 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 07 18.1794* 00 00 21.26 +53 34 11.0 12.1 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,2461239.6794,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260718.1794 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.28 23:19:39.71 +53:12:18.9
109.31921 -7.22353 galactic Cas Second-epoch detections are separated by 1.6" and 8.4 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 | 23:19:39.71 +53:12:18.9 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:39.71 +53:12:18.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:39.71 +53:12:18.9: 13.58 +/- 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 07 18.1794* 23 19 39.71 +53 12 18.9 12.3 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,2461239.6794,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.10 23:45:47.67 +57:16:15.0
114.11845 -4.47335 galactic Cas Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.4612+57.2675 | 23:45:47.67 +57:16:15.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.345+/-0.058 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:47.67 +57:16:15.0: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:47.67 +57:16:15.0: 13.60 +/- 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 07 18.1794* 23 45 47.67 +57 16 15.0 12.1 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 J356.4612+57.2675,2461239.6794,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J356.4612+57.2675 20260718.1794 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.21 23:49:09.36 +57:30:17.1
114.61646 -4.35800 galactic Cas Second-epoch detections are separated by 2.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J357.2749+57.4948 | 23:49:09.36 +57:30:17.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.861+/-0.034 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:09.36 +57:30:17.1: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:09.36 +57:30:17.1: 13.57 +/- 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 07 18.1794* 23 49 09.36 +57 30 17.1 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.2749+57.4948,2461239.6794,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.2749+57.4948 20260718.1794 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.97 00:09:01.30 +54:47:06.9
116.78664 -7.57961 galactic Cas Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:09:01.30 +54:47:06.9 (user input) | T | P | (position from user input) J-Ks=0.601+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:01.30 +54:47:06.9: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:01.30 +54:47:06.9: 13.65 +/- 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 07 18.1794* 00 09 01.30 +54 47 06.9 12.0 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,2461239.6794,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 11.97CV 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 07 18.1794 2461239.6794 11.95 00:17:01.90 +57:24:20.9
118.29194 -5.15565 galactic Cas Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:17:01.90 +57:24:20.9 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.031 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:17:01.90 +57:24:20.9: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:17:01.90 +57:24:20.9: 13.52 +/- 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 07 18.1794* 00 17 01.90 +57 24 20.9 11.9 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,2461239.6794,11.95,0.05,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 20260718.1794 11.95CV 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 07 18.1794 2461239.6794 11.78 00:31:04.38 +55:22:25.2
120.01737 -7.38279 galactic Cas Second-epoch detections are separated by 4.9" and 8.0 pix
The object was found in VSX 2" Gaia DR3 418234333222683648
Type: ROT
# Max. Min./Amp. JD0 Period
13.930 G 13.950 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:04.38 +55:22:25.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:04.38 +55:22:25.2: 13.42 +/- 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 07 18.1794* 00 31 04.38 +55 22 25.2 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 418234333222683648,2461239.6794,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 418234333222683648 20260718.1794 11.78CV 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 07 18.1794 2461239.6794 12.37 23:21:01.34 +54:13:16.2
109.86428 -6.34056 galactic Cas Second-epoch detections are separated by 1.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1995983521359752448 | 23:21:03.17 +54:13:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:01.34 +54:13:16.2: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:01.34 +54:13:16.2: 13.54 +/- 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 07 18.1794* 23 21 01.34 +54 13 16.2 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
Gaia DR3 1995983521359752448,2461239.6794,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995983521359752448 20260718.1794 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.27 23:19:14.60 +54:14:10.7
109.62431 -6.23606 galactic Cas Second-epoch detections are separated by 0.2" and 8.1 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 1995993077666419072 | 23:19:11.33 +54:14:05.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.411+/-0.037 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:14.60 +54:14:10.7: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:14.60 +54:14:10.7: 13.52 +/- 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 07 18.1794* 23 19 14.60 +54 14 10.7 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995993077666419072,2461239.6794,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1995993077666419072 20260718.1794 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.06 23:31:48.14 +56:54:18.1
112.18562 -4.29591 galactic Cas Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1998596652484201600 | 23:31:48.61 +56:53:39.2 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.415+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:48.14 +56:54:18.1: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:48.14 +56:54:18.1: 13.45 +/- 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 07 18.1794* 23 31 48.14 +56 54 18.1 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998596652484201600,2461239.6794,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998596652484201600 20260718.1794 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.03 23:34:43.94 +55:56:14.6
112.28350 -5.34038 galactic Cas Second-epoch detections are separated by 2.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.6763+55.9290 | 23:34:43.94 +55:56:14.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.438+/-0.041 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:43.94 +55:56:14.6: 13.66 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:43.94 +55:56:14.6: 13.21 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 07 18.1794* 23 34 43.94 +55 56 14.6 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.6763+55.9290,2461239.6794,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.6763+55.9290 20260718.1794 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.84 00:09:10.89 +54:30:27.4
116.76344 -7.85726 galactic Cas Second-epoch detections are separated by 2.1" and 7.3 pix
The object was found in VSX 4" Gaia DR3 420200809767588608
Type: ROT
# Max. Min./Amp. JD0 Period
13.580 G 13.620 G M
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:10.89 +54:30:27.4: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:10.89 +54:30:27.4: 13.66 +/- 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 07 18.1794* 00 09 10.89 +54 30 27.4 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420200809767588608,2461239.6794,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420200809767588608 20260718.1794 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.98 00:11:25.03 +55:00:14.4
117.16494 -7.41900 galactic Cas Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J002.8471+55.0015 | 00:11:25.03 +55:00:14.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.379+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:25.03 +55:00:14.4: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:25.03 +55:00:14.4: 13.64 +/- 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 07 18.1794* 00 11 25.03 +55 00 14.4 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.8471+55.0015,2461239.6794,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J002.8471+55.0015 20260718.1794 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.06 23:31:10.13 +52:06:28.4
110.61797 -8.83429 galactic Cas Second-epoch detections are separated by 3.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1991628016502919424 | 23:31:08.08 +52:06:52.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:10.13 +52:06:28.4: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:10.13 +52:06:28.4: 13.67 +/- 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 07 18.1794* 23 31 10.13 +52 06 28.4 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991628016502919424,2461239.6794,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991628016502919424 20260718.1794 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.05 23:54:15.97 +53:20:53.8
114.36071 -8.56936 galactic Cas Second-epoch detections are separated by 0.2" and 7.8 pix
The object was found in VSX16" Gaia DR3 1945440522318576000
Type: S
# Max. Min./Amp. JD0 Period
16.570 G 17.260 G F
ATTENTION: measured mag 12.05 is 4.5 mag brighter than the VSX record maximum brightness 16.57 - 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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:15.97 +53:20:53.8: 12.91 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:15.97 +53:20:53.8: 12.96 +/- 0.23 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.1794* 23 54 15.97 +53 20 53.8 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1945440522318576000,2461239.6794,12.05,0.05,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
Gaia DR3 1945440522318576000 20260718.1794 12.05CV 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 07 18.1794 2461239.6794 11.93 23:44:33.09 +53:02:41.1
112.85890 -8.51386 galactic Cas Second-epoch detections are separated by 0.3" and 7.9 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 | 23:44:33.09 +53:02:41.1 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:33.09 +53:02:41.1: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:33.09 +53:02:41.1: 13.61 +/- 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 07 18.1794* 23 44 33.09 +53 02 41.1 11.9 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,2461239.6794,11.93,0.05,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 20260718.1794 11.93CV 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 07 18.1794 2461239.6794 12.23 23:10:11.92 +57:07:36.4
109.49457 -3.08002 galactic Cas Second-epoch detections are separated by 0.3" and 8.1 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 2009160313529262592 | 23:10:17.09 +57:07:18.1 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE SpType: A1V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:11.92 +57:07:36.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:11.92 +57:07:36.4: 13.45 +/- 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 07 18.1794* 23 10 11.92 +57 07 36.4 12.2 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 2009160313529262592,2461239.6794,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009160313529262592 20260718.1794 12.23CV 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 07 18.1794 2461239.6794 12.00 00:04:07.82 +56:06:30.8
116.33116 -6.15571 galactic Cas Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J001.0225+56.1167 | 00:04:07.82 +56:06:30.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.318+/-0.035 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:07.82 +56:06:30.8: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:07.82 +56:06:30.8: 13.56 +/- 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 07 18.1794* 00 04 07.82 +56 06 30.8 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.0225+56.1167,2461239.6794,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J001.0225+56.1167 20260718.1794 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.13 23:30:56.70 +51:10:35.3
110.29210 -9.70911 galactic Cas Second-epoch detections are separated by 1.6" and 8.3 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 | 23:30:56.70 +51:10:35.3 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:56.70 +51:10:35.3: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:56.70 +51:10:35.3: 13.67 +/- 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 07 18.1794* 23 30 56.70 +51 10 35.3 12.1 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,2461239.6794,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.02 23:36:46.52 +53:03:07.8
111.72481 -8.18724 galactic Cas Second-epoch detections are separated by 2.4" and 7.6 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 | 23:36:46.52 +53:03:07.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:46.52 +53:03:07.8: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:46.52 +53:03:07.8: 13.55 +/- 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 07 18.1794* 23 36 46.52 +53 03 07.8 12.0 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,2461239.6794,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260718.1794 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.88 23:57:35.32 +56:46:47.2
115.57231 -5.32053 galactic Cas Second-epoch detections are separated by 2.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | NSV 26176 | 23:57:34.31 +56:46:02.9 (Gaia DR3) | (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A2p 1970ApJ...162..523S NGC 7789 799
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:35.32 +56:46:47.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:35.32 +56:46:47.2: 12.88 +/- 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 07 18.1794* 23 57 35.32 +56 46 47.2 11.9 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
NSV 26176,2461239.6794,11.88,0.05,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
NSV 26176 20260718.1794 11.88CV 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 07 18.1794 2461239.6794 11.71 00:15:29.86 +57:39:49.5
118.12260 -4.87201 galactic Cas Second-epoch detections are separated by 2.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 422779748649330176 | 00:15:28.06 +57:40:14.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.130+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:29.86 +57:39:49.5: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:29.86 +57:39:49.5: 13.62 +/- 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 07 18.1794* 00 15 29.86 +57 39 49.5 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 422779748649330176,2461239.6794,11.71,0.05,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
Gaia DR3 422779748649330176 20260718.1794 11.71CV 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 07 18.1794 2461239.6794 12.12 23:21:40.85 +51:06:26.3
108.87715 -9.29858 galactic And Second-epoch detections are separated by 1.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:21:40.85 +51:06:26.3 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.030 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:40.85 +51:06:26.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:40.85 +51:06:26.3: 13.57 +/- 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 07 18.1794* 23 21 40.85 +51 06 26.3 12.1 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,2461239.6794,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260718.1794 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.74 00:23:19.31 +56:00:17.1
118.98198 -6.65122 galactic Cas Second-epoch detections are separated by 2.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J005.8273+56.0081 | 00:23:19.31 +56:00:17.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.367+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:19.31 +56:00:17.1: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:19.31 +56:00:17.1: 13.67 +/- 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 07 18.1794* 00 23 19.31 +56 00 17.1 11.7 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 J005.8273+56.0081,2461239.6794,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J005.8273+56.0081 20260718.1794 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.78 23:39:31.73 +55:18:15.0
112.75446 -6.14027 galactic Cas Second-epoch detections are separated by 0.1" and 7.8 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 | 23:39:31.73 +55:18:15.0 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.460+/-0.042 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:31.73 +55:18:15.0: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:31.73 +55:18:15.0: 13.56 +/- 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 07 18.1794* 23 39 31.73 +55 18 15.0 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.6794,11.78,0.05,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 20260718.1794 11.78CV 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 07 18.1794 2461239.6794 11.81 23:46:34.81 +51:28:31.5
112.75642 -10.11039 galactic Cas Second-epoch detections are separated by 0.9" and 7.7 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 J356.6454+51.4778 | 23:46:34.81 +51:28:31.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.391+/-0.039 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:34.81 +51:28:31.5: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:34.81 +51:28:31.5: 13.70 +/- 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 07 18.1794* 23 46 34.81 +51 28 31.5 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.6454+51.4778,2461239.6794,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.6454+51.4778 20260718.1794 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.56 00:22:56.82 +50:57:51.9
118.35851 -11.65416 galactic Cas Second-epoch detections are separated by 2.2" and 7.8 pix
The object was found in VSX19" Gaia DR3 394749726919235328
Type: ROT
# Max. Min./Amp. JD0 Period
13.920 G 13.950 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:56.82 +50:57:51.9: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:56.82 +50:57:51.9: 13.56 +/- 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 07 18.1794* 00 22 56.82 +50 57 51.9 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394749726919235328,2461239.6794,11.56,0.05,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
Gaia DR3 394749726919235328 20260718.1794 11.56CV 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 07 18.1794 2461239.6794 11.90 23:36:55.78 +54:03:09.9
112.03692 -7.23538 galactic Cas Second-epoch detections are separated by 2.0" and 8.0 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 | 23:36:55.78 +54:03:09.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:55.78 +54:03:09.9: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:55.78 +54:03:09.9: 13.73 +/- 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 07 18.1794* 23 36 55.78 +54 03 09.9 11.9 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,2461239.6794,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.98 23:43:23.43 +57:27:43.1
113.85350 -4.20544 galactic Cas Second-epoch detections are separated by 8.5" and 7.0 pix
The object was found in VSX 7" Gaia DR3 1998661386231043584
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.000 G 14.030 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:23.43 +57:27:43.1: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:23.43 +57:27:43.1: 13.64 +/- 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 07 18.1794* 23 43 23.43 +57 27 43.1 12.0 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 1998661386231043584,2461239.6794,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998661386231043584 20260718.1794 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.85 23:47:36.03 +55:28:07.4
113.91064 -6.28091 galactic Cas Second-epoch detections are separated by 0.5" and 7.8 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 | 23:47:36.03 +55:28:07.4 (user input) | T | P | (position from user input) J-Ks=1.204+/-0.034 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:36.03 +55:28:07.4: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:47:36.03 +55:28:07.4: 13.69 +/- 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 07 18.1794* 23 47 36.03 +55 28 07.4 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.6794,11.85,0.05,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 20260718.1794 11.85CV 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 07 18.1794 2461239.6794 11.84 23:27:32.45 +54:50:50.7
110.97063 -6.06413 galactic Cas Second-epoch detections are separated by 1.3" and 7.7 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 J351.8904+54.8483 | 23:27:32.45 +54:50:50.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:32.45 +54:50:50.7: 13.24 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:32.45 +54:50:50.7: 12.84 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.1794* 23 27 32.45 +54 50 50.7 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.8904+54.8483,2461239.6794,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.8904+54.8483 20260718.1794 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.70 00:26:43.09 +57:15:38.6
119.57912 -5.45002 galactic Cas Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:26:43.09 +57:15:38.6 (user input) | T | P | (position from user input) J-Ks=0.728+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:43.09 +57:15:38.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:43.09 +57:15:38.6: 13.52 +/- 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 07 18.1794* 00 26 43.09 +57 15 38.6 11.7 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,2461239.6794,11.70,0.05,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
target 20260718.1794 11.70CV 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 07 18.1794 2461239.6794 11.76 23:46:38.85 +53:36:25.6
113.30953 -8.04982 galactic Cas Second-epoch detections are separated by 1.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1993497559929926016 | 23:46:37.87 +53:36:44.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.497+/-0.048 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:38.85 +53:36:25.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:38.85 +53:36:25.6: 13.64 +/- 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 07 18.1794* 23 46 38.85 +53 36 25.6 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993497559929926016,2461239.6794,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993497559929926016 20260718.1794 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.95 23:17:04.27 +54:39:05.6
109.47529 -5.73588 galactic Cas Second-epoch detections are separated by 1.2" and 8.0 pix
The object was found in VSX12" Gaia DR3 1996793934448061696
Type: ROT
# Max. Min./Amp. JD0 Period
13.510 G 13.550 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:04.27 +54:39:05.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:04.27 +54:39:05.6: 13.56 +/- 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 07 18.1794* 23 17 04.27 +54 39 05.6 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996793934448061696,2461239.6794,11.95,0.05,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 1996793934448061696 20260718.1794 11.95CV 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 07 18.1794 2461239.6794 11.78 23:28:21.63 +53:30:44.0
110.65581 -7.36773 galactic Cas Second-epoch detections are separated by 0.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1992745425257923200 | 23:28:20.51 +53:30:28.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.366+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:21.63 +53:30:44.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:21.63 +53:30:44.0: 13.53 +/- 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 07 18.1794* 23 28 21.63 +53 30 44.0 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992745425257923200,2461239.6794,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992745425257923200 20260718.1794 11.78CV 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 07 18.1794 2461239.6794 11.76 23:28:33.67 +53:36:15.8
110.71383 -7.28982 galactic Cas Second-epoch detections are separated by 0.6" and 7.9 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 | 23:28:33.67 +53:36:15.8 (user input) | T | P | (position from user input) J-Ks=0.863+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:33.67 +53:36:15.8: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:33.67 +53:36:15.8: 13.59 +/- 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 07 18.1794* 23 28 33.67 +53 36 15.8 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.6794,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.90 23:19:36.59 +55:55:15.9
110.26500 -4.67578 galactic Cas Second-epoch detections are separated by 0.6" and 7.9 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 J349.8878+55.9195 | 23:19:36.59 +55:55:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:36.59 +55:55:15.9: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:36.59 +55:55:15.9: 13.45 +/- 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 07 18.1794* 23 19 36.59 +55 55 15.9 11.9 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 J349.8878+55.9195,2461239.6794,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.8878+55.9195 20260718.1794 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.74 23:23:22.79 +53:36:20.4
109.98216 -7.03743 galactic Cas Second-epoch detections are separated by 1.8" and 7.8 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 1995798429747316736 | 23:23:25.49 +53:36:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.178+/-0.036 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:22.79 +53:36:20.4: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:22.79 +53:36:20.4: 13.64 +/- 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 07 18.1794* 23 23 22.79 +53 36 20.4 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995798429747316736,2461239.6794,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1995798429747316736 20260718.1794 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.37 00:19:06.06 +56:05:25.4
118.40303 -6.49675 galactic Cas Second-epoch detections are separated by 2.2" and 7.7 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 J004.7658+56.1014 | 00:19:06.06 +56:05:25.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.764+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:06.06 +56:05:25.4: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:06.06 +56:05:25.4: 13.62 +/- 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 07 18.1794* 00 19 06.06 +56 05 25.4 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J004.7658+56.1014,2461239.6794,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J004.7658+56.1014 20260718.1794 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.54 23:18:44.42 +55:58:25.7
110.16910 -4.58381 galactic Cas Second-epoch detections are separated by 1.9" and 8.2 pix
The object was found in VSX12" NSVS J2318429+555826
Type: SR
# Max. Min./Amp. JD0 Period
15.453 g Y 0.762 g 2458235.85240 249.075952100000 M5
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:44.42 +55:58:25.7: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:44.42 +55:58:25.7: 13.60 +/- 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 07 18.1794* 23 18 44.42 +55 58 25.7 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2318429+555826,2461239.6794,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2318429+555826 20260718.1794 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.62 23:29:01.37 +54:47:45.0
111.15770 -6.18086 galactic Cas Second-epoch detections are separated by 0.5" and 8.0 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 | 23:29:01.37 +54:47:45.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.370+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:01.37 +54:47:45.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:01.37 +54:47:45.0: 13.49 +/- 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 07 18.1794* 23 29 01.37 +54 47 45.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.6794,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.65 23:21:46.84 +54:35:20.7
110.09538 -6.03274 galactic Cas Second-epoch detections are separated by 2.0" and 8.1 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 | Large-amplitude variable Gaia DR2 1996007405677510528 | 23:21:46.14 +54:35:02.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: K1 (LAMOST DR5) J-Ks=0.682+/-0.026 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:46.84 +54:35:20.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:46.84 +54:35:20.7: 13.38 +/- 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 07 18.1794* 23 21 46.84 +54 35 20.7 11.7 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
Large-amplitude variable Gaia DR2 1996007405677510528,2461239.6794,11.65,0.05,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
Large-amplitude variable Gaia DR2 1996007405677510528 20260718.1794 11.65CV 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 07 18.1794 2461239.6794 11.31 00:14:30.85 +56:43:30.3
117.85676 -5.78238 galactic Cas Second-epoch detections are separated by 3.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J003.6271+56.7453 | 00:14:30.53 +56:44:02.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=1.189+/-0.030 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:30.85 +56:43:30.3: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:30.85 +56:43:30.3: 13.53 +/- 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 07 18.1794* 00 14 30.85 +56 43 30.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.6271+56.7453,2461239.6794,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J003.6271+56.7453 20260718.1794 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.60 23:19:37.54 +55:36:21.9
110.15698 -4.97183 galactic Cas Second-epoch detections are separated by 1.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996916976673295232 | 23:19:38.38 +55:36:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:37.54 +55:36:21.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:37.54 +55:36:21.9: 13.60 +/- 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 07 18.1794* 23 19 37.54 +55 36 21.9 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996916976673295232,2461239.6794,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996916976673295232 20260718.1794 11.60CV 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 07 18.1794 2461239.6794 11.78 23:11:07.55 +55:23:53.7
108.95599 -4.72795 galactic Cas Second-epoch detections are separated by 1.5" and 7.9 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 J347.7659+55.4001 | 23:11:07.55 +55:23:53.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.513+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:07.55 +55:23:53.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:07.55 +55:23:53.7: 13.40 +/- 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 07 18.1794* 23 11 07.55 +55 23 53.7 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.7659+55.4001,2461239.6794,11.78,0.05,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
ATO J347.7659+55.4001 20260718.1794 11.78CV 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 07 18.1794 2461239.6794 11.63 23:22:31.11 +52:04:54.8
109.33850 -8.42741 galactic And Second-epoch detections are separated by 1.5" and 8.1 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 1992336857905747328 | 23:22:28.82 +52:04:37.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.729+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:31.11 +52:04:54.8: 12.82 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:31.11 +52:04:54.8: 12.37 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.1794* 23 22 31.11 +52 04 54.8 11.6 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
Gaia DR3 1992336857905747328,2461239.6794,11.63,0.05,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
Gaia DR3 1992336857905747328 20260718.1794 11.63CV 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 07 18.1794 2461239.6794 11.13 23:58:38.60 +53:54:05.1
115.12102 -8.16774 galactic Cas Second-epoch detections are separated by 0.5" and 7.7 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 J359.6649+53.9052 | 23:58:38.60 +53:54:05.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.368+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:38.60 +53:54:05.1: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:38.60 +53:54:05.1: 13.73 +/- 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 07 18.1794* 23 58 38.60 +53 54 05.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.6649+53.9052,2461239.6794,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.6649+53.9052 20260718.1794 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.30 23:22:38.99 +54:02:34.6
110.02857 -6.58945 galactic Cas Second-epoch detections are separated by 0.9" and 7.9 pix
The object was found in VSX16" ZTF J232240.59+540227.7
Type: RS
# Max. Min./Amp. JD0 Period
12.964 g Y 0.058 g 2458494.64530 0.743440200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:38.99 +54:02:34.6: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:38.99 +54:02:34.6: 13.60 +/- 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 07 18.1794* 23 22 38.99 +54 02 34.6 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J232240.59+540227.7,2461239.6794,11.30,0.05,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
ZTF J232240.59+540227.7 20260718.1794 11.30CV 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 07 18.1794 2461239.6794 11.36 23:14:10.72 +54:09:43.9
108.90239 -6.03892 galactic Cas Second-epoch detections are separated by 0.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.5351+54.1603 | 23:14:08.43 +54:09:37.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:10.72 +54:09:43.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:10.72 +54:09:43.9: 13.52 +/- 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 07 18.1794* 23 14 10.72 +54 09 43.9 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.5351+54.1603,2461239.6794,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.5351+54.1603 20260718.1794 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 10.95 23:56:33.15 +56:44:32.1
115.42497 -5.32740 galactic Cas Second-epoch detections are separated by 1.0" and 7.5 pix
The object was found in VSX17" V0874 Cas
Type: EA
# Max. Min./Amp. JD0 Period
13.980 V 14.310 V 2449904.93000 1.200070000000
ATTENTION: measured mag 10.95 is 3.0 mag brighter than the VSX record maximum brightness 13.98 - 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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:33.15 +56:44:32.1: 12.97 +/- 0.26 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:33.15 +56:44:32.1: 12.60 +/- 0.21 detection
Forced photometry reference-image weighted average: 12.75 +/- 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 07 18.1794* 23 56 33.15 +56 44 32.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0874 Cas,2461239.6794,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0874 Cas 20260718.1794 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.21 23:12:41.12 +54:49:12.3
108.94526 -5.34754 galactic Cas Second-epoch detections are separated by 1.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996494626770732160 | 23:12:37.83 +54:49:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:41.12 +54:49:12.3: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:41.12 +54:49:12.3: 13.45 +/- 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 07 18.1794* 23 12 41.12 +54 49 12.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996494626770732160,2461239.6794,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996494626770732160 20260718.1794 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.16 23:18:40.97 +54:16:19.0
109.55982 -6.17392 galactic Cas Second-epoch detections are separated by 1.6" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1995973075999277440 | 23:18:38.04 +54:16:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.721+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:40.97 +54:16:19.0: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:40.97 +54:16:19.0: 13.62 +/- 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 07 18.1794* 23 18 40.97 +54 16 19.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995973075999277440,2461239.6794,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995973075999277440 20260718.1794 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.14 23:28:23.31 +57:13:12.8
111.84131 -3.85237 galactic Cas Second-epoch detections are separated by 0.9" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1998829370990757376 | 23:28:25.30 +57:13:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.453+/-0.029 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:23.31 +57:13:12.8: 13.72 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:23.31 +57:13:12.8: 13.59 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.72 +/- 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 07 18.1794* 23 28 23.31 +57 13 12.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998829370990757376,2461239.6794,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998829370990757376 20260718.1794 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.16 23:13:35.90 +55:20:55.7
109.26430 -4.90523 galactic Cas Second-epoch detections are separated by 1.7" and 7.8 pix
The object was found in VSX 1" Gaia DR3 1996708378701541632
Type: VAR
# Max. Min./Amp. JD0 Period
13.040 G 13.100 G 0.017762900000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:35.90 +55:20:55.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:35.90 +55:20:55.7: 13.35 +/- 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 07 18.1794* 23 13 35.90 +55 20 55.7 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996708378701541632,2461239.6794,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996708378701541632 20260718.1794 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 10.88 23:36:52.71 +53:45:16.2
111.94340 -7.51895 galactic Cas Second-epoch detections are separated by 0.2" and 7.8 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 1994035431572565760 | 23:36:49.96 +53:45:46.2 (Gaia DR3) | (local) | 1.506050000000 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:52.71 +53:45:16.2: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:52.71 +53:45:16.2: 13.69 +/- 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 07 18.1794* 23 36 52.71 +53 45 16.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994035431572565760,2461239.6794,10.88,0.05,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
Gaia DR3 1994035431572565760 20260718.1794 10.88CV 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 07 18.1794 2461239.6794 11.11 23:10:02.61 +56:51:39.2
109.37346 -3.31776 galactic Cas Second-epoch detections are separated by 0.4" and 8.0 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 J347.5055+56.8648 | 23:10:04.48 +56:52:03.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:02.61 +56:51:39.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:02.61 +56:51:39.2: 13.36 +/- 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 07 18.1794* 23 10 02.61 +56 51 39.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.5055+56.8648,2461239.6794,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.5055+56.8648 20260718.1794 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.04 23:18:56.64 +53:20:37.4
109.26691 -7.05621 galactic Cas Second-epoch detections are separated by 0.1" and 8.2 pix
The object was found in VSX 2" Gaia DR3 1995687275993223168
Type: ROT
# Max. Min./Amp. JD0 Period
12.980 G 13.010 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:56.64 +53:20:37.4: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:56.64 +53:20:37.4: 13.63 +/- 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 07 18.1794* 23 18 56.64 +53 20 37.4 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995687275993223168,2461239.6794,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995687275993223168 20260718.1794 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 10.97 23:14:46.56 +55:59:21.1
109.65542 -4.37072 galactic Cas Second-epoch detections are separated by 0.7" and 8.1 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 | 23:14:46.56 +55:59:21.1 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.036 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:46.56 +55:59:21.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:46.56 +55:59:21.1: 13.38 +/- 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 07 18.1794* 23 14 46.56 +55 59 21.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.6794,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 10.84 23:18:34.91 +54:31:30.6
109.63577 -5.93178 galactic Cas Second-epoch detections are separated by 2.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996050389711552512 | 23:18:37.19 +54:31:28.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.236+/-0.028 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:34.91 +54:31:30.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:34.91 +54:31:30.6: 13.47 +/- 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 07 18.1794* 23 18 34.91 +54 31 30.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996050389711552512,2461239.6794,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996050389711552512 20260718.1794 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 10.78 23:21:14.43 +55:23:13.6
110.29646 -5.25633 galactic Cas Second-epoch detections are separated by 0.5" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996852414723764608 | 23:21:11.12 +55:23:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5) J-Ks=0.546+/-0.028 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:14.43 +55:23:13.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:14.43 +55:23:13.6: 13.49 +/- 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 07 18.1794* 23 21 14.43 +55 23 13.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996852414723764608,2461239.6794,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996852414723764608 20260718.1794 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 10.62 23:19:00.25 +56:28:03.4
110.37727 -4.13424 galactic Cas Second-epoch detections are separated by 0.9" and 7.8 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 J349.7399+56.4563 | 23:18:59.67 +56:27:48.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.003+/-0.026 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:00.25 +56:28:03.4: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:00.25 +56:28:03.4: 13.45 +/- 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 07 18.1794* 23 19 00.25 +56 28 03.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.7399+56.4563,2461239.6794,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.7399+56.4563 20260718.1794 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 10.39 23:33:10.43 +52:52:20.3
111.14768 -8.19943 galactic Cas Second-epoch detections are separated by 1.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1993221548150793472 | 23:33:14.36 +52:52:24.7 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.153+/-0.028 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:10.43 +52:52:20.3: 13.14 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:10.43 +52:52:20.3: 12.86 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.1794* 23 33 10.43 +52 52 20.3 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993221548150793472,2461239.6794,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993221548150793472 20260718.1794 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 10.31 23:19:46.37 +55:43:11.4
110.21625 -4.87241 galactic Cas Second-epoch detections are separated by 1.3" and 8.2 pix
The object was found in VSX 1" Gaia DR3 1996921576577099136
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.110 G 12.220 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:46.37 +55:43:11.4: 13.53 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:46.37 +55:43:11.4: 12.99 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 07 18.1794* 23 19 46.37 +55 43 11.4 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996921576577099136,2461239.6794,10.31,0.05,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
Gaia DR3 1996921576577099136 20260718.1794 10.31CV 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 07 18.1794 2461239.6794 9.99 23:36:32.74 +50:40:33.3
110.99421 -10.45178 galactic And Second-epoch detections are separated by 0.3" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1944540365891633792 | 23:36:31.17 +50:40:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:32.74 +50:40:33.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:32.74 +50:40:33.3: 13.55 +/- 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 07 18.1794* 23 36 32.74 +50 40 33.3 10.0 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 1944540365891633792,2461239.6794,9.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944540365891633792 20260718.1794 9.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 9.97 23:27:26.38 +49:36:02.3
109.24446 -11.02568 galactic And Second-epoch detections are separated by 1.2" and 8.0 pix
The object was not found in VSX
The object was found in ASASSN-V 2" ASASSN-V J232726.19+493602.3
Type: L
MeanMag 11.8 m Amp. 0.09 m Period d
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:26.38 +49:36:02.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:26.38 +49:36:02.3: 13.46 +/- 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 07 18.1794* 23 27 26.38 +49 36 02.3 10.0 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
VARIABLE_NAME,2461239.6794,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260718.1794 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 9.59 00:15:19.64 +53:12:02.5
117.46676 -9.28744 galactic Cas Second-epoch detections are separated by 1.6" and 7.5 pix
The object was found in VSX 2" Gaia DR3 419244578251557888
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.410 G 11.480 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:19.64 +53:12:02.5: 13.19 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:19.64 +53:12:02.5: 13.10 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.1794* 00 15 19.64 +53 12 02.5 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419244578251557888,2461239.6794,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419244578251557888 20260718.1794 9.59CV 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 07 18.1794 2461239.6794 9.08 23:15:52.60 +52:57:57.5
108.69795 -7.24444 galactic And Second-epoch detections are separated by 0.8" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.9601+52.9506 | 23:15:51.87 +52:57:37.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1927AnHar.100...33C HD 236076 J-Ks=0.396+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:52.60 +52:57:57.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:52.60 +52:57:57.5: 13.52 +/- 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 07 18.1794* 23 15 52.60 +52 57 57.5 9.1 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 J348.9601+52.9506,2461239.6794,9.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.9601+52.9506 20260718.1794 9.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 9.98 23:20:57.79 +55:40:09.9
110.35672 -4.97770 galactic Cas Second-epoch detections are separated by 0.7" and 8.1 pix
The object was found in VSX16" Gaia DR3 1996906600032621824
Type: ROT
# Max. Min./Amp. JD0 Period
14.660 G 14.690 G F
ATTENTION: measured mag 9.98 is 4.7 mag brighter than the VSX record maximum brightness 14.66 - 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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:57.79 +55:40:09.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:57.79 +55:40:09.9: 13.46 +/- 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 07 18.1794* 23 20 57.79 +55 40 09.9 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996906600032621824,2461239.6794,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996906600032621824 20260718.1794 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 10.99 23:23:10.42 +55:05:29.1
110.45604 -5.62799 galactic Cas Second-epoch detections are separated by 0.8" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996170575775034880 | 23:23:14.91 +55:05:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1927AnHar.100...33C HD 236110
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:10.42 +55:05:29.1: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:10.42 +55:05:29.1: 13.46 +/- 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 07 18.1794* 23 23 10.42 +55 05 29.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996170575775034880,2461239.6794,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996170575775034880 20260718.1794 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.12 23:13:38.92 +53:34:20.1
108.60997 -6.55821 galactic Cas Second-epoch detections are separated by 0.9" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1995573094286898944 | 23:13:35.10 +53:34:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.475+/-0.027 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:38.92 +53:34:20.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:38.92 +53:34:20.1: 13.49 +/- 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 07 18.1794* 23 13 38.92 +53 34 20.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995573094286898944,2461239.6794,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1995573094286898944 20260718.1794 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.13 23:28:46.84 +52:18:46.0
110.33145 -8.52509 galactic Cas Second-epoch detections are separated by 1.0" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1991700068875645312 | 23:28:50.45 +52:18:52.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.468+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:46.84 +52:18:46.0: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:46.84 +52:18:46.0: 13.56 +/- 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 07 18.1794* 23 28 46.84 +52 18 46.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991700068875645312,2461239.6794,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991700068875645312 20260718.1794 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.27 23:25:04.95 +55:05:34.0
110.71530 -5.71751 galactic Cas Second-epoch detections are separated by 0.6" and 7.9 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 | 23:25:04.95 +55:05:34.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.363+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:04.95 +55:05:34.0: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:04.95 +55:05:34.0: 13.31 +/- 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 07 18.1794* 23 25 04.95 +55 05 34.0 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.6794,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260718.1794 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.25 23:56:52.61 +52:09:34.7
114.48927 -9.81546 galactic Cas Second-epoch detections are separated by 0.9" and 7.8 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 | 23:56:52.61 +52:09:34.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:52.61 +52:09:34.7: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:52.61 +52:09:34.7: 13.64 +/- 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 07 18.1794* 23 56 52.61 +52 09 34.7 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.6794,11.25,0.05,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
target 20260718.1794 11.25CV 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 07 18.1794 2461239.6794 11.62 23:23:13.28 +52:06:50.2
109.45214 -8.43385 galactic And Second-epoch detections are separated by 2.0" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1992342699061284736 | 23:23:09.69 +52:06:54.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:13.28 +52:06:50.2: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:13.28 +52:06:50.2: 13.58 +/- 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 07 18.1794* 23 23 13.28 +52 06 50.2 11.6 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
Gaia DR3 1992342699061284736,2461239.6794,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992342699061284736 20260718.1794 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.69 23:12:17.52 +57:05:09.7
109.74277 -3.22501 galactic Cas Second-epoch detections are separated by 2.1" and 7.8 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 J348.0943+57.0885 | 23:12:17.52 +57:05:09.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:17.52 +57:05:09.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:17.52 +57:05:09.7: 13.39 +/- 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 07 18.1794* 23 12 17.52 +57 05 09.7 11.7 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 J348.0943+57.0885,2461239.6794,11.69,0.05,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
ATO J348.0943+57.0885 20260718.1794 11.69CV 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 07 18.1794 2461239.6794 11.71 23:11:51.47 +55:18:27.4
109.01837 -4.85114 galactic Cas Second-epoch detections are separated by 2.3" and 8.3 pix
The object was found in VSX 6" Gaia DR3 1996757100812082688
Type: ROT
# Max. Min./Amp. JD0 Period
13.540 G 13.560 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:51.47 +55:18:27.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:51.47 +55:18:27.4: 13.52 +/- 0.36 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 07 18.1794* 23 11 51.47 +55 18 27.4 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996757100812082688,2461239.6794,11.71,0.05,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
Gaia DR3 1996757100812082688 20260718.1794 11.71CV 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 07 18.1794 2461239.6794 11.69 23:30:32.33 +49:52:16.9
109.81588 -10.92894 galactic And Second-epoch detections are separated by 1.3" and 8.0 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 J352.6481+49.8736 | 23:30:33.67 +49:52:45.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:32.33 +49:52:16.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:32.33 +49:52:16.9: 13.57 +/- 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 07 18.1794* 23 30 32.33 +49 52 16.9 11.7 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 J352.6481+49.8736,2461239.6794,11.69,0.05,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
ATO J352.6481+49.8736 20260718.1794 11.69CV 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 07 18.1794 2461239.6794 11.63 23:25:28.16 +49:20:12.3
108.84799 -11.16971 galactic And Second-epoch detections are separated by 1.4" and 7.9 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 | 23:25:28.16 +49:20:12.3 (user input) | T | P | (position from user input) J-Ks=0.648+/-0.029 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:28.16 +49:20:12.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:28.16 +49:20:12.3: 13.57 +/- 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 07 18.1794* 23 25 28.16 +49 20 12.3 11.6 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,2461239.6794,11.63,0.05,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 20260718.1794 11.63CV 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 07 18.1794 2461239.6794 11.65 23:41:50.00 +54:40:25.9
112.90192 -6.83674 galactic Cas Second-epoch detections are separated by 0.9" and 7.8 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 J355.4769+54.6722 | 23:41:50.00 +54:40:25.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.736+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:50.00 +54:40:25.9: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:50.00 +54:40:25.9: 13.56 +/- 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 07 18.1794* 23 41 50.00 +54 40 25.9 11.7 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 J355.4769+54.6722,2461239.6794,11.65,0.05,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
ATO J355.4769+54.6722 20260718.1794 11.65CV 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 07 18.1794 2461239.6794 11.68 23:29:24.02 +51:39:58.0
110.21576 -9.16868 galactic Cas Second-epoch detections are separated by 1.5" and 7.8 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 | Large-amplitude variable Gaia DR2 1991424538127002368 | 23:29:24.02 +51:39:58.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.374+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:24.02 +51:39:58.0: 13.23 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:24.02 +51:39:58.0: 13.06 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.1794* 23 29 24.02 +51 39 58.0 11.7 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
Large-amplitude variable Gaia DR2 1991424538127002368,2461239.6794,11.68,0.05,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
Large-amplitude variable Gaia DR2 1991424538127002368 20260718.1794 11.68CV 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 07 18.1794 2461239.6794 11.64 23:34:32.79 +49:44:27.7
110.40252 -11.25092 galactic And Second-epoch detections are separated by 3.2" and 7.6 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 J353.6511+49.7393 | 23:34:32.79 +49:44:27.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:32.79 +49:44:27.7: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:32.79 +49:44:27.7: 13.59 +/- 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 07 18.1794* 23 34 32.79 +49 44 27.7 11.6 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
ATO J353.6511+49.7393,2461239.6794,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.6511+49.7393 20260718.1794 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.81 23:24:53.22 +54:29:08.3
110.48732 -6.28143 galactic Cas Second-epoch detections are separated by 3.2" and 8.4 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 | 23:24:53.22 +54:29:08.3 (user input) | T | P | (position from user input) J-Ks=0.790+/-0.030 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:53.22 +54:29:08.3: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:53.22 +54:29:08.3: 13.68 +/- 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 07 18.1794* 23 24 53.22 +54 29 08.3 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.6794,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.61 23:41:08.61 +51:40:42.4
111.98317 -9.69273 galactic Cas Second-epoch detections are separated by 1.8" and 7.8 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 | 23:41:08.61 +51:40:42.4 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.033 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:08.61 +51:40:42.4: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:08.61 +51:40:42.4: 13.66 +/- 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 07 18.1794* 23 41 08.61 +51 40 42.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461239.6794,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260718.1794 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.95 23:20:29.87 +55:32:14.0
110.24907 -5.07917 galactic Cas Second-epoch detections are separated by 0.7" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.1127+55.5429 | 23:20:29.87 +55:32:14.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A2IV (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:29.87 +55:32:14.0: 13.07 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:29.87 +55:32:14.0: 13.24 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 07 18.1794* 23 20 29.87 +55 32 14.0 11.9 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 J350.1127+55.5429,2461239.6794,11.95,0.05,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
ATO J350.1127+55.5429 20260718.1794 11.95CV 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 07 18.1794 2461239.6794 11.83 23:34:08.21 +54:02:57.3
111.64072 -7.11917 galactic Cas Second-epoch detections are separated by 0.9" and 7.8 pix
The object was found in VSX 1" Gaia DR3 1994286807419596416
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.630 G 13.670 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:08.21 +54:02:57.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:08.21 +54:02:57.3: 13.47 +/- 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 07 18.1794* 23 34 08.21 +54 02 57.3 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994286807419596416,2461239.6794,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994286807419596416 20260718.1794 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.96 23:21:05.99 +55:55:40.1
110.46384 -4.74161 galactic Cas Second-epoch detections are separated by 1.4" and 8.0 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 | 23:21:05.99 +55:55:40.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:05.99 +55:55:40.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:05.99 +55:55:40.1: 13.53 +/- 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 07 18.1794* 23 21 05.99 +55 55 40.1 12.0 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,2461239.6794,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.89 23:17:29.54 +52:31:56.9
108.77027 -7.73694 galactic And Second-epoch detections are separated by 1.0" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1992633451161006720 | 23:17:33.26 +52:31:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.271+/-0.044 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:29.54 +52:31:56.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:29.54 +52:31:56.9: 13.47 +/- 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 07 18.1794* 23 17 29.54 +52 31 56.9 11.9 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 1992633451161006720,2461239.6794,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992633451161006720 20260718.1794 11.89CV 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 07 18.1794 2461239.6794 11.88 23:19:45.13 +49:15:32.4
107.92869 -10.92331 galactic And Second-epoch detections are separated by 2.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1942716374879051904 | 23:19:40.83 +49:15:23.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.568+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:45.13 +49:15:32.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:45.13 +49:15:32.4: 13.46 +/- 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 07 18.1794* 23 19 45.13 +49 15 32.4 11.9 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 1942716374879051904,2461239.6794,11.88,0.05,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
Gaia DR3 1942716374879051904 20260718.1794 11.88CV 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 07 18.1794 2461239.6794 12.02 23:28:27.82 +53:49:27.9
110.77046 -7.07659 galactic Cas Second-epoch detections are separated by 3.9" and 7.7 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 J352.1131+53.8121 | 23:28:30.29 +53:48:52.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:27.82 +53:49:27.9: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:27.82 +53:49:27.9: 13.58 +/- 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 07 18.1794* 23 28 27.82 +53 49 27.9 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.1131+53.8121,2461239.6794,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J352.1131+53.8121 20260718.1794 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.53 00:26:37.19 +54:30:45.7
119.29767 -8.18383 galactic Cas Second-epoch detections are separated by 1.7" and 7.3 pix
The object was found in VSX 4" Gaia DR3 419605596020621824
Type: ROT
# Max. Min./Amp. JD0 Period
13.590 G 13.610 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:37.19 +54:30:45.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:37.19 +54:30:45.7: 13.48 +/- 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 07 18.1794* 00 26 37.19 +54 30 45.7 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419605596020621824,2461239.6794,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419605596020621824 20260718.1794 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.03 23:15:33.12 +54:04:33.4
109.05896 -6.19286 galactic Cas Second-epoch detections are separated by 3.9" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996013865309055488 | 23:15:32.09 +54:05:11.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.261+/-0.033 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:33.12 +54:04:33.4: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:33.12 +54:04:33.4: 13.58 +/- 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 07 18.1794* 23 15 33.12 +54 04 33.4 12.0 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 1996013865309055488,2461239.6794,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996013865309055488 20260718.1794 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.96 23:27:19.57 +52:32:29.0
110.19310 -8.23753 galactic Cas Second-epoch detections are separated by 1.8" and 7.9 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 | 23:27:19.57 +52:32:29.0 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.032 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:19.57 +52:32:29.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:19.57 +52:32:29.0: 13.48 +/- 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 07 18.1794* 23 27 19.57 +52 32 29.0 12.0 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,2461239.6794,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.94 23:29:15.25 +51:14:31.0
110.05789 -9.56387 galactic Cas Second-epoch detections are separated by 1.0" and 7.9 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 J352.3145+51.2458 | 23:29:15.25 +51:14:31.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.145+/-0.043 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:15.25 +51:14:31.0: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:15.25 +51:14:31.0: 13.22 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.22 +/- 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 07 18.1794* 23 29 15.25 +51 14 31.0 11.9 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 J352.3145+51.2458,2461239.6794,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.3145+51.2458 20260718.1794 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.97 23:21:16.69 +54:35:03.8
110.02498 -6.01224 galactic Cas Second-epoch detections are separated by 0.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1996006855921682048 | 23:21:15.41 +54:34:37.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:16.69 +54:35:03.8: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:16.69 +54:35:03.8: 13.63 +/- 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 07 18.1794* 23 21 16.69 +54 35 03.8 12.0 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 1996006855921682048,2461239.6794,11.97,0.05,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 1996006855921682048 20260718.1794 11.97CV 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 07 18.1794 2461239.6794 11.88 00:10:04.64 +50:47:20.7
116.28130 -11.54780 galactic Cas Second-epoch detections are separated by 4.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J002.5137+50.7986 | 00:10:04.64 +50:47:20.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.826+/-0.029 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:04.64 +50:47:20.7: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:04.64 +50:47:20.7: 13.41 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.1794* 00 10 04.64 +50 47 20.7 11.9 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 J002.5137+50.7986,2461239.6794,11.88,0.05,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
ATO J002.5137+50.7986 20260718.1794 11.88CV 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 07 18.1794 2461239.6794 12.18 23:16:56.83 +54:01:31.7
109.23270 -6.31389 galactic Cas Second-epoch detections are separated by 2.9" and 8.1 pix
The object was found in VSX14" ZTF J231656.43+540117.9
Type: BY
# Max. Min./Amp. JD0 Period
16.668 r Y 0.065 r 2458386.77740 0.683370600000
ATTENTION: measured mag 12.18 is 4.4 mag brighter than the VSX record maximum brightness 16.60 - 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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:56.83 +54:01:31.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:56.83 +54:01:31.7: 13.40 +/- 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 07 18.1794* 23 16 56.83 +54 01 31.7 12.2 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 J231656.43+540117.9,2461239.6794,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J231656.43+540117.9 20260718.1794 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.15 23:25:51.16 +53:03:56.8
110.15261 -7.66923 galactic Cas Second-epoch detections are separated by 1.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1992711379053690112 | 23:25:48.37 +53:03:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:51.16 +53:03:56.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:51.16 +53:03:56.8: 13.52 +/- 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 07 18.1794* 23 25 51.16 +53 03 56.8 12.2 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 1992711379053690112,2461239.6794,12.15,0.05,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
Gaia DR3 1992711379053690112 20260718.1794 12.15CV 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 07 18.1794 2461239.6794 12.16 23:56:36.22 +56:16:48.6
115.33347 -5.78047 galactic Cas Second-epoch detections are separated by 0.1" and 7.6 pix
The object was found in VSX25" PS1-3PI J235634.62+561627.8
Type: EW
# Max. Min./Amp. JD0 Period
14.350 V 14.750 V 2458396.98050 0.428352000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:36.22 +56:16:48.6: 13.15 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:36.22 +56:16:48.6: 13.02 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 18.1794* 23 56 36.22 +56 16 48.6 12.2 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
PS1-3PI J235634.62+561627.8,2461239.6794,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PS1-3PI J235634.62+561627.8 20260718.1794 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.17 23:42:46.07 +57:25:47.2
113.76399 -4.21454 galactic Cas Second-epoch detections are separated by 0.5" and 7.6 pix
The object was found in VSX 9" ZTF J234245.31+572553.5
Type: SR
# Max. Min./Amp. JD0 Period
14.015 r Y 0.069 r 2458280.02390 126.817299200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:46.07 +57:25:47.2: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:46.07 +57:25:47.2: 13.58 +/- 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 07 18.1794* 23 42 46.07 +57 25 47.2 12.2 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 J234245.31+572553.5,2461239.6794,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J234245.31+572553.5 20260718.1794 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.06 23:56:18.97 +57:40:50.0
115.59353 -4.40369 galactic Cas Second-epoch detections are separated by 5.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:56:18.97 +57:40:50.0 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:18.97 +57:40:50.0: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:18.97 +57:40:50.0: 13.57 +/- 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 07 18.1794* 23 56 18.97 +57 40 50.0 12.1 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,2461239.6794,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260718.1794 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.57 23:10:21.38 +56:59:47.8
109.46478 -3.20854 galactic Cas Second-epoch detections are separated by 0.3" and 8.0 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 J347.5891+57.0002 | 23:10:21.38 +56:59:47.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.466+/-0.033 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:21.38 +56:59:47.8: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:21.38 +56:59:47.8: 13.28 +/- 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 07 18.1794* 23 10 21.38 +56 59 47.8 12.6 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 J347.5891+57.0002,2461239.6794,12.57,0.05,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 J347.5891+57.0002 20260718.1794 12.57CV 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 07 18.1794 2461239.6794 12.61 23:13:59.11 +55:52:57.5
109.51289 -4.42923 galactic Cas Second-epoch detections are separated by 1.7" and 8.0 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 | 23:13:59.11 +55:52:57.5 (user input) | T | P | (position from user input) J-Ks=0.746+/-0.031 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:59.11 +55:52:57.5: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:59.11 +55:52:57.5: 13.33 +/- 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 07 18.1794* 23 13 59.11 +55 52 57.5 12.6 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,2461239.6794,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260718.1794 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.29 00:22:19.64 +55:04:30.4
118.73647 -7.55933 galactic Cas Second-epoch detections are separated by 2.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:19.64 +55:04:30.4 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:19.64 +55:04:30.4: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:19.64 +55:04:30.4: 13.40 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 07 18.1794* 00 22 19.64 +55 04 30.4 12.3 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,2461239.6794,12.29,0.05,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 20260718.1794 12.29CV 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 07 18.1794 2461239.6794 12.21 23:54:06.62 +54:45:02.9
114.65270 -7.19679 galactic Cas Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1993848823833987072 | 23:54:11.06 +54:45:18.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.451+/-0.043 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:06.62 +54:45:02.9: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:06.62 +54:45:02.9: 13.70 +/- 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 07 18.1794* 23 54 06.62 +54 45 02.9 12.2 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
Large-amplitude variable Gaia DR2 1993848823833987072,2461239.6794,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1993848823833987072 20260718.1794 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.57 23:16:43.23 +54:09:55.3
109.25204 -6.17140 galactic Cas Second-epoch detections are separated by 4.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:16:43.23 +54:09:55.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:43.23 +54:09:55.3: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:43.23 +54:09:55.3: 13.48 +/- 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 07 18.1794* 23 16 43.23 +54 09 55.3 12.6 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,2461239.6794,12.57,0.05,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
target 20260718.1794 12.57CV 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 07 18.1794 2461239.6794 12.40 23:30:34.29 +54:58:11.5
111.42515 -6.08505 galactic Cas Second-epoch detections are separated by 4.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1997423782814582400 | 23:30:37.00 +54:58:36.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:34.29 +54:58:11.5: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:34.29 +54:58:11.5: 13.65 +/- 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 07 18.1794* 23 30 34.29 +54 58 11.5 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
Gaia DR3 1997423782814582400,2461239.6794,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997423782814582400 20260718.1794 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.53 23:57:50.86 +57:26:58.1
115.74632 -4.67271 galactic Cas Second-epoch detections are separated by 1.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J359.4630+57.4387 | 23:57:54.76 +57:26:27.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.480+/-0.035 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:50.86 +57:26:58.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:50.86 +57:26:58.1: 13.59 +/- 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 07 18.1794* 23 57 50.86 +57 26 58.1 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
ATO J359.4630+57.4387,2461239.6794,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.4630+57.4387 20260718.1794 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.38 23:43:00.29 +52:15:00.1
112.41896 -9.21932 galactic Cas Second-epoch detections are separated by 2.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J355.7547+52.2417 | 23:43:04.56 +52:14:49.7 (Gaia DR3) | LPV (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.334+/-0.035 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:00.29 +52:15:00.1: 13.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:00.29 +52:15:00.1: 13.74 +/- 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 07 18.1794* 23 43 00.29 +52 15 00.1 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 J355.7547+52.2417,2461239.6794,12.38,0.05,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
ATO J355.7547+52.2417 20260718.1794 12.38CV 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 07 18.1794 2461239.6794 12.58 23:33:17.55 +55:45:53.1
112.03828 -5.44540 galactic Cas Second-epoch detections are separated by 1.7" and 7.6 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 | 23:33:17.55 +55:45:53.1 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.034 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:17.55 +55:45:53.1: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:17.55 +55:45:53.1: 13.62 +/- 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 07 18.1794* 23 33 17.55 +55 45 53.1 12.6 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,2461239.6794,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260718.1794 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 12.61 23:50:37.24 +53:31:24.4
113.86702 -8.27450 galactic Cas Second-epoch detections are separated by 0.7" and 7.7 pix
The object was found in VSX 3" Gaia DR3 1993449426235149056
Type: ROT
# Max. Min./Amp. JD0 Period
14.630 G 14.660 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:37.24 +53:31:24.4: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:37.24 +53:31:24.4: 13.64 +/- 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 07 18.1794* 23 50 37.24 +53 31 24.4 12.6 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 1993449426235149056,2461239.6794,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 1993449426235149056 20260718.1794 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 11.62 23:26:01.26 +49:55:45.1
109.13356 -10.64024 galactic And Second-epoch detections are separated by 1.9" and 7.9 pix
The object was found in VSX 2" Gaia DR3 1943087155117309568
Type:
# Max. Min./Amp. JD0 Period
14.000 G 14.030 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:01.26 +49:55:45.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:01.26 +49:55:45.1: 13.59 +/- 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 07 18.1794* 23 26 01.26 +49 55 45.1 11.6 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
Gaia DR3 1943087155117309568,2461239.6794,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943087155117309568 20260718.1794 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 18.1794 2461239.6794 10.86 23:21:11.96 +50:00:11.8
108.41708 -10.30814 galactic And Second-epoch detections are separated by 2.0" and 7.8 pix
The object was found in VSX 3" AK And
Type: M
# Max. Min./Amp. JD0 Period
10.000 V < 15.000 V 2452930.00000 317.000000000000 S:
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:11.96 +50:00:11.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:11.96 +50:00:11.8: 13.46 +/- 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 07 18.1794* 23 21 11.96 +50 00 11.8 10.9 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
AK And,2461239.6794,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AK And 20260718.1794 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461239.67970484 18.07.2026 04:18:36.498 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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: 14 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 21610
Objects passed selection criteria: 21571
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 18553.5
Average stars matched: 17607.2 (94.8999 %)
Memory usage VmPeak: 131332 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 04:27:17 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: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
First image: 2461211.92320941 20.06.2026 10:09:15.293 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Last image: 2461239.67970484 18.07.2026 04:18:36.498 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 318
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 211 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 163905
Objects passed selection criteria: 163522
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 147823
Average stars matched: 140944 (95.3465 %)
Memory usage VmPeak: 1998080 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 17 15:05:04 CDT 2026
VaST build number 1.0rc89-157-gbf7d0e63
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-17)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jul 18 04:35:39 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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.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: 2461239.67906222
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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 926.8'x616.3' 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: 23:59:57.586 +54:01:07.73 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
Image size: 938.8'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:02.155 +53:59:56.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.155 +53:59:56.83
Angular distance between the image centers 0.0226 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
Image size: 938.7'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:05.654 +53:59:23.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:05.654 +53:59:23.54
Angular distance between the image centers 0.0350 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 00:00:02.155 +53:59:56.83
Second-epoch second image center 00:00:05.654 +53:59:23.54
Angular distance between the image centers 0.01261 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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.oMZoDJHD6j
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits &> /tmp/tmp.tULNKyRNw6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits &> /tmp/tmp.nLofwIQ3Zw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits &> /tmp/tmp.7pBxntkR8S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0012 to 359.9998 deg, Dec +48.2682 to +59.2677 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 0.0012 to 359.9998 deg, Dec 48.2682 to 59.2677 deg
Loaded 153348 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): 52 out of 57 total matches.
Matched with Tycho-2 57 out of 28951 detected stars.
ERROR: only 52 of 28951 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.18%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.575300
a=0.000000 b=1.000000 c=22.575300
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.91
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.91
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0012 to 359.9998 deg, Dec +48.2682 to +59.2677 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 0.0012 to 359.9998 deg, Dec 48.2682 to 59.2677 deg
Loaded 153348 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): 52 out of 57 total matches.
Matched with Tycho-2 57 out of 28951 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=6.3)
Read 32399 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0011 to 359.9996 deg, Dec +48.2682 to +59.2618 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 0.0011 to 359.9996 deg, Dec 48.2682 to 59.2618 deg
Loaded 153285 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): 56 out of 62 total matches.
Matched with Tycho-2 62 out of 32399 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.3 pix Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
2.3 pix fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
2.4 pix wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.3 pix wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Limiting magnitude estimates:
14.9 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
15.0 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
14.4 mag. fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
14.4 mag. fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.oMZoDJHD6j (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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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=2748, bad_region=6855, passed=28951
Got 28951 stars (including 19826 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 28951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (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 345.0821 through 0 to 14.9840, gap 14.9840 to 345.0821
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 331 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 241 matched stars entering correct_measured_positions(), 177 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.18"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 235 matched stars entering correct_measured_positions(), 5819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.02"
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 345.0724 through 0 to 15.0101, gap 15.0101 to 345.0724
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 401 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 345 matched stars entering correct_measured_positions(), 5883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.97"
Accuracy estimation diagnostic: 341 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.85"
Excluding outliers - 341 stars left (next iteration limit 258)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=341 sigma_overall_arcsec=10.000 sigma_q1_arcsec=26.458 sigma_q2_arcsec=26.280 sigma_q3_arcsec=7.321 sigma_q4_arcsec=8.000 n_q1=41 n_q2=24 n_q3=122 n_q4=154 worst_quadrant_to_overall_ratio=2.646
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tULNKyRNw6 (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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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=3204, bad_region=7312, passed=32399
Got 32399 stars (including 22421 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 32399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (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 345.0823 through 0 to 14.9840, gap 14.9840 to 345.0823
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 320 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 234 matched stars entering correct_measured_positions(), 171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 6406 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.53"
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 345.0732 through 0 to 15.0096, gap 15.0096 to 345.0732
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 399 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 343 matched stars entering correct_measured_positions(), 6467 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.48"
Accuracy estimation diagnostic: 340 matched stars entering correct_measured_positions(), 9572 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.44"
Excluding outliers - 340 stars left (next iteration limit 248)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=340 sigma_overall_arcsec=11.206 sigma_q1_arcsec=29.679 sigma_q2_arcsec=28.591 sigma_q3_arcsec=8.393 sigma_q4_arcsec=9.911 n_q1=41 n_q2=25 n_q3=115 n_q4=159 worst_quadrant_to_overall_ratio=2.649
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -region wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nLofwIQ3Zw (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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.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_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.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=1273, bad_region=3123, passed=16816
Got 16816 stars (including 12568 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat
util/solve_plate_with_UCAC5 got 16816 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8491 through 0 to 14.6558, gap 14.6558 to 344.8491
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 14073 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8484 through 0 to 14.6562, gap 14.6562 to 344.8484
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 14072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 14072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits N_match=973 sigma_overall_arcsec=0.632 sigma_q1_arcsec=0.638 sigma_q2_arcsec=0.611 sigma_q3_arcsec=0.656 sigma_q4_arcsec=0.661 n_q1=318 n_q2=180 n_q3=284 n_q4=191 worst_quadrant_to_overall_ratio=1.045
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.7pBxntkR8S (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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.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_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.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=1278, bad_region=3130, passed=16908
Got 16908 stars (including 12665 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat
util/solve_plate_with_UCAC5 got 16908 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8492 through 0 to 14.6558, gap 14.6558 to 344.8492
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 14136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8484 through 0 to 14.6562, gap 14.6562 to 344.8484
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 14136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 14136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits N_match=972 sigma_overall_arcsec=0.694 sigma_q1_arcsec=0.626 sigma_q2_arcsec=0.720 sigma_q3_arcsec=0.727 sigma_q4_arcsec=0.708 n_q1=314 n_q2=181 n_q3=288 n_q4=189 worst_quadrant_to_overall_ratio=1.047
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits sigma_overall=10.000 worst_q_ratio=2.646
ref2=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits sigma_overall=11.206 worst_q_ratio=2.649
new1=fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits sigma_overall=0.632 worst_q_ratio=1.045
new2=fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits sigma_overall=0.694 worst_q_ratio=1.047
reference average sigma_overall=10.603 worst_q_ratio=2.6475
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468_astrometric_residuals.png (341 matched stars from wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.98 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450_astrometric_residuals.png (340 matched stars from wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.94 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100_astrometric_residuals.png (973 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.57 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101_astrometric_residuals.png (972 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.59 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:31.98 +52:58:03.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:33.06 +52:40:59.3: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:47:31.98 +52:58:03.6: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:33.06 +52:40:59.3: 15.65 +/- 99.00 upperlimit
Adding exclusion_list_gaiadr2.txt__out33731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33732.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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 33731_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 33731_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:47:31.98 +52:58:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 1.063 1945375857291421056 356.88289708597 +52.96787165656 11.8544 11.5049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33732_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 33732_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:35:33.06 +52:40:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 2.018 1993177675063854592 353.88685196575 +52.68327249602 11.9313 11.5093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.018#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21482_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 21482_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:44:31.91 +56:34:50.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07077_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 07077_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:09:36.50 +51:34:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06239_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 06239_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:58:25.06 +51:23:24.9 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
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 ####
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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Image size: 926.8'x616.3' 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: 23:59:57.586 +54:01:07.73 J2000 4789.000 3195.000
###################################
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
Image size: 938.8'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:02.155 +53:59:56.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:02.155 +53:59:56.83
Angular distance between the image centers 0.0226 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
Image size: 938.7'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:05.654 +53:59:23.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:57.586 +54:01:07.73
Second-epoch image center 00:00:05.654 +53:59:23.54
Angular distance between the image centers 0.0350 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 00:00:02.155 +53:59:56.83
Second-epoch second image center 00:00:05.654 +53:59:23.54
Angular distance between the image centers 0.01261 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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits &> /tmp/tmp.qz119mVrZI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits &> /tmp/tmp.bMUpod6sDk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits &> /tmp/tmp.fOfNTFIhcN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits &> /tmp/tmp.xrHWZJaHSr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits and wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat' -> 'wcsmag.cat'
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9998 deg, Dec +48.2503 to +59.2677 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 0.0002 to 359.9998 deg, Dec 48.2503 to 59.2677 deg
Loaded 153589 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): 104 out of 148 total matches.
Matched with Tycho-2 148 out of 200953 detected stars.
ERROR: only 104 of 200953 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.05%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 20.521000
a=0.000000 b=1.000000 c=20.521000
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.21
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9998 deg, Dec +48.2503 to +59.2677 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 0.0002 to 359.9998 deg, Dec 48.2503 to 59.2677 deg
Loaded 153589 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): 104 out of 148 total matches.
Matched with Tycho-2 148 out of 200953 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (aperture=4.7)
Read 213202 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9999 deg, Dec +48.2308 to +59.2649 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 0.0002 to 359.9999 deg, Dec 48.2308 to 59.2649 deg
Loaded 153847 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): 122 out of 166 total matches.
Matched with Tycho-2 166 out of 213202 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 255 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.2 pix Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
2.2 pix wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Limiting magnitude estimates:
13.2 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
13.3 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
12.7 mag. fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
12.7 mag. fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.qz119mVrZI (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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.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=60, blended=29230, bad_region=30798, passed=200893
Got 200893 stars (including 144443 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat
util/solve_plate_with_UCAC5 got 200893 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.8'
Seting catalog search parameters based on the expected field of view 926.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012872 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010298 (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 345.0121 through 0 to 15.0290, gap 15.0290 to 345.0121
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 326 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 236 matched stars entering correct_measured_positions(), 169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 225 matched stars entering correct_measured_positions(), 42039 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.34"
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 345.0161 through 0 to 15.0639, gap 15.0639 to 345.0161
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 402 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 42110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.32"
Accuracy estimation diagnostic: 341 matched stars entering correct_measured_positions(), 65834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.71"
Excluding outliers - 341 stars left (next iteration limit 247)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=341 sigma_overall_arcsec=10.173 sigma_q1_arcsec=28.653 sigma_q2_arcsec=29.926 sigma_q3_arcsec=7.272 sigma_q4_arcsec=10.943 n_q1=31 n_q2=26 n_q3=117 n_q4=167 worst_quadrant_to_overall_ratio=2.942
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits -region wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bMUpod6sDk (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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits' -> 'wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.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=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=33709, bad_region=29431, passed=213150
Got 213150 stars (including 154424 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 213150 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (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 345.0123 through 0 to 15.0317, gap 15.0317 to 345.0123
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 319 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 236 matched stars entering correct_measured_positions(), 166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 227 matched stars entering correct_measured_positions(), 46390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.45"
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 345.0158 through 0 to 15.0663, gap 15.0663 to 345.0158
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.2 to 59.3)
Done reading UCAC5 zone files...
Matched 395 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 336 matched stars entering correct_measured_positions(), 46448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.44"
Accuracy estimation diagnostic: 332 matched stars entering correct_measured_positions(), 66751 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.69"
Excluding outliers - 332 stars left (next iteration limit 249)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=332 sigma_overall_arcsec=11.113 sigma_q1_arcsec=28.693 sigma_q2_arcsec=26.729 sigma_q3_arcsec=8.129 sigma_q4_arcsec=9.837 n_q1=36 n_q2=26 n_q3=118 n_q4=152 worst_quadrant_to_overall_ratio=2.582
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits -region wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fOfNTFIhcN (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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.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_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.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=32, blended=13439, bad_region=16745, passed=136234
Got 136234 stars (including 107260 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat
util/solve_plate_with_UCAC5 got 136234 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8112 through 0 to 14.8086, gap 14.8086 to 344.8112
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 121818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 344.8113 through 0 to 14.8091, gap 14.8091 to 344.8113
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 121819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 121818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits N_match=975 sigma_overall_arcsec=0.627 sigma_q1_arcsec=0.645 sigma_q2_arcsec=0.576 sigma_q3_arcsec=0.637 sigma_q4_arcsec=0.640 n_q1=324 n_q2=182 n_q3=271 n_q4=198 worst_quadrant_to_overall_ratio=1.029
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xrHWZJaHSr (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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.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_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.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=31, blended=13757, bad_region=16976, passed=137811
Got 137811 stars (including 108408 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat
util/solve_plate_with_UCAC5 got 137811 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8492 through 0 to 14.8256, gap 14.8256 to 344.8492
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 122935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8483 through 0 to 14.8262, gap 14.8262 to 344.8483
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 122934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 122934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits N_match=976 sigma_overall_arcsec=0.653 sigma_q1_arcsec=0.669 sigma_q2_arcsec=0.640 sigma_q3_arcsec=0.664 sigma_q4_arcsec=0.711 n_q1=318 n_q2=184 n_q3=277 n_q4=197 worst_quadrant_to_overall_ratio=1.089
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-17-40_20.00sec_5.00C_LIGHT_0100.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.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_2026-07-17_CI_Cas-04-Q2b1x1_231940_TTUQ2b1x1_2393820_j3sH60Dq/wcs_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:37.78 +53:35:38.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:05:02.13 +57:44:55.3: 12.70 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:28.13 +56:40:39.6: 13.18 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:15.15 +52:45:10.8: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:59:42.96 +56:08:04.5: 13.12 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:24.02 +56:03:24.6: 12.60 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:52.27 +55:30:17.0: 13.48 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:16.80 +51:40:48.6: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:05:02.13 +57:44:55.3: 12.56 +/- 0.14 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.10
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:58.72 +55:01:33.5: 13.71 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 00:05:02.13 +57:44:55.3: ref_mag=12.63 +/- 0.10 new_mean_mag=12.4703 delta=0.16 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:37.78 +53:35:38.7: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:59:42.96 +56:08:04.5: 12.99 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.16
Forced photometry filter REJECTED candidate at 23:59:42.96 +56:08:04.5: ref_mag=13.06 +/- 0.16 new_mean_mag=12.5141 delta=0.54 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:52.27 +55:30:17.0: 13.14 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.18
Forced photometry filter REJECTED candidate at 23:29:52.27 +55:30:17.0: ref_mag=13.28 +/- 0.18 new_mean_mag=12.7033 delta=0.57 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:28.13 +56:40:39.6: 13.12 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:15.15 +52:45:10.8: 13.66 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.15 +/- 0.15
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:16.80 +51:40:48.6: 13.62 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:54:28.13 +56:40:39.6: ref_mag=13.15 +/- 0.15 new_mean_mag=12.5252 delta=0.63 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:58.72 +55:01:33.5: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:24.02 +56:03:24.6: 12.22 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.08
Forced photometry filter REJECTED candidate at 00:00:24.02 +56:03:24.6: ref_mag=12.37 +/- 0.08 new_mean_mag=12.5343 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:32.87 +56:05:53.8: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:32.87 +56:05:53.8: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:20.24 +55:31:33.7: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:12.88 +55:36:14.5: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:36.57 +56:38:33.0: 11.63 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:12.88 +55:36:14.5: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:20.24 +55:31:33.7: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:17.74 +55:33:07.6: 13.20 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:36.57 +56:38:33.0: 11.41 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.04
Forced photometry filter REJECTED candidate at 00:00:36.57 +56:38:33.0: ref_mag=11.51 +/- 0.04 new_mean_mag=12.2301 delta=-0.72 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:49.02 +56:55:01.8: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:17.74 +55:33:07.6: 13.08 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.17
Forced photometry filter KEPT candidate at 23:37:17.74 +55:33:07.6: ref_mag=13.14 +/- 0.17 new_mean_mag=12.2204 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:49.02 +56:55:01.8: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:36.44 +54:09:45.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:36.44 +54:09:45.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:56.98 +52:55:46.6: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:56.98 +52:55:46.6: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:20.02 +54:55:24.7: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:20.02 +54:55:24.7: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:40.51 +53:59:08.7: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:40.51 +53:59:08.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:17.99 +53:07:48.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:17.99 +53:07:48.6: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:21.26 +53:34:11.0: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:21.26 +53:34:11.0: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:35.57 +56:18:33.8: 12.11 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:01.07 +52:09:26.9: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:01.07 +52:09:26.9: 13.05 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.23
Forced photometry filter REJECTED candidate at 23:27:01.07 +52:09:26.9: ref_mag=13.05 +/- 0.23 new_mean_mag=12.2348 delta=0.82 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:39.71 +53:12:18.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:35.57 +56:18:33.8: 11.81 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:47.67 +57:16:15.0: 13.77 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.93 +/- 0.05
Forced photometry filter REJECTED candidate at 23:52:35.57 +56:18:33.8: ref_mag=11.93 +/- 0.05 new_mean_mag=12.2931 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:47.67 +57:16:15.0: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:39.71 +53:12:18.9: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:09.36 +57:30:17.1: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:01.30 +54:47:06.9: 13.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:09.36 +57:30:17.1: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:17:01.90 +57:24:20.9: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:01.30 +54:47:06.9: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:17:01.90 +57:24:20.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:21.26 +54:44:52.4: 11.68 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:21.26 +54:44:52.4: 11.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.04
Forced photometry filter REJECTED candidate at 23:23:21.26 +54:44:52.4: ref_mag=11.68 +/- 0.04 new_mean_mag=12.1516 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:31:04.38 +55:22:25.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:01.34 +54:13:16.2: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:31:04.38 +55:22:25.2: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:01.34 +54:13:16.2: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:14.60 +54:14:10.7: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:14.60 +54:14:10.7: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:48.14 +56:54:18.1: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:48.14 +56:54:18.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:43.94 +55:56:14.6: 13.66 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:43.94 +55:56:14.6: 13.21 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.20
Forced photometry filter KEPT candidate at 23:34:43.94 +55:56:14.6: ref_mag=13.38 +/- 0.20 new_mean_mag=12.0102 delta=1.37 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:02.45 +56:51:05.4: 10.25 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:10.89 +54:30:27.4: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:02.45 +56:51:05.4: 9.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.02 +/- 0.01
Forced photometry filter REJECTED candidate at 23:41:02.45 +56:51:05.4: ref_mag=10.02 +/- 0.01 new_mean_mag=12.2185 delta=-2.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:10.89 +54:30:27.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:10.13 +52:06:28.4: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:25.03 +55:00:14.4: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:10.13 +52:06:28.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:15.97 +53:20:53.8: 12.91 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:25.03 +55:00:14.4: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:15.97 +53:20:53.8: 12.96 +/- 0.23 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.14
Forced photometry filter KEPT candidate at 23:54:15.97 +53:20:53.8: ref_mag=12.93 +/- 0.14 new_mean_mag=12.0267 delta=0.90 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:33.09 +53:02:41.1: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:33.09 +53:02:41.1: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:11.92 +57:07:36.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:04:07.82 +56:06:30.8: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:11.92 +57:07:36.4: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:04:07.82 +56:06:30.8: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:34.23 +56:49:22.9: 12.25 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:56.70 +51:10:35.3: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:34.23 +56:49:22.9: 12.07 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.09
Forced photometry filter REJECTED candidate at 23:58:34.23 +56:49:22.9: ref_mag=12.16 +/- 0.09 new_mean_mag=11.7791 delta=0.38 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:56.70 +51:10:35.3: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:46.52 +53:03:07.8: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:35.32 +56:46:47.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:46.52 +53:03:07.8: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:35.32 +56:46:47.2: 12.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:29.86 +57:39:49.5: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:29.86 +57:39:49.5: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:40.85 +51:06:26.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:40.85 +51:06:26.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:19.31 +56:00:17.1: 13.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:31.73 +55:18:15.0: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:19.31 +56:00:17.1: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:31.73 +55:18:15.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:34.81 +51:28:31.5: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:34.81 +51:28:31.5: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:56.82 +50:57:51.9: 13.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:56.82 +50:57:51.9: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:55.78 +54:03:09.9: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:55.78 +54:03:09.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:23.43 +57:27:43.1: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:23.43 +57:27:43.1: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:36.03 +55:28:07.4: 13.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:47:36.03 +55:28:07.4: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:32.45 +54:50:50.7: 13.24 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:32.45 +54:50:50.7: 12.84 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.17
Forced photometry filter KEPT candidate at 23:27:32.45 +54:50:50.7: ref_mag=13.00 +/- 0.17 new_mean_mag=11.8279 delta=1.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:43.09 +57:15:38.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:43.09 +57:15:38.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:38.85 +53:36:25.6: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:04.27 +54:39:05.6: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:38.85 +53:36:25.6: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:04.27 +54:39:05.6: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:21.63 +53:30:44.0: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:33.67 +53:36:15.8: 13.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:21.63 +53:30:44.0: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:22.79 +53:36:20.4: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:36.59 +55:55:15.9: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:33.67 +53:36:15.8: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:22.79 +53:36:20.4: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:36.59 +55:55:15.9: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:24.80 +54:13:46.4: 12.17 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:24.80 +54:13:46.4: 11.79 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.06
Forced photometry filter REJECTED candidate at 23:16:24.80 +54:13:46.4: ref_mag=11.95 +/- 0.06 new_mean_mag=11.7182 delta=0.24 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:41.33 +54:51:10.7: 12.26 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:41.33 +54:51:10.7: 11.97 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.07
Forced photometry filter REJECTED candidate at 23:16:41.33 +54:51:10.7: ref_mag=12.10 +/- 0.07 new_mean_mag=11.8183 delta=0.28 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:06.06 +56:05:25.4: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:06.06 +56:05:25.4: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:03.10 +55:02:06.5: 12.19 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:03.10 +55:02:06.5: 11.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.05
Forced photometry filter REJECTED candidate at 23:36:03.10 +55:02:06.5: ref_mag=12.07 +/- 0.05 new_mean_mag=11.5132 delta=0.55 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:44.42 +55:58:25.7: 13.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:44.42 +55:58:25.7: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:01.37 +54:47:45.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:01.37 +54:47:45.0: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:46.84 +54:35:20.7: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:30.85 +56:43:30.3: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:46.84 +54:35:20.7: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:30.85 +56:43:30.3: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:37.54 +55:36:21.9: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:07.55 +55:23:53.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:37.54 +55:36:21.9: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:07.55 +55:23:53.7: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:30:38.15 +57:55:02.5: 10.70 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:31.11 +52:04:54.8: 12.82 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:30:38.15 +57:55:02.5: 10.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.58 +/- 0.02
Forced photometry filter REJECTED candidate at 00:30:38.15 +57:55:02.5: ref_mag=10.58 +/- 0.02 new_mean_mag=11.1721 delta=-0.59 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:31.11 +52:04:54.8: 12.37 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.09
Forced photometry filter KEPT candidate at 23:22:31.11 +52:04:54.8: ref_mag=12.53 +/- 0.09 new_mean_mag=11.6064 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:38.60 +53:54:05.1: 13.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:38.60 +53:54:05.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:28.14 +56:13:38.6: 10.55 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:38.99 +54:02:34.6: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:28.14 +56:13:38.6: 10.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.39 +/- 0.01
Forced photometry filter REJECTED candidate at 23:56:28.14 +56:13:38.6: ref_mag=10.39 +/- 0.01 new_mean_mag=11.2069 delta=-0.82 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:38.99 +54:02:34.6: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:10.72 +54:09:43.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:10.72 +54:09:43.9: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:33.15 +56:44:32.1: 12.97 +/- 0.26 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:33.15 +56:44:32.1: 12.60 +/- 0.21 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.16
Forced photometry filter KEPT candidate at 23:56:33.15 +56:44:32.1: ref_mag=12.75 +/- 0.16 new_mean_mag=10.9499 delta=1.80 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:41.12 +54:49:12.3: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:41.12 +54:49:12.3: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:40.97 +54:16:19.0: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:40.97 +54:16:19.0: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:23.31 +57:13:12.8: 13.72 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:23.31 +57:13:12.8: 13.59 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.72 +/- 0.35
Forced photometry filter KEPT candidate at 23:28:23.31 +57:13:12.8: ref_mag=13.72 +/- 0.35 new_mean_mag=11.1348 delta=2.58 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:35.90 +55:20:55.7: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:35.90 +55:20:55.7: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:52.71 +53:45:16.2: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:52.71 +53:45:16.2: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:02.61 +56:51:39.2: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:02.61 +56:51:39.2: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:56.64 +53:20:37.4: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:56.64 +53:20:37.4: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:46.56 +55:59:21.1: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:46.56 +55:59:21.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:34.91 +54:31:30.6: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:14.43 +55:23:13.6: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:34.91 +54:31:30.6: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:14.43 +55:23:13.6: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:00.25 +56:28:03.4: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:00.25 +56:28:03.4: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:10.43 +52:52:20.3: 13.14 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:10.43 +52:52:20.3: 12.86 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.14
Forced photometry filter KEPT candidate at 23:33:10.43 +52:52:20.3: ref_mag=12.99 +/- 0.14 new_mean_mag=10.3902 delta=2.60 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:46.37 +55:43:11.4: 13.53 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:46.37 +55:43:11.4: 12.99 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.19
Forced photometry filter KEPT candidate at 23:19:46.37 +55:43:11.4: ref_mag=13.18 +/- 0.19 new_mean_mag=10.3132 delta=2.86 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:32.74 +50:40:33.3: 13.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:32.74 +50:40:33.3: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:26.38 +49:36:02.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:19.64 +53:12:02.5: 13.19 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:26.38 +49:36:02.3: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:19.64 +53:12:02.5: 13.10 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.15
Forced photometry filter KEPT candidate at 00:15:19.64 +53:12:02.5: ref_mag=13.15 +/- 0.15 new_mean_mag=9.5787 delta=3.57 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:52.60 +52:57:57.5: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:57.79 +55:40:09.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:52.60 +52:57:57.5: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:57.79 +55:40:09.9: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:10.42 +55:05:29.1: 13.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:10.42 +55:05:29.1: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:55.51 +56:28:28.8: 10.77 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:55.51 +56:28:28.8: 10.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.61 +/- 0.03
Forced photometry filter REJECTED candidate at 23:57:55.51 +56:28:28.8: ref_mag=10.61 +/- 0.03 new_mean_mag=10.9032 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:38.92 +53:34:20.1: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:38.92 +53:34:20.1: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:46.84 +52:18:46.0: 13.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:46.84 +52:18:46.0: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:04.95 +55:05:34.0: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:04.95 +55:05:34.0: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:56.52 +53:10:40.5: 9.67 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:56.52 +53:10:40.5: 9.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.41 +/- 0.01
Forced photometry filter REJECTED candidate at 23:17:56.52 +53:10:40.5: ref_mag=9.41 +/- 0.01 new_mean_mag=11.4495 delta=-2.04 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:48:29.72 +51:25:24.1: 12.17 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:48:29.72 +51:25:24.1: 12.00 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.06
Forced photometry filter REJECTED candidate at 23:48:29.72 +51:25:24.1: ref_mag=12.08 +/- 0.06 new_mean_mag=11.2712 delta=0.81 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:52.61 +52:09:34.7: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:52.61 +52:09:34.7: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:13.28 +52:06:50.2: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:17.52 +57:05:09.7: 13.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:13.28 +52:06:50.2: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:17.52 +57:05:09.7: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:51.47 +55:18:27.4: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:51.47 +55:18:27.4: 13.52 +/- 0.36 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.36
Forced photometry filter KEPT candidate at 23:11:51.47 +55:18:27.4: ref_mag=13.52 +/- 0.36 new_mean_mag=11.7137 delta=1.80 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:32.33 +49:52:16.9: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:28.16 +49:20:12.3: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:32.33 +49:52:16.9: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:28.16 +49:20:12.3: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:50.00 +54:40:25.9: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:50.00 +54:40:25.9: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:24.02 +51:39:58.0: 13.23 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:24.02 +51:39:58.0: 13.06 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.15
Forced photometry filter KEPT candidate at 23:29:24.02 +51:39:58.0: ref_mag=13.14 +/- 0.15 new_mean_mag=11.6722 delta=1.47 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:32.79 +49:44:27.7: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:53.22 +54:29:08.3: 13.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:32.79 +49:44:27.7: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:53.22 +54:29:08.3: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:08.61 +51:40:42.4: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:13.53 +57:25:56.5: 9.47 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:08.61 +51:40:42.4: 13.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:13.53 +57:25:56.5: 9.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.29 +/- 0.00
Forced photometry filter REJECTED candidate at 00:00:13.53 +57:25:56.5: ref_mag=9.29 +/- 0.00 new_mean_mag=11.6565 delta=-2.37 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:29.87 +55:32:14.0: 13.07 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:08.21 +54:02:57.3: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:29.87 +55:32:14.0: 13.24 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.20
Forced photometry filter KEPT candidate at 23:20:29.87 +55:32:14.0: ref_mag=13.13 +/- 0.20 new_mean_mag=11.9448 delta=1.18 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:08.21 +54:02:57.3: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:05.99 +55:55:40.1: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:05.99 +55:55:40.1: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:17:29.54 +52:31:56.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:45.13 +49:15:32.4: 13.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:17:29.54 +52:31:56.9: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:45.13 +49:15:32.4: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:27.82 +53:49:27.9: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:27.82 +53:49:27.9: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:37.19 +54:30:45.7: 13.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:37.19 +54:30:45.7: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:33.12 +54:04:33.4: 13.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:33.12 +54:04:33.4: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:19.57 +52:32:29.0: 13.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:19.57 +52:32:29.0: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:52.93 +50:45:40.4: 11.97 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:52.93 +50:45:40.4: 11.91 +/- 0.07 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.05
Forced photometry filter REJECTED candidate at 23:29:52.93 +50:45:40.4: ref_mag=11.94 +/- 0.05 new_mean_mag=12.0040 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:15.25 +51:14:31.0: 13.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:16.69 +54:35:03.8: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:15.25 +51:14:31.0: 13.22 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.24
Forced photometry filter KEPT candidate at 23:29:15.25 +51:14:31.0: ref_mag=13.22 +/- 0.24 new_mean_mag=11.9360 delta=1.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:16.69 +54:35:03.8: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:10:04.64 +50:47:20.7: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:10:04.64 +50:47:20.7: 13.41 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.28
Forced photometry filter KEPT candidate at 00:10:04.64 +50:47:20.7: ref_mag=13.41 +/- 0.28 new_mean_mag=11.8079 delta=1.60 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:39.89 +56:40:37.1: 12.09 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:39.89 +56:40:37.1: 11.86 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.06
Forced photometry filter REJECTED candidate at 23:49:39.89 +56:40:37.1: ref_mag=11.96 +/- 0.06 new_mean_mag=11.9871 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:12.77 +54:21:37.6: 11.96 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:11.65 +54:35:58.1: 12.81 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:12.77 +54:21:37.6: 11.80 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.06
Forced photometry filter REJECTED candidate at 23:52:12.77 +54:21:37.6: ref_mag=11.88 +/- 0.06 new_mean_mag=11.7902 delta=0.09 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:11.65 +54:35:58.1: 12.39 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.10
Forced photometry filter REJECTED candidate at 23:55:11.65 +54:35:58.1: ref_mag=12.55 +/- 0.10 new_mean_mag=11.9247 delta=0.63 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:56.83 +54:01:31.7: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:56.83 +54:01:31.7: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:51.16 +53:03:56.8: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:51.16 +53:03:56.8: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:36.22 +56:16:48.6: 13.15 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:36.22 +56:16:48.6: 13.02 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.14
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:46.07 +57:25:47.2: 13.71 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 23:56:36.22 +56:16:48.6: ref_mag=13.08 +/- 0.14 new_mean_mag=12.1228 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:18.97 +57:40:50.0: 13.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:46.07 +57:25:47.2: 13.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:18.97 +57:40:50.0: 13.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:21.38 +56:59:47.8: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:21.38 +56:59:47.8: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:59.11 +55:52:57.5: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:13:59.11 +55:52:57.5: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:19.64 +55:04:30.4: 13.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:19.64 +55:04:30.4: 13.40 +/- 0.34 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.34
Forced photometry filter KEPT candidate at 00:22:19.64 +55:04:30.4: ref_mag=13.40 +/- 0.34 new_mean_mag=12.2249 delta=1.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:08.11 +56:23:04.6: 10.45 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:08.11 +56:23:04.6: 10.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.29 +/- 0.01
Forced photometry filter REJECTED candidate at 23:56:08.11 +56:23:04.6: ref_mag=10.29 +/- 0.01 new_mean_mag=12.3106 delta=-2.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:06.62 +54:45:02.9: 13.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:43.23 +54:09:55.3: 13.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:06.62 +54:45:02.9: 13.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:34.29 +54:58:11.5: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:43.23 +54:09:55.3: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:50.86 +57:26:58.1: 13.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:34.29 +54:58:11.5: 13.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:50.86 +57:26:58.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:00.29 +52:15:00.1: 13.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:00.29 +52:15:00.1: 13.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:33:17.55 +55:45:53.1: 13.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:33:17.55 +55:45:53.1: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:44.79 +55:30:17.5: 12.62 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:44.79 +55:30:17.5: 12.41 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.09
Forced photometry filter REJECTED candidate at 23:52:44.79 +55:30:17.5: ref_mag=12.51 +/- 0.09 new_mean_mag=12.3951 delta=0.11 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:30.03 +55:43:32.3: 12.11 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:30.03 +55:43:32.3: 11.97 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.06
Forced photometry filter REJECTED candidate at 23:50:30.03 +55:43:32.3: ref_mag=12.04 +/- 0.06 new_mean_mag=12.5305 delta=-0.49 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:08.83 +55:55:18.4: 12.84 +/- 0.17 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:08.83 +55:55:18.4: 12.40 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.10
Forced photometry filter REJECTED candidate at 23:52:08.83 +55:55:18.4: ref_mag=12.56 +/- 0.10 new_mean_mag=12.3500 delta=0.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:37.24 +53:31:24.4: 13.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:37.24 +53:31:24.4: 13.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:01.26 +49:55:45.1: 13.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:01.26 +49:55:45.1: 13.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:11.96 +50:00:11.8: 13.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:11.96 +50:00:11.8: 13.46 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out219245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236891.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out236910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237188.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out237289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25587.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 240s
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: 132s
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Considering the candidate 235438_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235438_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 235439_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235439_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 235442_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235442_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235445_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235445_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 235450_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235450_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235453_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235453_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235457_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235457_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235460_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235460_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 235461_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235461_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 235470_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235470_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 235478_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235478_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235491_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235491_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235494_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235494_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235498_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235498_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235506_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235506_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 235520_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235520_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235522_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235522_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235526_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235526_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235532_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235532_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235543_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235543_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235546_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235546_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235548_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235548_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235553_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235553_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235554_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235554_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235555_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235555_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235559_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235559_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235571_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235571_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235572_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235572_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235574_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235574_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235576_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235576_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235578_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235578_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235580_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235580_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235581_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235581_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235585_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235585_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235591_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235591_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235606_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235606_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235611_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235611_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235614_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235614_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235618_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235618_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235624_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235624_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:41:11.82 +57:06:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235626_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235626_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235631_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235631_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235632_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235632_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235634_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235634_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235635_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235635_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:37:32.70 +52:48:38.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235636_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235636_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235637_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235637_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235638_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235638_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235639_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235639_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235642_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235642_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235649_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235649_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235659_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235659_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235670_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235670_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235673_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235673_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:41:57.33 +51:42:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235674_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235674_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235678_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235678_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235679_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235679_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235681_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235681_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235685_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235685_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235686_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235686_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235695_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235695_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235696_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235696_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:48:17.69 +53:25:48.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235699_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235699_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235700_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235700_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235702_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235702_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:08:36.82 +55:38:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235705_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235705_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235707_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235707_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235712_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235712_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:31:00.25 +57:24:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235713_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235713_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:07:21.16 +55:34:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235727_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235727_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:22:17.86 +54:20:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235732_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235732_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235736_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235736_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235739_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235739_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235750_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235750_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235753_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235753_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235754_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235754_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:56:55.50 +55:04:12.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235756_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235756_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235757_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235757_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:34:43.34 +51:31:34.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235765_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235765_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:25:16.21 +53:39:16.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235766_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235766_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235772_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235772_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:57:16.01 +56:30:05.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235774_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235774_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 235775_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235775_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235778_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235778_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:37:09.99 +56:33:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235779_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235779_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235780_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235780_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:08:45.68 +53:03:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235788_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235788_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235791_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235791_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235792_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235792_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 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 235794_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235794_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235795_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235795_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235801_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235801_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235805_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235805_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 235810_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235810_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:55:04.11 +54:11:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235813_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235813_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:04:21.95 +51:49:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235818_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235818_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:57:02.03 +56:44:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235821_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235821_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235826_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235826_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 235828_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235828_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235829_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235829_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:57:55.30 +56:42:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235832_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235832_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:45:59.24 +56:53:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235835_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235835_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:14:15.39 +54:02:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235841_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235841_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:06:20.97 +56:11:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235842_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235842_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235844_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235844_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235845_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235845_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235849_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235849_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235850_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235850_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235851_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235851_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235853_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235853_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235855_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235855_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:14:23.69 +54:44:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235856_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235856_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235858_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235858_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235861_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235861_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235862_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235862_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:46:28.75 +55:12:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235865_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235865_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:51:56.64 +53:07:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235870_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235870_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235872_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235872_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235875_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235875_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:56:00.03 +52:01:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235876_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235876_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235877_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235877_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235880_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235880_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235882_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235882_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235885_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235885_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 235886_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235886_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235890_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 235890_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:46:46.58 +51:02:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235892_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 235892_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 236039_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236039_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236185_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236185_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:13:11.40 +57:10:46.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 236210_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236210_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:59:23.85 +50:31:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236257_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236257_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:47:14.69 +57:25:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236270_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236270_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:43:56.61 +56:20:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236309_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236309_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:20:34.12 +52:06:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236320_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236320_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236348_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236348_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 236357_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236357_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
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Considering the candidate 236390_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236390_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:32:37.71 +54:45:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236398_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236398_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:25:46.00 +57:59:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236409_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236409_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236433_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236433_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:16:20.72 +53:35:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236461_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236461_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:23:25.89 +55:49:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236464_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236464_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236487_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236487_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:56:32.08 +53:44:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236505_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236505_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236515_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236515_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:57:59.41 +50:26:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236519_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236519_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:41:07.31 +51:33:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 236527_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236527_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236545_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236545_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:58:51.70 +54:42:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236564_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236564_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:28:20.91 +54:48:23.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236566_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236566_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236576_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236576_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:43:15.38 +51:56:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236583_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236583_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:18:03.85 +49:50:44.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236595_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236595_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:49:47.23 +56:38:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236600_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236600_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:38:44.17 +56:37:47.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236613_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236613_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236617_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236617_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236625_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236625_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:13:03.02 +49:56:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236629_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236629_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236631_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236631_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:32:34.96 +54:04:40.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236637_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236637_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:57:58.30 +50:27:12.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236646_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236646_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:24:57.67 +53:01:58.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236656_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236656_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:11:49.41 +54:49:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236672_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236672_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:37:53.31 +50:55:26.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236676_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236676_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:20:12.47 +50:06:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236685_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236685_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:21:17.00 +55:55:01.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236688_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236688_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:32:51.65 +51:53:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236698_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236698_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:08:02.11 +53:40:08.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236702_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236702_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:27:19.53 +49:58:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236706_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236706_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:59:00.37 +53:16:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236707_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236707_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:52:01.85 +50:05:57.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236709_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236709_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:25:48.65 +57:59:16.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236716_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236716_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:47:01.70 +57:24:59.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236720_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236720_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236735_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236735_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236736_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236736_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:29:50.23 +54:38:53.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236747_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236747_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236763_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236763_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:31:40.42 +54:09:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236769_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236769_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:38:36.44 +57:11:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236780_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236780_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:22:46.45 +56:26:54.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236782_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236782_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236793_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236793_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236795_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236795_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236797_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236797_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:40:53.39 +54:25:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236813_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236813_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:48:26.67 +54:40:39.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236817_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236817_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:14:01.18 +55:16:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236822_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236822_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:47:42.38 +56:51:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236826_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236826_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:32:59.55 +57:36:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236831_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236831_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236839_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236839_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236840_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236840_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:44:19.97 +57:20:44.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236844_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236844_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:20:15.57 +57:50:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236869_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236869_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:47:36.70 +55:14:21.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236874_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236874_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:00:23.25 +56:50:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236891_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236891_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236894_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236894_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236896_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236896_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:54:44.66 +53:43:03.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236899_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236899_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236910_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236910_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236913_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236913_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236921_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236921_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:32:31.50 +51:13:06.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236924_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236924_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:07:40.63 +57:11:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236928_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236928_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:02:24.69 +55:25:33.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236930_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236930_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:12:53.14 +55:50:48.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236934_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236934_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236949_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236949_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:51:04.23 +51:22:54.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236953_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236953_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:55:33.19 +52:42:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236958_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236958_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:36:15.15 +49:55:40.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236964_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236964_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:50:23.49 +54:12:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236967_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236967_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:12:07.26 +53:36:07.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236968_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236968_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:24:30.85 +56:57:00.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236970_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236970_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236973_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236973_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236975_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236975_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236976_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236976_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:14:16.70 +56:52:52.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236990_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236990_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:00:26.38 +55:27:29.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236991_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236991_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236996_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 236996_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:31:16.90 +57:14:11.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236997_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 236997_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237001_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237001_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237004_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237004_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237021_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237021_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237038_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237038_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:00:57.52 +53:16:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237047_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237047_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237050_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237050_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237070_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237070_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:56:17.54 +53:09:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237090_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237090_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:02:26.98 +54:33:03.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237100_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237100_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237102_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237102_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:51:00.11 +54:43:19.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237120_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237120_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237137_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237137_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:25:09.07 +52:50:46.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237144_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237144_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237148_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237148_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237186_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237186_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237188_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237188_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237236_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237236_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:51:28.10 +51:30:29.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237247_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237247_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237289_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237289_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237305_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237305_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237312_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237312_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237327_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237327_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237330_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237330_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237348_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237348_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237353_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237353_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237355_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237355_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237360_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237360_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237363_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237363_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237374_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237374_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237383_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 237383_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237454_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 237454_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197606_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 197606_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:44:31.91 +56:34:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219245_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 219245_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219159_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 219159_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:27:11.68 +53:53:45.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46841_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 46841_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:09:36.48 +51:34:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
Preparing report for the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179100_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101
The candidate 179100_fd_Cas-04-Q2b1x1_2026-07-17_23-18-36_20.00sec_5.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:15:50.73 +57:32:37.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 23s
make_report_in_HTML.sh TOTAL: 395s
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 ####
23:26:01.26 +49:55:45.1
23:44:16.80 +51:40:48.6
23:46:15.15 +52:45:10.8
23:44:58.72 +55:01:33.5
23:34:37.78 +53:35:38.7
23:35:32.87 +56:05:53.8
23:49:20.24 +55:31:33.7
00:04:12.88 +55:36:14.5
23:37:17.74 +55:33:07.6
23:36:49.02 +56:55:01.8
23:46:36.44 +54:09:45.1
23:16:56.98 +52:55:46.6
23:35:20.02 +54:55:24.7
23:27:40.51 +53:59:08.7
00:15:17.99 +53:07:48.6
00:00:21.26 +53:34:11.0
23:19:39.71 +53:12:18.9
23:45:47.67 +57:16:15.0
23:49:09.36 +57:30:17.1
00:09:01.30 +54:47:06.9
00:17:01.90 +57:24:20.9
00:31:04.38 +55:22:25.2
23:21:01.34 +54:13:16.2
23:19:14.60 +54:14:10.7
23:31:48.14 +56:54:18.1
23:34:43.94 +55:56:14.6
00:09:10.89 +54:30:27.4
00:11:25.03 +55:00:14.4
23:31:10.13 +52:06:28.4
23:54:15.97 +53:20:53.8
23:44:33.09 +53:02:41.1
23:10:11.92 +57:07:36.4
00:04:07.82 +56:06:30.8
23:30:56.70 +51:10:35.3
23:36:46.52 +53:03:07.8
23:57:35.32 +56:46:47.2
00:15:29.86 +57:39:49.5
23:21:40.85 +51:06:26.3
00:23:19.31 +56:00:17.1
23:39:31.73 +55:18:15.0
23:46:34.81 +51:28:31.5
00:22:56.82 +50:57:51.9
23:36:55.78 +54:03:09.9
23:43:23.43 +57:27:43.1
23:47:36.03 +55:28:07.4
23:27:32.45 +54:50:50.7
00:26:43.09 +57:15:38.6
23:46:38.85 +53:36:25.6
23:17:04.27 +54:39:05.6
23:28:21.63 +53:30:44.0
23:28:33.67 +53:36:15.8
23:19:36.59 +55:55:15.9
23:23:22.79 +53:36:20.4
00:19:06.06 +56:05:25.4
23:18:44.42 +55:58:25.7
23:29:01.37 +54:47:45.0
23:21:46.84 +54:35:20.7
00:14:30.85 +56:43:30.3
23:19:37.54 +55:36:21.9
23:11:07.55 +55:23:53.7
23:22:31.11 +52:04:54.8
23:58:38.60 +53:54:05.1
23:22:38.99 +54:02:34.6
23:14:10.72 +54:09:43.9
23:56:33.15 +56:44:32.1
23:12:41.12 +54:49:12.3
23:18:40.97 +54:16:19.0
23:28:23.31 +57:13:12.8
23:13:35.90 +55:20:55.7
23:36:52.71 +53:45:16.2
23:10:02.61 +56:51:39.2
23:18:56.64 +53:20:37.4
23:14:46.56 +55:59:21.1
23:18:34.91 +54:31:30.6
23:21:14.43 +55:23:13.6
23:19:00.25 +56:28:03.4
23:33:10.43 +52:52:20.3
23:19:46.37 +55:43:11.4
23:36:32.74 +50:40:33.3
23:27:26.38 +49:36:02.3
00:15:19.64 +53:12:02.5
23:15:52.60 +52:57:57.5
23:20:57.79 +55:40:09.9
23:23:10.42 +55:05:29.1
23:13:38.92 +53:34:20.1
23:28:46.84 +52:18:46.0
23:25:04.95 +55:05:34.0
23:56:52.61 +52:09:34.7
23:23:13.28 +52:06:50.2
23:12:17.52 +57:05:09.7
23:11:51.47 +55:18:27.4
23:30:32.33 +49:52:16.9
23:25:28.16 +49:20:12.3
23:41:50.00 +54:40:25.9
23:29:24.02 +51:39:58.0
23:34:32.79 +49:44:27.7
23:24:53.22 +54:29:08.3
23:41:08.61 +51:40:42.4
23:20:29.87 +55:32:14.0
23:34:08.21 +54:02:57.3
23:21:05.99 +55:55:40.1
23:17:29.54 +52:31:56.9
23:19:45.13 +49:15:32.4
23:28:27.82 +53:49:27.9
00:26:37.19 +54:30:45.7
23:15:33.12 +54:04:33.4
23:27:19.57 +52:32:29.0
23:29:15.25 +51:14:31.0
23:21:16.69 +54:35:03.8
00:10:04.64 +50:47:20.7
23:16:56.83 +54:01:31.7
23:25:51.16 +53:03:56.8
23:56:36.22 +56:16:48.6
23:42:46.07 +57:25:47.2
23:56:18.97 +57:40:50.0
23:10:21.38 +56:59:47.8
23:13:59.11 +55:52:57.5
00:22:19.64 +55:04:30.4
23:54:06.62 +54:45:02.9
23:16:43.23 +54:09:55.3
23:30:34.29 +54:58:11.5
23:57:50.86 +57:26:58.1
23:43:00.29 +52:15:00.1
23:33:17.55 +55:45:53.1
23:50:37.24 +53:31:24.4
23:21:11.96 +50:00:11.8
########### 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 ####
23:44:16.80 +51:40:48.6
23:46:15.15 +52:45:10.8
23:44:58.72 +55:01:33.5
23:34:37.78 +53:35:38.7
23:35:32.87 +56:05:53.8
23:49:20.24 +55:31:33.7
00:04:12.88 +55:36:14.5
23:37:17.74 +55:33:07.6
23:36:49.02 +56:55:01.8
23:46:36.44 +54:09:45.1
23:16:56.98 +52:55:46.6
23:35:20.02 +54:55:24.7
23:27:40.51 +53:59:08.7
00:15:17.99 +53:07:48.6
00:00:21.26 +53:34:11.0
23:19:39.71 +53:12:18.9
23:45:47.67 +57:16:15.0
23:49:09.36 +57:30:17.1
00:09:01.30 +54:47:06.9
00:17:01.90 +57:24:20.9
00:31:04.38 +55:22:25.2
23:21:01.34 +54:13:16.2
23:19:14.60 +54:14:10.7
23:31:48.14 +56:54:18.1
23:34:43.94 +55:56:14.6
00:09:10.89 +54:30:27.4
00:11:25.03 +55:00:14.4
23:31:10.13 +52:06:28.4
23:54:15.97 +53:20:53.8
23:44:33.09 +53:02:41.1
23:10:11.92 +57:07:36.4
00:04:07.82 +56:06:30.8
23:30:56.70 +51:10:35.3
23:36:46.52 +53:03:07.8
23:57:35.32 +56:46:47.2
00:15:29.86 +57:39:49.5
23:21:40.85 +51:06:26.3
00:23:19.31 +56:00:17.1
23:39:31.73 +55:18:15.0
23:46:34.81 +51:28:31.5
00:22:56.82 +50:57:51.9
23:36:55.78 +54:03:09.9
23:43:23.43 +57:27:43.1
23:47:36.03 +55:28:07.4
23:27:32.45 +54:50:50.7
00:26:43.09 +57:15:38.6
23:46:38.85 +53:36:25.6
23:17:04.27 +54:39:05.6
23:28:21.63 +53:30:44.0
23:28:33.67 +53:36:15.8
23:19:36.59 +55:55:15.9
23:23:22.79 +53:36:20.4
00:19:06.06 +56:05:25.4
23:18:44.42 +55:58:25.7
23:29:01.37 +54:47:45.0
23:21:46.84 +54:35:20.7
00:14:30.85 +56:43:30.3
23:19:37.54 +55:36:21.9
23:11:07.55 +55:23:53.7
23:22:31.11 +52:04:54.8
23:58:38.60 +53:54:05.1
23:22:38.99 +54:02:34.6
23:14:10.72 +54:09:43.9
23:56:33.15 +56:44:32.1
23:12:41.12 +54:49:12.3
23:18:40.97 +54:16:19.0
23:28:23.31 +57:13:12.8
23:13:35.90 +55:20:55.7
23:36:52.71 +53:45:16.2
23:10:02.61 +56:51:39.2
23:18:56.64 +53:20:37.4
23:14:46.56 +55:59:21.1
23:18:34.91 +54:31:30.6
23:21:14.43 +55:23:13.6
23:19:00.25 +56:28:03.4
23:33:10.43 +52:52:20.3
23:19:46.37 +55:43:11.4
23:36:32.74 +50:40:33.3
23:27:26.38 +49:36:02.3
00:15:19.64 +53:12:02.5
23:15:52.60 +52:57:57.5
23:20:57.79 +55:40:09.9
23:23:10.42 +55:05:29.1
23:13:38.92 +53:34:20.1
23:28:46.84 +52:18:46.0
23:25:04.95 +55:05:34.0
23:56:52.61 +52:09:34.7
23:23:13.28 +52:06:50.2
23:12:17.52 +57:05:09.7
23:11:51.47 +55:18:27.4
23:30:32.33 +49:52:16.9
23:25:28.16 +49:20:12.3
23:41:50.00 +54:40:25.9
23:29:24.02 +51:39:58.0
23:34:32.79 +49:44:27.7
23:24:53.22 +54:29:08.3
23:41:08.61 +51:40:42.4
23:20:29.87 +55:32:14.0
23:34:08.21 +54:02:57.3
23:21:05.99 +55:55:40.1
23:17:29.54 +52:31:56.9
23:19:45.13 +49:15:32.4
23:28:27.82 +53:49:27.9
00:26:37.19 +54:30:45.7
23:15:33.12 +54:04:33.4
23:27:19.57 +52:32:29.0
23:29:15.25 +51:14:31.0
23:21:16.69 +54:35:03.8
00:10:04.64 +50:47:20.7
23:16:56.83 +54:01:31.7
23:25:51.16 +53:03:56.8
23:56:36.22 +56:16:48.6
23:42:46.07 +57:25:47.2
23:56:18.97 +57:40:50.0
23:10:21.38 +56:59:47.8
23:13:59.11 +55:52:57.5
00:22:19.64 +55:04:30.4
23:54:06.62 +54:45:02.9
23:16:43.23 +54:09:55.3
23:30:34.29 +54:58:11.5
23:57:50.86 +57:26:58.1
23:43:00.29 +52:15:00.1
23:33:17.55 +55:45:53.1
23:50:37.24 +53:31:24.4
23:26:01.26 +49:55:45.1
23:21:11.96 +50:00:11.8
###################################################################################
23:44:16.80 +51:40:48.6 -- not an asteroid (will add it to exclusion list)
23:46:15.15 +52:45:10.8 -- not an asteroid (will add it to exclusion list)
23:44:58.72 +55:01:33.5 -- not an asteroid (will add it to exclusion list)
23:34:37.78 +53:35:38.7 -- not an asteroid (will add it to exclusion list)
23:35:32.87 +56:05:53.8 -- not an asteroid (will add it to exclusion list)
23:49:20.24 +55:31:33.7 -- not an asteroid (will add it to exclusion list)
00:04:12.88 +55:36:14.5 -- not an asteroid (will add it to exclusion list)
23:37:17.74 +55:33:07.6 -- not an asteroid (will add it to exclusion list)
23:36:49.02 +56:55:01.8 -- not an asteroid (will add it to exclusion list)
23:46:36.44 +54:09:45.1 -- not an asteroid (will add it to exclusion list)
23:16:56.98 +52:55:46.6 -- not an asteroid (will add it to exclusion list)
23:35:20.02 +54:55:24.7 -- not an asteroid (will add it to exclusion list)
23:27:40.51 +53:59:08.7 -- not an asteroid (will add it to exclusion list)
00:15:17.99 +53:07:48.6 -- not an asteroid (will add it to exclusion list)
00:00:21.26 +53:34:11.0 -- not an asteroid (will add it to exclusion list)
23:19:39.71 +53:12:18.9 -- not an asteroid (will add it to exclusion list)
23:45:47.67 +57:16:15.0 -- not an asteroid (will add it to exclusion list)
23:49:09.36 +57:30:17.1 -- not an asteroid (will add it to exclusion list)
00:09:01.30 +54:47:06.9 -- not an asteroid (will add it to exclusion list)
00:17:01.90 +57:24:20.9 -- not an asteroid (will add it to exclusion list)
00:31:04.38 +55:22:25.2 -- not an asteroid (will add it to exclusion list)
23:21:01.34 +54:13:16.2 -- not an asteroid (will add it to exclusion list)
23:19:14.60 +54:14:10.7 -- not an asteroid (will add it to exclusion list)
23:31:48.14 +56:54:18.1 -- not an asteroid (will add it to exclusion list)
23:34:43.94 +55:56:14.6 -- not an asteroid (will add it to exclusion list)
00:09:10.89 +54:30:27.4 -- not an asteroid (will add it to exclusion list)
00:11:25.03 +55:00:14.4 -- not an asteroid (will add it to exclusion list)
23:31:10.13 +52:06:28.4 -- not an asteroid (will add it to exclusion list)
23:54:15.97 +53:20:53.8 -- not an asteroid (will add it to exclusion list)
23:44:33.09 +53:02:41.1 -- not an asteroid (will add it to exclusion list)
23:10:11.92 +57:07:36.4 -- not an asteroid (will add it to exclusion list)
00:04:07.82 +56:06:30.8 -- not an asteroid (will add it to exclusion list)
23:30:56.70 +51:10:35.3 -- not an asteroid (will add it to exclusion list)
23:36:46.52 +53:03:07.8 -- not an asteroid (will add it to exclusion list)
23:57:35.32 +56:46:47.2 -- not an asteroid (will add it to exclusion list)
00:15:29.86 +57:39:49.5 -- not an asteroid (will add it to exclusion list)
23:21:40.85 +51:06:26.3 -- not an asteroid (will add it to exclusion list)
00:23:19.31 +56:00:17.1 -- not an asteroid (will add it to exclusion list)
23:39:31.73 +55:18:15.0 -- not an asteroid (will add it to exclusion list)
23:46:34.81 +51:28:31.5 -- not an asteroid (will add it to exclusion list)
00:22:56.82 +50:57:51.9 -- not an asteroid (will add it to exclusion list)
23:36:55.78 +54:03:09.9 -- not an asteroid (will add it to exclusion list)
23:43:23.43 +57:27:43.1 -- not an asteroid (will add it to exclusion list)
23:47:36.03 +55:28:07.4 -- not an asteroid (will add it to exclusion list)
23:27:32.45 +54:50:50.7 -- not an asteroid (will add it to exclusion list)
00:26:43.09 +57:15:38.6 -- not an asteroid (will add it to exclusion list)
23:46:38.85 +53:36:25.6 -- not an asteroid (will add it to exclusion list)
23:17:04.27 +54:39:05.6 -- not an asteroid (will add it to exclusion list)
23:28:21.63 +53:30:44.0 -- not an asteroid (will add it to exclusion list)
23:28:33.67 +53:36:15.8 -- not an asteroid (will add it to exclusion list)
23:19:36.59 +55:55:15.9 -- not an asteroid (will add it to exclusion list)
23:23:22.79 +53:36:20.4 -- not an asteroid (will add it to exclusion list)
00:19:06.06 +56:05:25.4 -- not an asteroid (will add it to exclusion list)
23:18:44.42 +55:58:25.7 -- not an asteroid (will add it to exclusion list)
23:29:01.37 +54:47:45.0 -- not an asteroid (will add it to exclusion list)
23:21:46.84 +54:35:20.7 -- not an asteroid (will add it to exclusion list)
00:14:30.85 +56:43:30.3 -- not an asteroid (will add it to exclusion list)
23:19:37.54 +55:36:21.9 -- not an asteroid (will add it to exclusion list)
23:11:07.55 +55:23:53.7 -- not an asteroid (will add it to exclusion list)
23:22:31.11 +52:04:54.8 -- not an asteroid (will add it to exclusion list)
23:58:38.60 +53:54:05.1 -- not an asteroid (will add it to exclusion list)
23:22:38.99 +54:02:34.6 -- not an asteroid (will add it to exclusion list)
23:14:10.72 +54:09:43.9 -- not an asteroid (will add it to exclusion list)
23:56:33.15 +56:44:32.1 -- not an asteroid (will add it to exclusion list)
23:12:41.12 +54:49:12.3 -- not an asteroid (will add it to exclusion list)
23:18:40.97 +54:16:19.0 -- not an asteroid (will add it to exclusion list)
23:28:23.31 +57:13:12.8 -- not an asteroid (will add it to exclusion list)
23:13:35.90 +55:20:55.7 -- not an asteroid (will add it to exclusion list)
23:36:52.71 +53:45:16.2 -- not an asteroid (will add it to exclusion list)
23:10:02.61 +56:51:39.2 -- not an asteroid (will add it to exclusion list)
23:18:56.64 +53:20:37.4 -- not an asteroid (will add it to exclusion list)
23:14:46.56 +55:59:21.1 -- not an asteroid (will add it to exclusion list)
23:18:34.91 +54:31:30.6 -- not an asteroid (will add it to exclusion list)
23:21:14.43 +55:23:13.6 -- not an asteroid (will add it to exclusion list)
23:19:00.25 +56:28:03.4 -- not an asteroid (will add it to exclusion list)
23:33:10.43 +52:52:20.3 -- not an asteroid (will add it to exclusion list)
23:19:46.37 +55:43:11.4 -- not an asteroid (will add it to exclusion list)
23:36:32.74 +50:40:33.3 -- not an asteroid (will add it to exclusion list)
23:27:26.38 +49:36:02.3 -- not an asteroid (will add it to exclusion list)
00:15:19.64 +53:12:02.5 -- not an asteroid (will add it to exclusion list)
23:15:52.60 +52:57:57.5 -- not an asteroid (will add it to exclusion list)
23:20:57.79 +55:40:09.9 -- not an asteroid (will add it to exclusion list)
23:23:10.42 +55:05:29.1 -- not an asteroid (will add it to exclusion list)
23:13:38.92 +53:34:20.1 -- not an asteroid (will add it to exclusion list)
23:28:46.84 +52:18:46.0 -- not an asteroid (will add it to exclusion list)
23:25:04.95 +55:05:34.0 -- not an asteroid (will add it to exclusion list)
23:56:52.61 +52:09:34.7 -- not an asteroid (will add it to exclusion list)
23:23:13.28 +52:06:50.2 -- not an asteroid (will add it to exclusion list)
23:12:17.52 +57:05:09.7 -- not an asteroid (will add it to exclusion list)
23:11:51.47 +55:18:27.4 -- not an asteroid (will add it to exclusion list)
23:30:32.33 +49:52:16.9 -- not an asteroid (will add it to exclusion list)
23:25:28.16 +49:20:12.3 -- not an asteroid (will add it to exclusion list)
23:41:50.00 +54:40:25.9 -- not an asteroid (will add it to exclusion list)
23:29:24.02 +51:39:58.0 -- not an asteroid (will add it to exclusion list)
23:34:32.79 +49:44:27.7 -- not an asteroid (will add it to exclusion list)
23:24:53.22 +54:29:08.3 -- not an asteroid (will add it to exclusion list)
23:41:08.61 +51:40:42.4 -- not an asteroid (will add it to exclusion list)
23:20:29.87 +55:32:14.0 -- not an asteroid (will add it to exclusion list)
23:34:08.21 +54:02:57.3 -- not an asteroid (will add it to exclusion list)
23:21:05.99 +55:55:40.1 -- not an asteroid (will add it to exclusion list)
23:17:29.54 +52:31:56.9 -- not an asteroid (will add it to exclusion list)
23:19:45.13 +49:15:32.4 -- not an asteroid (will add it to exclusion list)
23:28:27.82 +53:49:27.9 -- not an asteroid (will add it to exclusion list)
00:26:37.19 +54:30:45.7 -- not an asteroid (will add it to exclusion list)
23:15:33.12 +54:04:33.4 -- not an asteroid (will add it to exclusion list)
23:27:19.57 +52:32:29.0 -- not an asteroid (will add it to exclusion list)
23:29:15.25 +51:14:31.0 -- not an asteroid (will add it to exclusion list)
23:21:16.69 +54:35:03.8 -- not an asteroid (will add it to exclusion list)
00:10:04.64 +50:47:20.7 -- not an asteroid (will add it to exclusion list)
23:16:56.83 +54:01:31.7 -- not an asteroid (will add it to exclusion list)
23:25:51.16 +53:03:56.8 -- not an asteroid (will add it to exclusion list)
23:56:36.22 +56:16:48.6 -- not an asteroid (will add it to exclusion list)
23:42:46.07 +57:25:47.2 -- not an asteroid (will add it to exclusion list)
23:56:18.97 +57:40:50.0 -- not an asteroid (will add it to exclusion list)
23:10:21.38 +56:59:47.8 -- not an asteroid (will add it to exclusion list)
23:13:59.11 +55:52:57.5 -- not an asteroid (will add it to exclusion list)
00:22:19.64 +55:04:30.4 -- not an asteroid (will add it to exclusion list)
23:54:06.62 +54:45:02.9 -- not an asteroid (will add it to exclusion list)
23:16:43.23 +54:09:55.3 -- not an asteroid (will add it to exclusion list)
23:30:34.29 +54:58:11.5 -- not an asteroid (will add it to exclusion list)
23:57:50.86 +57:26:58.1 -- not an asteroid (will add it to exclusion list)
23:43:00.29 +52:15:00.1 -- not an asteroid (will add it to exclusion list)
23:33:17.55 +55:45:53.1 -- not an asteroid (will add it to exclusion list)
23:50:37.24 +53:31:24.4 -- not an asteroid (will add it to exclusion list)
23:26:01.26 +49:55:45.1 -- not an asteroid (will add it to exclusion list)
23:21:11.96 +50:00:11.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:21.26 +53:34:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:07.82 +56:06:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:12.88 +55:36:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:01.30 +54:47:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:10.89 +54:30:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:04.64 +50:47:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:25.03 +55:00:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:30.85 +56:43:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:17.99 +53:07:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:19.64 +53:12:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:29.86 +57:39:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:01.90 +57:24:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:06.06 +56:05:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:19.64 +55:04:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:56.82 +50:57:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:19.31 +56:00:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:37.19 +54:30:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:43.09 +57:15:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:04.38 +55:22:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:02.61 +56:51:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:11.92 +57:07:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:21.38 +56:59:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:07.55 +55:23:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:51.47 +55:18:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:17.52 +57:05:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:41.12 +54:49:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:35.90 +55:20:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:38.92 +53:34:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:59.11 +55:52:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:10.72 +54:09:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:46.56 +55:59:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:33.12 +54:04:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:52.60 +52:57:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:43.23 +54:09:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:56.83 +54:01:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:56.98 +52:55:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:04.27 +54:39:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:29.54 +52:31:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:34.91 +54:31:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:40.97 +54:16:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:44.42 +55:58:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:56.64 +53:20:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:00.25 +56:28:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:14.60 +54:14:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:36.59 +55:55:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:37.54 +55:36:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:39.71 +53:12:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:45.13 +49:15:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:46.37 +55:43:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:29.87 +55:32:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:57.79 +55:40:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:01.34 +54:13:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:05.99 +55:55:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:11.96 +50:00:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:14.43 +55:23:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:16.69 +54:35:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:40.85 +51:06:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:46.84 +54:35:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:31.11 +52:04:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:38.99 +54:02:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:10.42 +55:05:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:13.28 +52:06:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:22.79 +53:36:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:53.22 +54:29:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:04.95 +55:05:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:28.16 +49:20:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:51.16 +53:03:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:01.26 +49:55:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:19.57 +52:32:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:26.38 +49:36:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:32.45 +54:50:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:40.51 +53:59:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:21.63 +53:30:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:23.31 +57:13:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:27.82 +53:49:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:33.67 +53:36:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:46.84 +52:18:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:01.37 +54:47:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:15.25 +51:14:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:24.02 +51:39:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:32.33 +49:52:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:34.29 +54:58:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:56.70 +51:10:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:10.13 +52:06:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:48.14 +56:54:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:10.43 +52:52:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:17.55 +55:45:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:08.21 +54:02:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:32.79 +49:44:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:37.78 +53:35:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:43.94 +55:56:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:20.02 +54:55:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:32.87 +56:05:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:32.74 +50:40:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:46.52 +53:03:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:49.02 +56:55:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:52.71 +53:45:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:55.78 +54:03:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:17.74 +55:33:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:31.73 +55:18:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:08.61 +51:40:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:50.00 +54:40:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:46.07 +57:25:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:00.29 +52:15:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:23.43 +57:27:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:16.80 +51:40:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:33.09 +53:02:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:58.72 +55:01:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:47.67 +57:16:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:15.15 +52:45:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:34.81 +51:28:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:36.44 +54:09:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:38.85 +53:36:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:36.03 +55:28:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:09.36 +57:30:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:20.24 +55:31:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:37.24 +53:31:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:06.62 +54:45:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:15.97 +53:20:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:18.97 +57:40:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:33.15 +56:44:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:36.22 +56:16:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:52.61 +52:09:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:35.32 +56:46:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:50.86 +57:26:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:38.60 +53:54:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:00:21.26 +53:34:11.0 -- not a known variable star
00:04:07.82 +56:06:30.8 -- not a known variable star
00:04:12.88 +55:36:14.5 -- not a known variable star
00:09:01.30 +54:47:06.9 -- not a known variable star
00:09:10.89 +54:30:27.4 -- a known variable star
00:10:04.64 +50:47:20.7 -- not a known variable star
00:11:25.03 +55:00:14.4 -- not a known variable star
00:14:30.85 +56:43:30.3 -- not a known variable star
00:15:17.99 +53:07:48.6 -- a known variable star
00:15:19.64 +53:12:02.5 -- a known variable star
00:15:29.86 +57:39:49.5 -- not a known variable star
00:17:01.90 +57:24:20.9 -- not a known variable star
00:19:06.06 +56:05:25.4 -- not a known variable star
00:22:19.64 +55:04:30.4 -- not a known variable star
00:22:56.82 +50:57:51.9 -- a known variable star
00:23:19.31 +56:00:17.1 -- not a known variable star
00:26:37.19 +54:30:45.7 -- a known variable star
00:26:43.09 +57:15:38.6 -- not a known variable star
00:31:04.38 +55:22:25.2 -- a known variable star
23:10:02.61 +56:51:39.2 -- not a known variable star
23:10:11.92 +57:07:36.4 -- not a known variable star
23:10:21.38 +56:59:47.8 -- not a known variable star
23:11:07.55 +55:23:53.7 -- not a known variable star
23:11:51.47 +55:18:27.4 -- a known variable star
23:12:17.52 +57:05:09.7 -- not a known variable star
23:12:41.12 +54:49:12.3 -- not a known variable star
23:13:35.90 +55:20:55.7 -- a known variable star
23:13:38.92 +53:34:20.1 -- not a known variable star
23:13:59.11 +55:52:57.5 -- not a known variable star
23:14:10.72 +54:09:43.9 -- not a known variable star
23:14:46.56 +55:59:21.1 -- not a known variable star
23:15:33.12 +54:04:33.4 -- not a known variable star
23:15:52.60 +52:57:57.5 -- not a known variable star
23:16:43.23 +54:09:55.3 -- not a known variable star
23:16:56.83 +54:01:31.7 -- a known variable star
23:16:56.98 +52:55:46.6 -- not a known variable star
23:17:04.27 +54:39:05.6 -- a known variable star
23:17:29.54 +52:31:56.9 -- not a known variable star
23:18:34.91 +54:31:30.6 -- not a known variable star
23:18:40.97 +54:16:19.0 -- not a known variable star
23:18:44.42 +55:58:25.7 -- a known variable star
23:18:56.64 +53:20:37.4 -- a known variable star
23:19:00.25 +56:28:03.4 -- not a known variable star
23:19:14.60 +54:14:10.7 -- not a known variable star
23:19:36.59 +55:55:15.9 -- not a known variable star
23:19:37.54 +55:36:21.9 -- not a known variable star
23:19:39.71 +53:12:18.9 -- not a known variable star
23:19:45.13 +49:15:32.4 -- not a known variable star
23:19:46.37 +55:43:11.4 -- a known variable star
23:20:29.87 +55:32:14.0 -- not a known variable star
23:20:57.79 +55:40:09.9 -- a known variable star
23:21:01.34 +54:13:16.2 -- not a known variable star
23:21:05.99 +55:55:40.1 -- not a known variable star
23:21:11.96 +50:00:11.8 -- a known variable star
23:21:14.43 +55:23:13.6 -- not a known variable star
23:21:16.69 +54:35:03.8 -- not a known variable star
23:21:40.85 +51:06:26.3 -- not a known variable star
23:21:46.84 +54:35:20.7 -- not a known variable star
23:22:31.11 +52:04:54.8 -- not a known variable star
23:22:38.99 +54:02:34.6 -- a known variable star
23:23:10.42 +55:05:29.1 -- not a known variable star
23:23:13.28 +52:06:50.2 -- not a known variable star
23:23:22.79 +53:36:20.4 -- not a known variable star
23:24:53.22 +54:29:08.3 -- not a known variable star
23:25:04.95 +55:05:34.0 -- not a known variable star
23:25:28.16 +49:20:12.3 -- not a known variable star
23:25:51.16 +53:03:56.8 -- not a known variable star
23:26:01.26 +49:55:45.1 -- a known variable star
23:27:19.57 +52:32:29.0 -- not a known variable star
23:27:26.38 +49:36:02.3 -- a known variable star
23:27:32.45 +54:50:50.7 -- not a known variable star
23:27:40.51 +53:59:08.7 -- not a known variable star
23:28:21.63 +53:30:44.0 -- not a known variable star
23:28:23.31 +57:13:12.8 -- not a known variable star
23:28:27.82 +53:49:27.9 -- not a known variable star
23:28:33.67 +53:36:15.8 -- not a known variable star
23:28:46.84 +52:18:46.0 -- not a known variable star
23:29:01.37 +54:47:45.0 -- not a known variable star
23:29:15.25 +51:14:31.0 -- not a known variable star
23:29:24.02 +51:39:58.0 -- not a known variable star
23:30:32.33 +49:52:16.9 -- not a known variable star
23:30:34.29 +54:58:11.5 -- not a known variable star
23:30:56.70 +51:10:35.3 -- not a known variable star
23:31:10.13 +52:06:28.4 -- not a known variable star
23:31:48.14 +56:54:18.1 -- not a known variable star
23:33:10.43 +52:52:20.3 -- not a known variable star
23:33:17.55 +55:45:53.1 -- not a known variable star
23:34:08.21 +54:02:57.3 -- a known variable star
23:34:32.79 +49:44:27.7 -- not a known variable star
23:34:37.78 +53:35:38.7 -- not a known variable star
23:34:43.94 +55:56:14.6 -- not a known variable star
23:35:20.02 +54:55:24.7 -- not a known variable star
23:35:32.87 +56:05:53.8 -- not a known variable star
23:36:32.74 +50:40:33.3 -- not a known variable star
23:36:46.52 +53:03:07.8 -- not a known variable star
23:36:49.02 +56:55:01.8 -- not a known variable star
23:36:52.71 +53:45:16.2 -- not a known variable star
23:36:55.78 +54:03:09.9 -- not a known variable star
23:37:17.74 +55:33:07.6 -- a known variable star
23:39:31.73 +55:18:15.0 -- not a known variable star
23:41:08.61 +51:40:42.4 -- not a known variable star
23:41:50.00 +54:40:25.9 -- not a known variable star
23:42:46.07 +57:25:47.2 -- a known variable star
23:43:00.29 +52:15:00.1 -- not a known variable star
23:43:23.43 +57:27:43.1 -- a known variable star
23:44:16.80 +51:40:48.6 -- not a known variable star
23:44:33.09 +53:02:41.1 -- not a known variable star
23:44:58.72 +55:01:33.5 -- not a known variable star
23:45:47.67 +57:16:15.0 -- not a known variable star
23:46:15.15 +52:45:10.8 -- not a known variable star
23:46:34.81 +51:28:31.5 -- not a known variable star
23:46:36.44 +54:09:45.1 -- not a known variable star
23:46:38.85 +53:36:25.6 -- not a known variable star
23:47:36.03 +55:28:07.4 -- not a known variable star
23:49:09.36 +57:30:17.1 -- not a known variable star
23:49:20.24 +55:31:33.7 -- not a known variable star
23:50:37.24 +53:31:24.4 -- a known variable star
23:54:06.62 +54:45:02.9 -- not a known variable star
23:54:15.97 +53:20:53.8 -- a known variable star
23:56:18.97 +57:40:50.0 -- not a known variable star
23:56:33.15 +56:44:32.1 -- a known variable star
23:56:36.22 +56:16:48.6 -- a known variable star
23:56:52.61 +52:09:34.7 -- not a known variable star
23:57:35.32 +56:46:47.2 -- not a known variable star
23:57:50.86 +57:26:58.1 -- not a known variable star
23:58:38.60 +53:54:05.1 -- not a known variable star
Found 100 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
126 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 126 (excluding asteroids and hot pixels, 100 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)2461239.67906222 -observatory V36
07:12:43.60 +17:30:16.9 Mercury (4.0mag)
10:43:43.12 +09:08:08.3 Venus (-4.2mag)
04:47:22.47 +22:17:47.4 Mars (1.3mag)
08:23:48.34 +19:48:28.4 Jupiter (-1.8mag)
00:56:31.25 +03:22:19.3 Saturn (0.7mag)
04:08:39.95 +20:48:54.0 Uranus (5.8mag)
00:16:55.74 +00:19:37.3 Neptune (7.7mag)
20:30:10.86 -23:21:26.9 Pluto (14.4mag)
11:02:34.15 +03:42:45.1 Moon (-9.3mag)
-rw-r--r-- 1 apache apache 361 Jul 18 04:27 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461239.67906222:
08:23:46.82 +19:48:33.7 Io (6.0mag)
08:23:59.57 +19:47:45.4 Europa (6.3mag)
08:24:05.01 +19:47:23.0 Ganymede (5.6mag)
08:23:22.09 +19:50:09.9 Callisto (6.8mag)
08:21:59.35 +19:36:08.9 Himalia (15.7mag)
08:23:49.84 +19:48:23.4 Thebe (16.6mag)
08:21:20.35 +19:38:54.0 Elara (17.7mag)
08:27:33.99 +19:38:28.8 Pasiphae (17.9mag)
08:28:18.85 +19:54:44.6 Carme (19.0mag)
00:56:41.74 +03:22:25.6 Titan (8.5mag)
00:56:31.62 +03:22:28.9 Rhea (9.8mag)
00:55:56.73 +03:20:10.4 Iapetus (11.2mag)
00:56:18.00 +03:22:11.3 Hyperion (14.5mag)
00:56:21.51 +03:18:24.9 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Jul 18 04:27 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461239.67906222:
17:59:10.70 -31:06:53.1 JWST
16:02:25.98 +52:01:37.9 Chandra
19:45:12.95 +14:01:09.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 18 04:27 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461239.67906222 -observatory V36
02:47:12.13 +15:19:48.0 17.8mag P/1996 R2 (Lagerkvist)
18:12:13.15 -34:32:30.2 13.8mag P/2010 H2 (Vales)
06:33:28.83 -68:16:59.7 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:03:28.62 +32:34:59.6 17.6mag C/2017 K2 (PANSTARRS)
02:27:45.03 +21:07:59.2 15.7mag P/2021 N1 (ZTF)
22:54:34.54 +32:13:34.0 17.3mag C/2022 E2 (ATLAS)
06:21:14.01 +26:50:52.8 16.7mag C/2022 N2 (PANSTARRS)
10:02:24.14 +29:25:41.6 16.9mag C/2022 QE78 (ATLAS)
09:14:49.78 +05:07:54.7 17.9mag C/2022 R6 (PANSTARRS)
15:11:02.94 -11:34:57.5 17.8mag P/2023 B1 (PANSTARRS)
21:39:23.69 +67:29:13.2 17.9mag C/2023 H5 (Lemmon)
16:16:20.89 -10:53:15.1 14.0mag C/2023 R1 (PANSTARRS)
08:14:27.36 +66:08:38.7 17.9mag C/2024 A1 (ATLAS)
07:42:55.18 +30:23:25.0 14.8mag C/2024 E1 (Wierzchos)
15:12:50.47 +15:29:56.7 17.6mag C/2024 G6 (ATLAS)
19:31:06.99 +40:48:02.1 13.7mag C/2024 J3 (ATLAS)
21:38:59.56 +47:07:13.3 17.8mag C/2024 R4 (PANSTARRS)
04:56:56.44 -13:28:20.0 15.7mag C/2024 T5 (ATLAS)
06:40:56.30 +27:45:41.4 18.0mag C/2025 J1 (Borisov)
07:19:35.98 -13:37:33.5 16.9mag C/2025 R3 (PANSTARRS)
10:05:23.20 +22:04:56.4 17.6mag C/2025 V2 (Rankin)
12:47:29.41 +03:34:45.0 17.0mag C/2025 Y1 (ATLAS)
16:31:16.68 +79:07:52.8 17.2mag C/2026 A2 (Bok)
02:54:01.72 +45:33:42.2 16.8mag C/2026 B2 (Sun-Gao)
11:30:42.28 +05:51:05.0 17.0mag A/2026 E1
21:31:01.45 -18:04:41.7 7.1mag 10P/Tempel
11:17:15.75 -02:14:25.2 16.2mag 29P/Schwassmann-Wachmann
04:11:19.79 +30:23:18.2 17.9mag 47P/Ashbrook-Jackson
10:24:23.42 +11:30:09.0 17.1mag 63P/Wild
00:51:21.81 -05:02:47.4 15.5mag 65P/Gunn
04:46:15.77 +20:31:23.8 13.7mag 78P/Gehrels
02:34:32.22 +11:38:02.2 16.4mag 88P/Howell
06:58:32.03 +29:59:26.6 15.8mag 93P/Lovas
04:46:35.90 +31:19:46.3 16.7mag 114P/Wiseman-Skiff
08:27:48.50 +29:46:41.1 15.2mag 123P/West-Hartley
11:02:49.99 -01:58:58.5 16.9mag 124P/Mrkos
05:04:14.20 +21:00:30.5 16.2mag 128P/Shoemaker-Holt
05:50:54.82 +19:36:53.9 17.8mag 131P/Mueller
07:41:25.37 +15:16:43.5 16.5mag 141P-D/Machholz
03:20:16.33 -20:45:25.2 15.1mag 161P/Hartley-IRAS
06:01:18.59 +35:28:52.1 15.5mag 162P/SidingSpring
18:39:41.57 +20:26:29.5 14.1mag 169P/NEAT
01:59:22.25 +08:23:58.0 17.6mag 220P/McNaught
16:35:32.48 -08:44:20.8 17.2mag 235P/LINEAR
09:01:39.28 +32:33:03.1 18.0mag 240P/NEAT
20:38:00.99 -51:07:40.0 17.8mag 259P/Garradd
02:21:21.57 +15:44:58.5 15.6mag 260P/McNaught
06:01:04.65 +37:22:52.6 17.3mag 295P/LINEAR
15:06:33.24 +05:20:01.3 17.6mag 391P/Kowalski
08:41:40.12 +19:21:01.1 17.9mag 450P/LONEOS
08:03:59.28 +38:33:35.6 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Jul 18 04:27 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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-26eg 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
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
04:50:01.03 -02:22:33.80 2026-07-16.17 17.02
-rw-r--r-- 1 apache apache 5.6K Jul 18 04:27 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
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
-rw-r--r-- 1 apache apache 189K Jul 18 04:27 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:35:24.753 -14:51:35.01 AT 2026svz 2026-06-27.33 22.2271
20:31:55.032 -25:17:26.05 AT 2026svy 2026-06-27.32 22.425
23:12:03.386 -07:08:51.16 AT 2026svx 2026-06-27.43 22.3341
21:38:52.469 -09:12:08.16 AT 2026svw 2026-06-27.33 20.826
21:24:07.399 -08:10:48.32 AT 2026svv 2026-06-27.34 22.9964
20:42:22.608 -20:56:09.99 AT 2026svu 2026-06-27.32 22.8033
22:49:29.419 -09:52:21.90 AT 2026svt 2026-06-27.41 23.2399
23:08:56.975 -10:56:50.31 AT 2026svs 2026-06-27.42 23.0562
23:03:48.038 -10:42:20.17 AT 2026svr 2026-06-27.42 23.1156
21:05:20.116 -12:39:02.09 AT 2026svq 2026-06-27.30 22.4649
04:03:37.997 -49:14:19.96 AT 2026svp 2026-06-26.43 23.1019
21:42:26.450 -12:30:39.78 AT 2026svo 2026-06-26.41 23.1202
22:23:57.549 -05:26:28.43 AT 2026svn 2026-06-26.40 23.0846
21:59:30.646 -08:36:23.43 AT 2026svm 2026-06-26.41 23.0458
00:40:45.913 -42:36:08.06 AT 2026svl 2026-06-26.42 23.627
22:01:49.708 -02:28:35.92 AT 2026svk 2026-06-26.41 22.3804
22:26:37.642 -04:12:59.57 AT 2026svj 2026-06-26.40 22.8575
21:46:45.471 -13:57:34.56 AT 2026svi 2026-06-26.41 22.7499
21:42:08.217 -14:29:27.43 AT 2026svh 2026-06-26.41 23.2705
21:57:43.950 -02:48:28.98 AT 2026svg 2026-06-26.41 21.5213
-rw-r--r-- 1 apache apache 89K Jul 18 04:27 tns_transients_list.txt
