This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd
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 26.3298 2461247.8298 9.79 23:44:32.67 +56:34:54.3
113.77686 -5.09628 galactic Cas Second-epoch detections are separated by 0.6" and 9.2 pix
The object was found in VSX10" Z Cas
Type: M
# Max. Min./Amp. JD0 Period
8.200 V 15.500 V 2457305.00000 492.300000000000 M7e
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 23:44:32.67 +56:34:54.3: 11.54 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:32.67 +56:34:54.3: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 44 32.67 +56 34 54.3 9.8 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
Z Cas,2461247.8298,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Z Cas 20260726.3298 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 14.52 00:02:37.40 +55:49:29.5
116.06955 -6.39513 galactic Cas Second-epoch detections are separated by 1.6" and 9.7 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 420889035328126592 | 00:02:33.89 +55:49:55.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:02:37.40 +55:49:29.5: 15.52 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:37.40 +55:49:29.5: 15.79 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.52 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 00 02 37.40 +55 49 29.5 14.5 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 420889035328126592,2461247.8298,14.52,0.05,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 420889035328126592 20260726.3298 14.52CV 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 26.3298 2461247.8298 14.26 00:13:11.54 +50:29:26.2
116.73157 -11.92013 galactic Cas Second-epoch detections are separated by 3.9" and 10.0 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 | 00:13:11.54 +50:29:26.2 (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 00:13:11.54 +50:29:26.2: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:11.54 +50:29:26.2: 15.83 +/- 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 26.3298* 00 13 11.54 +50 29 26.2 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 14.45 23:28:47.68 +55:42:05.1
111.41357 -5.31118 galactic Cas Second-epoch detections are separated by 3.3" and 9.1 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 | 23:28:47.68 +55:42:05.1 (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 23:28:47.68 +55:42:05.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:47.68 +55:42:05.1: 15.73 +/- 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 26.3298* 23 28 47.68 +55 42 05.1 14.4 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,2461247.8298,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260726.3298 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 26.3298 2461247.8298 14.45 23:47:00.89 +55:10:15.3
113.75528 -6.54886 galactic Cas Second-epoch detections are separated by 8.5" and 9.3 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 J356.7588+55.1781 | 23:47:00.89 +55:10:15.3 (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 23:47:00.89 +55:10:15.3: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:47:00.89 +55:10:15.3: 15.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 47 00.89 +55 10 15.3 14.4 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 J356.7588+55.1781,2461247.8298,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J356.7588+55.1781 20260726.3298 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 26.3298 2461247.8298 14.08 00:02:53.27 +56:47:56.8
116.29053 -5.44529 galactic Cas Second-epoch detections are separated by 4.2" and 9.0 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 | 00:02:53.27 +56:47:56.8 (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 00:02:53.27 +56:47:56.8: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:53.27 +56:47:56.8: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 00 02 53.27 +56 47 56.8 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 14.08CV 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 26.3298 2461247.8298 14.14 23:35:05.74 +56:37:22.4
112.53339 -4.69969 galactic Cas Second-epoch detections are separated by 4.8" and 9.1 pix
The object was found in VSX12" Gaia DR3 1998519682372943616
Type: E
# Max. Min./Amp. JD0 Period
19.690 G 20.300 G 0.437711000000
ATTENTION: measured mag 14.14 is 5.6 mag brighter than the VSX record maximum brightness 19.69 - 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 23:35:05.74 +56:37:22.4: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:05.74 +56:37:22.4: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 35 05.74 +56 37 22.4 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998519682372943616,2461247.8298,14.14,0.05,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 1998519682372943616 20260726.3298 14.14CV 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 26.3298 2461247.8298 13.91 00:29:49.87 +57:44:24.4
120.04071 -5.01029 galactic Cas Second-epoch detections are separated by 3.3" and 9.9 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 J007.4672+57.7512 | 00:29:49.87 +57:44:24.4 (user input) | IRR (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 00:29:49.87 +57:44:24.4: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:29:49.87 +57:44:24.4: 15.81 +/- 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 26.3298* 00 29 49.87 +57 44 24.4 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J007.4672+57.7512,2461247.8298,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J007.4672+57.7512 20260726.3298 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.99 23:56:52.73 +55:03:44.2
115.11217 -6.97897 galactic Cas Second-epoch detections are separated by 4.3" and 9.3 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 | WISE J235655.3+550414 | 23:56:56.59 +55:03:52.8 (Gaia DR3) | EW (local) | 0.900229400000 (local) | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:52.73 +55:03:44.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:52.73 +55:03:44.2: 15.71 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.71 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 56 52.73 +55 03 44.2 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J235655.3+550414,2461247.8298,13.99,0.05,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
WISE J235655.3+550414 20260726.3298 13.99CV 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 26.3298 2461247.8298 13.97 23:44:40.09 +53:04:18.5
112.88309 -8.49226 galactic Cas Second-epoch detections are separated by 5.6" and 9.2 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 | 23:44:40.09 +53:04:18.5 (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 23:44:40.09 +53:04:18.5: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:40.09 +53:04:18.5: 15.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 44 40.09 +53 04 18.5 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 14.20 23:18:39.20 +55:18:48.8
109.92453 -5.19757 galactic Cas Second-epoch detections are separated by 3.8" and 9.1 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 J349.6470+55.3100 | 23:18:39.20 +55:18:48.8 (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 23:18:39.20 +55:18:48.8: 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 23:18:39.20 +55:18:48.8: 15.75 +/- 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 26.3298* 23 18 39.20 +55 18 48.8 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.6470+55.3100,2461247.8298,14.20,0.05,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
ATO J349.6470+55.3100 20260726.3298 14.20CV 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 26.3298 2461247.8298 13.92 23:48:20.18 +55:11:05.3
113.94278 -6.58181 galactic Cas Second-epoch detections are separated by 7.2" and 9.1 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 J357.0924+55.1883 | 23:48:20.18 +55:11:05.3 (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 23:48:20.18 +55:11:05.3: 15.52 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:48:20.18 +55:11:05.3: 15.67 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.59 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 48 20.18 +55 11 05.3 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.0924+55.1883,2461247.8298,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.0924+55.1883 20260726.3298 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.73 00:11:00.58 +52:48:13.1
116.75537 -9.58259 galactic Cas Second-epoch detections are separated by 8.6" and 9.8 pix
The object was found in VSX14" Gaia DR3 395953142400335744
Type: VAR
# Max. Min./Amp. JD0 Period
13.730 G 13.820 G 0.036568200000 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 00:11:00.58 +52:48:13.1: 14.64 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:00.58 +52:48:13.1: 15.06 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 26.3298* 00 11 00.58 +52 48 13.1 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395953142400335744,2461247.8298,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 395953142400335744 20260726.3298 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.93 23:41:09.88 +57:06:07.9
113.46696 -4.47254 galactic Cas Second-epoch detections are separated by 3.8" and 9.1 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 J355.3012+57.1115 | 23:41:13.68 +57:05:58.3 (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 23:41:09.88 +57:06:07.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:09.88 +57:06:07.9: 15.77 +/- 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 26.3298* 23 41 09.88 +57 06 07.9 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.3012+57.1115,2461247.8298,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.3012+57.1115 20260726.3298 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.88 23:45:45.38 +57:15:51.9
114.11182 -4.47826 galactic Cas Second-epoch detections are separated by 7.0" and 9.0 pix
The object was found in VSX25" Gaia DR3 1998270372407912320
Type: S
# Max. Min./Amp. JD0 Period
16.840 G 17.570 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 23:45:45.38 +57:15:51.9: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:45.38 +57:15:51.9: 15.85 +/- 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 26.3298* 23 45 45.38 +57 15 51.9 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998270372407912320,2461247.8298,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998270372407912320 20260726.3298 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.90 23:58:32.13 +54:07:42.3
115.15247 -7.94233 galactic Cas Second-epoch detections are separated by 1.6" and 9.8 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 J359.6202+54.1183 | 23:58:32.13 +54:07:42.3 (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 23:58:32.13 +54:07:42.3: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:32.13 +54:07:42.3: 15.57 +/- 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 26.3298* 23 58 32.13 +54 07 42.3 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.6202+54.1183,2461247.8298,13.90,0.05,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 J359.6202+54.1183 20260726.3298 13.90CV 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 26.3298 2461247.8298 13.88 00:15:25.71 +57:02:54.6
118.02702 -5.47992 galactic Cas Second-epoch detections are separated by 2.7" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:15:25.71 +57:02:54.6 (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 00:15:25.71 +57:02:54.6: 15.76 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:25.71 +57:02:54.6: 15.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.76 +/- 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 26.3298* 00 15 25.71 +57 02 54.6 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.94 23:50:14.74 +56:24:08.4
114.49824 -5.46412 galactic Cas Second-epoch detections are separated by 3.9" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:50:14.74 +56:24:08.4 (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 23:50:14.74 +56:24:08.4: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:14.74 +56:24:08.4: 15.74 +/- 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 26.3298* 23 50 14.74 +56 24 08.4 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.94,0.05,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
target 20260726.3298 13.94CV 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 26.3298 2461247.8298 13.86 23:41:22.47 +52:21:55.0
112.20712 -9.04144 galactic Cas Second-epoch detections are separated by 7.1" and 9.0 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 J355.3484+52.3555 | 23:41:22.47 +52:21:55.0 (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 23:41:22.47 +52:21:55.0: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:22.47 +52:21:55.0: 15.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 41 22.47 +52 21 55.0 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.3484+52.3555,2461247.8298,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.3484+52.3555 20260726.3298 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.77 23:39:35.07 +55:18:05.3
112.76137 -6.14505 galactic Cas Second-epoch detections are separated by 4.0" and 9.1 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 | 23:39:35.07 +55:18:05.3 (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 23:39:35.07 +55:18:05.3: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:35.07 +55:18:05.3: 15.76 +/- 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 26.3298* 23 39 35.07 +55 18 05.3 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260726.3298 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 26.3298 2461247.8298 13.81 23:38:03.17 +51:03:31.7
111.33761 -10.15344 galactic Cas Second-epoch detections are separated by 1.6" and 9.4 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 | 23:38:03.17 +51:03:31.7 (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 23:38:03.17 +51:03:31.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:38:03.17 +51:03:31.7: 15.85 +/- 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 26.3298* 23 38 03.17 +51 03 31.7 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.81,0.05,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 20260726.3298 13.81CV 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 26.3298 2461247.8298 13.99 23:22:35.16 +54:22:00.3
110.13003 -6.28160 galactic Cas Second-epoch detections are separated by 3.6" and 9.4 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 | 23:22:35.16 +54:22:00.3 (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 23:22:35.16 +54:22:00.3: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:35.16 +54:22:00.3: 15.79 +/- 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 26.3298* 23 22 35.16 +54 22 00.3 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.99CV 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 26.3298 2461247.8298 13.78 23:23:41.19 +53:38:23.8
110.03691 -7.02040 galactic Cas Second-epoch detections are separated by 4.9" and 9.0 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 | 23:23:41.19 +53:38:23.8 (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 23:23:41.19 +53:38:23.8: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:41.19 +53:38:23.8: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 23 41.19 +53 38 23.8 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.50 00:20:49.80 +52:35:26.1
118.22028 -10.00093 galactic Cas Second-epoch detections are separated by 4.9" and 10.2 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 | 00:20:49.80 +52:35:26.1 (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 00:20:49.80 +52:35:26.1: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:49.80 +52:35:26.1: 15.88 +/- 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 26.3298* 00 20 49.80 +52 35 26.1 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260726.3298 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 26.3298 2461247.8298 13.99 23:16:52.09 +55:47:52.0
109.86023 -4.65527 galactic Cas Second-epoch detections are separated by 2.5" and 9.1 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 | 23:16:52.09 +55:47:52.0 (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 23:16:52.09 +55:47:52.0: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:52.09 +55:47:52.0: 15.70 +/- 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 26.3298* 23 16 52.09 +55 47 52.0 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.99CV 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 26.3298 2461247.8298 13.72 00:08:31.06 +56:46:19.6
117.04801 -5.60851 galactic Cas Second-epoch detections are separated by 2.3" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:08:31.06 +56:46:19.6 (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 00:08:31.06 +56:46:19.6: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:31.06 +56:46:19.6: 15.76 +/- 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 26.3298* 00 08 31.06 +56 46 19.6 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.80 23:19:36.82 +50:24:58.0
108.32229 -9.83266 galactic And Second-epoch detections are separated by 3.2" and 10.1 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 | 23:19:36.82 +50:24:58.0 (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 23:19:36.82 +50:24:58.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:36.82 +50:24:58.0: 15.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 19 36.82 +50 24 58.0 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.67 23:52:23.28 +51:58:06.5
113.76350 -9.84898 galactic Cas Second-epoch detections are separated by 6.3" and 9.3 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 | 23:52:23.28 +51:58:06.5 (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 23:52:23.28 +51:58:06.5: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:23.28 +51:58:06.5: 15.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 52 23.28 +51 58 06.5 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.82 23:37:44.85 +55:12:16.6
112.48136 -6.16489 galactic Cas Second-epoch detections are separated by 7.4" and 9.3 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 | 23:37:44.85 +55:12:16.6 (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 23:37:44.85 +55:12:16.6: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:44.85 +55:12:16.6: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 37 44.85 +55 12 16.6 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.76 23:16:05.34 +55:19:44.4
109.58790 -5.05308 galactic Cas Second-epoch detections are separated by 4.4" and 9.0 pix
The object was found in VSX21" Gaia DR3 1996886190347011840
Type: E
# Max. Min./Amp. JD0 Period
17.430 G 18.010 G 0.419873000000 F
ATTENTION: measured mag 13.76 is 3.7 mag brighter than the VSX record maximum brightness 17.43 - 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 23:16:05.34 +55:19:44.4: 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 23:16:05.34 +55:19:44.4: 15.72 +/- 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 26.3298* 23 16 05.34 +55 19 44.4 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996886190347011840,2461247.8298,13.76,0.05,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 1996886190347011840 20260726.3298 13.76CV 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 26.3298 2461247.8298 13.74 23:16:22.00 +52:30:46.5
108.60195 -7.69355 galactic And Second-epoch detections are separated by 4.5" and 8.9 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 J349.0799+52.5089 | 23:16:22.00 +52:30:46.5 (user input) | SINE (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 23:16:22.00 +52:30:46.5: 15.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:22.00 +52:30:46.5: 15.39 +/- 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 26.3298* 23 16 22.00 +52 30 46.5 13.7 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 J349.0799+52.5089,2461247.8298,13.74,0.05,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 J349.0799+52.5089 20260726.3298 13.74CV 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 26.3298 2461247.8298 13.66 23:25:38.82 +57:34:19.1
111.60405 -3.40067 galactic Cas Second-epoch detections are separated by 7.3" and 8.5 pix
The object was found in VSX25" ZTF J232539.68+573355.5
Type: RS
# Max. Min./Amp. JD0 Period
16.195 r Y 0.058 r 2458366.84600 0.266515900000
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 23:25:38.82 +57:34:19.1: 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 23:25:38.82 +57:34:19.1: 15.55 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.55 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 25 38.82 +57 34 19.1 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J232539.68+573355.5,2461247.8298,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J232539.68+573355.5 20260726.3298 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.77 23:19:22.56 +56:55:30.8
110.58549 -3.72332 galactic Cas Second-epoch detections are separated by 1.1" and 9.5 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 J349.8385+56.9126 | 23:19:22.56 +56:55:30.8 (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 23:19:22.56 +56:55:30.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:22.56 +56:55:30.8: 15.77 +/- 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 26.3298* 23 19 22.56 +56 55 30.8 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.8385+56.9126,2461247.8298,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J349.8385+56.9126 20260726.3298 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 26.3298 2461247.8298 13.67 23:22:52.86 +52:08:27.7
109.41172 -8.39069 galactic And Second-epoch detections are separated by 0.8" and 9.6 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 1992345928876656640 | 23:22:53.96 +52:09:05.9 (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 23:22:52.86 +52:08:27.7: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:52.86 +52:08:27.7: 15.65 +/- 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 26.3298* 23 22 52.86 +52 08 27.7 13.7 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
Gaia DR3 1992345928876656640,2461247.8298,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1992345928876656640 20260726.3298 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.40 00:11:44.19 +54:49:05.1
117.18153 -7.60979 galactic Cas Second-epoch detections are separated by 6.0" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:11:44.19 +54:49:05.1 (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 00:11:44.19 +54:49:05.1: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:44.19 +54:49:05.1: 15.52 +/- 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 26.3298* 00 11 44.19 +54 49 05.1 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.40CV 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 26.3298 2461247.8298 13.62 23:24:46.67 +54:41:49.8
110.54258 -6.07655 galactic Cas Second-epoch detections are separated by 3.4" and 9.5 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 J351.1741+54.6969 | 23:24:41.62 +54:41:35.2 (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 23:24:46.67 +54:41:49.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:46.67 +54:41:49.8: 15.73 +/- 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 26.3298* 23 24 46.67 +54 41 49.8 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.1741+54.6969,2461247.8298,13.62,0.05,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 J351.1741+54.6969 20260726.3298 13.62CV 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 26.3298 2461247.8298 13.30 00:25:44.00 +54:04:10.8
119.12323 -8.61189 galactic Cas Second-epoch detections are separated by 4.2" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:25:44.00 +54:04:10.8 (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 00:25:44.00 +54:04:10.8: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:44.00 +54:04:10.8: 15.85 +/- 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 26.3298* 00 25 44.00 +54 04 10.8 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.30CV 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 26.3298 2461247.8298 13.43 23:56:38.30 +56:24:23.5
115.36510 -5.65800 galactic Cas Second-epoch detections are separated by 1.0" and 9.7 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 J359.1870+56.4173 | 23:56:42.64 +56:24:36.7 (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 23:56:38.30 +56:24:23.5: 15.68 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:38.30 +56:24:23.5: 15.54 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.60 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 56 38.30 +56 24 23.5 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.1870+56.4173,2461247.8298,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.1870+56.4173 20260726.3298 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.52 23:50:35.75 +57:09:06.4
114.72193 -4.74696 galactic Cas Second-epoch detections are separated by 2.9" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J357.6571+57.1583 | 23:50:35.75 +57:09:06.4 (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 23:50:35.75 +57:09:06.4: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:35.75 +57:09:06.4: 15.49 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.49 +/- 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 26.3298* 23 50 35.75 +57 09 06.4 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.6571+57.1583,2461247.8298,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.6571+57.1583 20260726.3298 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.51 23:26:57.46 +54:34:29.6
110.80228 -6.29511 galactic Cas Second-epoch detections are separated by 3.4" and 9.1 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 J351.7307+54.5747 | 23:26:57.46 +54:34:29.6 (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 23:26:57.46 +54:34:29.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:57.46 +54:34:29.6: 15.59 +/- 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 26.3298* 23 26 57.46 +54 34 29.6 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.7307+54.5747,2461247.8298,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.7307+54.5747 20260726.3298 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.30 00:25:08.26 +53:39:22.1
118.99216 -9.01430 galactic Cas Second-epoch detections are separated by 5.8" and 10.0 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 | 00:25:08.26 +53:39:22.1 (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 00:25:08.26 +53:39:22.1: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:08.26 +53:39:22.1: 15.73 +/- 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 26.3298* 00 25 08.26 +53 39 22.1 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.30CV 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 26.3298 2461247.8298 13.63 23:12:31.37 +56:31:47.0
109.56402 -3.75287 galactic Cas Second-epoch detections are separated by 1.9" and 8.8 pix
The object was found in VSX18" ZTF J231231.44+563205.2
Type: EA
# Max. Min./Amp. JD0 Period
17.381 r Y 0.374 r 2458471.64550 1.274344400000
ATTENTION: measured mag 13.63 is 3.4 mag brighter than the VSX record maximum brightness 17.01 - 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 23:12:31.37 +56:31:47.0: 15.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:31.37 +56:31:47.0: 15.46 +/- 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 26.3298* 23 12 31.37 +56 31 47.0 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J231231.44+563205.2,2461247.8298,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J231231.44+563205.2 20260726.3298 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.53 23:20:45.99 +53:19:15.9
109.51591 -7.17236 galactic Cas Second-epoch detections are separated by 4.7" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:20:45.99 +53:19:15.9 (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 23:20:45.99 +53:19:15.9: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:45.99 +53:19:15.9: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 20 45.99 +53 19 15.9 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.53,0.05,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
target 20260726.3298 13.53CV 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 26.3298 2461247.8298 13.28 23:56:26.14 +56:13:16.2
115.29796 -5.83317 galactic Cas Second-epoch detections are separated by 0.5" and 9.4 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 J359.1170+56.2277 | 23:56:30.45 +56:13:42.9 (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 23:56:26.14 +56:13:16.2: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:26.14 +56:13:16.2: 15.70 +/- 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 26.3298* 23 56 26.14 +56 13 16.2 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.1170+56.2277,2461247.8298,13.28,0.05,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
ATO J359.1170+56.2277 20260726.3298 13.28CV 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 26.3298 2461247.8298 13.43 23:37:15.03 +56:33:09.8
112.79817 -4.85233 galactic Cas Second-epoch detections are separated by 2.1" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:37:15.03 +56:33:09.8 (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 23:37:15.03 +56:33:09.8: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:15.03 +56:33:09.8: 15.85 +/- 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 26.3298* 23 37 15.03 +56 33 09.8 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.36 23:30:30.10 +54:53:43.2
111.39236 -6.15282 galactic Cas Second-epoch detections are separated by 3.7" and 8.9 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 | 23:30:30.10 +54:53:43.2 (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 23:30:30.10 +54:53:43.2: 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 23:30:30.10 +54:53:43.2: 15.75 +/- 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 26.3298* 23 30 30.10 +54 53 43.2 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.36CV 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 26.3298 2461247.8298 13.36 23:31:57.48 +54:10:54.8
111.37413 -6.89665 galactic Cas Second-epoch detections are separated by 3.4" and 8.9 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 J352.9793+54.1776 | 23:31:57.48 +54:10:54.8 (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 23:31:57.48 +54:10:54.8: 14.92 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:57.48 +54:10:54.8: 15.26 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.92 +/- 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 26.3298* 23 31 57.48 +54 10 54.8 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.9793+54.1776,2461247.8298,13.36,0.05,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 J352.9793+54.1776 20260726.3298 13.36CV 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 26.3298 2461247.8298 13.38 23:19:01.09 +54:18:02.6
109.61608 -6.16420 galactic Cas Second-epoch detections are separated by 2.9" and 9.1 pix
The object was found in VSX21" Gaia DR3 1995996616719747200
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.700 G 14.720 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 23:19:01.09 +54:18:02.6: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:01.09 +54:18:02.6: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 19 01.09 +54 18 02.6 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995996616719747200,2461247.8298,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995996616719747200 20260726.3298 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.19 23:56:58.11 +56:44:18.6
115.48016 -5.34311 galactic Cas Second-epoch detections are separated by 6.4" and 9.7 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 J359.2287+56.7427 | 23:56:56.47 +56:44:38.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8III 1987ApJS...64..241S NGC 7789 338
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:58.11 +56:44:18.6: 14.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:58.11 +56:44:18.6: 14.50 +/- 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 26.3298* 23 56 58.11 +56 44 18.6 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.2287+56.7427,2461247.8298,13.19,0.05,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
ATO J359.2287+56.7427 20260726.3298 13.19CV 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 26.3298 2461247.8298 13.02 23:58:37.14 +53:54:47.1
115.11990 -8.15559 galactic Cas Second-epoch detections are separated by 2.8" and 9.6 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 J359.6649+53.9052 | 23:58:37.14 +53:54:47.1 (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 23:58:37.14 +53:54:47.1: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:37.14 +53:54:47.1: 15.88 +/- 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 26.3298* 23 58 37.14 +53 54 47.1 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.6649+53.9052,2461247.8298,13.02,0.05,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 J359.6649+53.9052 20260726.3298 13.02CV 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 26.3298 2461247.8298 13.14 23:45:57.02 +56:53:10.3
114.04176 -4.85091 galactic Cas Second-epoch detections are separated by 1.3" and 9.1 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 | 23:45:57.02 +56:53:10.3 (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 23:45:57.02 +56:53:10.3: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:57.02 +56:53:10.3: 15.70 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.70 +/- 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 26.3298* 23 45 57.02 +56 53 10.3 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.08 23:39:40.85 +57:15:46.7
113.31683 -4.26311 galactic Cas Second-epoch detections are separated by 4.2" and 8.9 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 1998666196594121216 | 23:39:43.17 +57:15:49.5 (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 23:39:40.85 +57:15:46.7: 14.16 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:40.85 +57:15:46.7: 14.27 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 39 40.85 +57 15 46.7 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998666196594121216,2461247.8298,13.08,0.05,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
Gaia DR3 1998666196594121216 20260726.3298 13.08CV 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 26.3298 2461247.8298 13.14 23:28:30.79 +57:13:04.9
111.85666 -3.85979 galactic Cas Second-epoch detections are separated by 1.5" and 9.4 pix
The object was found in VSX19" Gaia DR3 1998830779740039040
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.210 G 13.250 G 0.048317000000 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 23:28:30.79 +57:13:04.9: 14.53 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:30.79 +57:13:04.9: 14.26 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 28 30.79 +57 13 04.9 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998830779740039040,2461247.8298,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998830779740039040 20260726.3298 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.11 23:13:55.36 +55:22:07.2
109.31465 -4.90379 galactic Cas Second-epoch detections are separated by 2.9" and 9.2 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 | 23:13:55.36 +55:22:07.2 (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 23:13:55.36 +55:22:07.2: 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 23:13:55.36 +55:22:07.2: 15.61 +/- 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 26.3298* 23 13 55.36 +55 22 07.2 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.11CV 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 26.3298 2461247.8298 13.06 23:19:18.68 +53:23:10.0
109.33362 -7.03578 galactic Cas Second-epoch detections are separated by 1.9" and 9.3 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 | 23:19:18.68 +53:23:10.0 (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 23:19:18.68 +53:23:10.0: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:18.68 +53:23:10.0: 15.80 +/- 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 26.3298* 23 19 18.68 +53 23 10.0 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.06,0.05,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 20260726.3298 13.06CV 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 26.3298 2461247.8298 13.08 23:10:18.23 +56:52:14.2
109.41011 -3.32233 galactic Cas Second-epoch detections are separated by 1.1" and 9.1 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 J347.5927+56.8757 | 23:10:18.23 +56:52:14.2 (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 23:10:18.23 +56:52:14.2: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:18.23 +56:52:14.2: 15.33 +/- 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 26.3298* 23 10 18.23 +56 52 14.2 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.5927+56.8757,2461247.8298,13.08,0.05,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 J347.5927+56.8757 20260726.3298 13.08CV 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 26.3298 2461247.8298 13.02 23:11:54.60 +56:27:28.4
109.45848 -3.78784 galactic Cas Second-epoch detections are separated by 0.3" and 9.0 pix
The object was found in VSX11" Gaia DR3 2008881243732655232
Type: ROT
# Max. Min./Amp. JD0 Period
16.030 G 16.070 G K
ATTENTION: measured mag 13.02 is 3.0 mag brighter than the VSX record maximum brightness 16.03 - 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 23:11:54.60 +56:27:28.4: 14.72 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:54.60 +56:27:28.4: 14.46 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 26.3298* 23 11 54.60 +56 27 28.4 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2008881243732655232,2461247.8298,13.02,0.05,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
Gaia DR3 2008881243732655232 20260726.3298 13.02CV 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 26.3298 2461247.8298 12.95 23:15:03.46 +56:00:09.2
109.69708 -4.37265 galactic Cas Second-epoch detections are separated by 3.0" and 9.1 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 | 23:15:03.46 +56:00:09.2 (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 23:15:03.46 +56:00:09.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:03.46 +56:00:09.2: 15.68 +/- 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 26.3298* 23 15 03.46 +56 00 09.2 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,12.95,0.05,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 20260726.3298 12.95CV 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 26.3298 2461247.8298 12.79 23:21:30.45 +55:24:07.9
110.33742 -5.25513 galactic Cas Second-epoch detections are separated by 4.4" and 9.1 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 J350.3670+55.4115 | 23:21:30.45 +55:24:07.9 (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 23:21:30.45 +55:24:07.9: 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 23:21:30.45 +55:24:07.9: 15.76 +/- 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 26.3298* 23 21 30.45 +55 24 07.9 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.3670+55.4115,2461247.8298,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.3670+55.4115 20260726.3298 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 12.70 23:51:58.61 +53:09:19.2
113.97916 -8.67969 galactic Cas Second-epoch detections are separated by 8.3" and 9.6 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 J358.0094+53.1476 | 23:51:58.61 +53:09:19.2 (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 23:51:58.61 +53:09:19.2: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:51:58.61 +53:09:19.2: 15.71 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.71 +/- 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 26.3298* 23 51 58.61 +53 09 19.2 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.0094+53.1476,2461247.8298,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.0094+53.1476 20260726.3298 12.70CV 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 26.3298 2461247.8298 12.92 23:14:33.63 +54:33:11.9
109.09896 -5.69567 galactic Cas Second-epoch detections are separated by 4.1" and 9.2 pix
The object was found in VSX23" Gaia DR3 1996426010371931776
Type: RS
# Max. Min./Amp. JD0 Period
17.260 G 17.350 G G
ATTENTION: measured mag 12.92 is 4.3 mag brighter than the VSX record maximum brightness 17.26 - 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 23:14:33.63 +54:33:11.9: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:33.63 +54:33:11.9: 15.47 +/- 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 26.3298* 23 14 33.63 +54 33 11.9 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996426010371931776,2461247.8298,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996426010371931776 20260726.3298 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 12.85 23:11:29.55 +56:00:28.5
109.23495 -4.18295 galactic Cas Second-epoch detections are separated by 3.8" and 9.0 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 J347.8679+56.0015 | 23:11:29.55 +56:00:28.5 (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 23:11:29.55 +56:00:28.5: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:29.55 +56:00:28.5: 15.61 +/- 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 26.3298* 23 11 29.55 +56 00 28.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.8679+56.0015,2461247.8298,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.8679+56.0015 20260726.3298 12.85CV 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 26.3298 2461247.8298 12.76 23:16:16.91 +52:28:06.7
108.57358 -7.73025 galactic And Second-epoch detections are separated by 2.1" and 9.4 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 | 23:16:16.91 +52:28:06.7 (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 23:16:16.91 +52:28:06.7: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:16.91 +52:28:06.7: 15.63 +/- 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 26.3298* 23 16 16.91 +52 28 06.7 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,12.76,0.05,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 20260726.3298 12.76CV 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 26.3298 2461247.8298 12.64 23:19:14.05 +56:28:30.4
110.40973 -4.13833 galactic Cas Second-epoch detections are separated by 3.0" and 9.1 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 | 23:19:14.05 +56:28:30.4 (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 23:19:14.05 +56:28:30.4: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:14.05 +56:28:30.4: 15.75 +/- 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 26.3298* 23 19 14.05 +56 28 30.4 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
target,2461247.8298,12.64,0.05,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
target 20260726.3298 12.64CV 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 26.3298 2461247.8298 12.65 23:22:04.37 +54:51:00.3
110.22464 -5.80172 galactic Cas Second-epoch detections are separated by 1.4" and 9.2 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 J350.5294+54.8578 | 23:22:04.37 +54:51:00.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.687+/-0.199 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:04.37 +54:51:00.3: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:04.37 +54:51:00.3: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 22 04.37 +54 51 00.3 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.5294+54.8578,2461247.8298,12.65,0.05,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 J350.5294+54.8578 20260726.3298 12.65CV 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 26.3298 2461247.8298 12.16 23:32:48.98 +53:52:50.1
111.40308 -7.22198 galactic Cas Second-epoch detections are separated by 1.2" and 9.2 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 | 23:32:48.98 +53:52:50.1 (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 23:32:48.98 +53:52:50.1: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:48.98 +53:52:50.1: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 32 48.98 +53 52 50.1 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
target,2461247.8298,12.16,0.05,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
target 20260726.3298 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 26.3298 2461247.8298 12.03 23:27:48.73 +49:42:25.7
109.33773 -10.94448 galactic And Second-epoch detections are separated by 1.1" and 9.5 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 | 23:27:48.73 +49:42:25.7 (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 23:27:48.73 +49:42:25.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:48.73 +49:42:25.7: 15.88 +/- 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 26.3298* 23 27 48.73 +49 42 25.7 12.0 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
target,2461247.8298,12.03,0.05,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
target 20260726.3298 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 26.3298 2461247.8298 11.94 23:36:47.40 +50:45:10.4
111.05455 -10.38933 galactic Cas Second-epoch detections are separated by 1.2" and 9.4 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 | 23:36:47.40 +50:45:10.4 (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 23:36:47.40 +50:45:10.4: 15.73 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:47.40 +50:45:10.4: 15.73 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.73 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 36 47.40 +50 45 10.4 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,2461247.8298,11.94,0.05,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
target 20260726.3298 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 26.3298 2461247.8298 12.12 23:21:13.25 +55:40:59.4
110.39570 -4.97725 galactic Cas Second-epoch detections are separated by 2.9" and 9.1 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 | 23:21:13.25 +55:40:59.4 (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 23:21:13.25 +55:40:59.4: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:13.25 +55:40:59.4: 15.69 +/- 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 26.3298* 23 21 13.25 +55 40 59.4 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
target,2461247.8298,12.12,0.05,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 20260726.3298 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 26.3298 2461247.8298 12.58 23:54:34.65 +57:28:04.2
115.31918 -4.56107 galactic Cas Second-epoch detections are separated by 1.3" and 9.2 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 | 23:54:34.65 +57:28:04.2 (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 23:54:34.65 +57:28:04.2: 14.41 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:34.65 +57:28:04.2: 14.26 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 54 34.65 +57 28 04.2 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,2461247.8298,12.58,0.05,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 20260726.3298 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 26.3298 2461247.8298 12.43 00:22:57.69 +55:45:15.2
118.90356 -6.89464 galactic Cas Second-epoch detections are separated by 8.2" and 9.5 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 | 00:22:57.69 +55:45:15.2 (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 00:22:57.69 +55:45:15.2: 15.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:57.69 +55:45:15.2: 15.37 +/- 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 26.3298* 00 22 57.69 +55 45 15.2 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
target,2461247.8298,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 12.72 23:20:48.61 +53:19:00.9
109.52063 -7.17853 galactic Cas Second-epoch detections are separated by 2.0" and 9.3 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 | 23:20:48.61 +53:19:00.9 (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 23:20:48.61 +53:19:00.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:48.61 +53:19:00.9: 15.75 +/- 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 26.3298* 23 20 48.61 +53 19 00.9 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 12.62 23:43:55.17 +56:19:46.5
113.62769 -5.31759 galactic Cas Second-epoch detections are separated by 2.2" and 9.3 pix
The object was found in VSX21" Gaia DR3 1997608810006234368
Type: ROT
# Max. Min./Amp. JD0 Period
12.510 G 12.540 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 23:43:55.17 +56:19:46.5: 14.59 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:55.17 +56:19:46.5: 14.63 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 43 55.17 +56 19 46.5 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
Gaia DR3 1997608810006234368,2461247.8298,12.62,0.05,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 1997608810006234368 20260726.3298 12.62CV 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 26.3298 2461247.8298 12.71 23:47:12.74 +57:25:28.7
114.34269 -4.37213 galactic Cas Second-epoch detections are separated by 0.5" and 9.2 pix
The object was found in VSX23" Gaia DR3 1998274151979352320
Type: ROT
# Max. Min./Amp. JD0 Period
12.580 G 12.630 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 23:47:12.74 +57:25:28.7: 14.36 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:47:12.74 +57:25:28.7: 14.38 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 47 12.74 +57 25 28.7 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998274151979352320,2461247.8298,12.71,0.05,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 1998274151979352320 20260726.3298 12.71CV 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 26.3298 2461247.8298 12.90 23:22:45.78 +57:23:00.7
111.17512 -3.45009 galactic Cas Second-epoch detections are separated by 3.1" and 9.0 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 | 23:22:45.78 +57:23:00.7 (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 23:22:45.78 +57:23:00.7: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:45.78 +57:23:00.7: 15.79 +/- 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 26.3298* 23 22 45.78 +57 23 00.7 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,12.90,0.05,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 20260726.3298 12.90CV 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 26.3298 2461247.8298 12.86 23:26:38.33 +53:47:40.3
110.50373 -7.01844 galactic Cas Second-epoch detections are separated by 2.1" and 9.1 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 | 23:26:38.33 +53:47:40.3 (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 23:26:38.33 +53:47:40.3: 15.59 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:38.33 +53:47:40.3: 15.68 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.59 +/- 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 26.3298* 23 26 38.33 +53 47 40.3 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.05 23:23:26.68 +54:23:40.1
110.25785 -6.29762 galactic Cas Second-epoch detections are separated by 2.0" and 9.3 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 | 23:23:26.68 +54:23:40.1 (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 23:23:26.68 +54:23:40.1: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:26.68 +54:23:40.1: 15.70 +/- 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 26.3298* 23 23 26.68 +54 23 40.1 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.05CV 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 26.3298 2461247.8298 13.02 23:22:02.31 +55:43:41.1
110.51976 -4.97432 galactic Cas Second-epoch detections are separated by 2.6" and 9.1 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 1997001535988548864 | 23:22:01.18 +55:43:06.8 (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 23:22:02.31 +55:43:41.1: 15.00 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:02.31 +55:43:41.1: 15.77 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.00 +/- 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 26.3298* 23 22 02.31 +55 43 41.1 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997001535988548864,2461247.8298,13.02,0.05,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
Gaia DR3 1997001535988548864 20260726.3298 13.02CV 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 26.3298 2461247.8298 13.08 23:32:49.01 +54:46:38.0
111.67538 -6.36708 galactic Cas Second-epoch detections are separated by 1.3" and 9.3 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 | 23:32:49.01 +54:46:38.0 (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 23:32:49.01 +54:46:38.0: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:49.01 +54:46:38.0: 15.78 +/- 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 26.3298* 23 32 49.01 +54 46 38.0 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.08CV 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 26.3298 2461247.8298 12.90 23:57:57.64 +50:30:08.3
114.30100 -11.47111 galactic Cas Second-epoch detections are separated by 5.4" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:57:57.64 +50:30:08.3 (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 23:57:57.64 +50:30:08.3: 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 23:57:57.64 +50:30:08.3: 15.72 +/- 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 26.3298* 23 57 57.64 +50 30 08.3 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,12.90,0.05,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 20260726.3298 12.90CV 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 26.3298 2461247.8298 13.03 23:57:54.05 +56:28:12.2
115.54992 -5.63242 galactic Cas Second-epoch detections are separated by 3.7" and 9.4 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 1994992071109248640 | 23:57:57.40 +56:27:41.6 (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 23:57:54.05 +56:28:12.2: 14.15 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:54.05 +56:28:12.2: 14.06 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 57 54.05 +56 28 12.2 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994992071109248640,2461247.8298,13.03,0.05,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 1994992071109248640 20260726.3298 13.03CV 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 26.3298 2461247.8298 13.26 23:25:19.53 +55:06:28.9
110.75333 -5.71453 galactic Cas Second-epoch detections are separated by 2.9" and 9.1 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 J351.3434+55.1051 | 23:25:19.53 +55:06:28.9 (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 23:25:19.53 +55:06:28.9: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:19.53 +55:06:28.9: 15.66 +/- 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 26.3298* 23 25 19.53 +55 06 28.9 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J351.3434+55.1051,2461247.8298,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.3434+55.1051 20260726.3298 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.32 23:30:23.41 +57:57:12.0
112.32611 -3.23978 galactic Cas Second-epoch detections are separated by 4.3" 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 | ATO J352.6192+57.9493 | 23:30:23.41 +57:57:12.0 (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 23:30:23.41 +57:57:12.0: 14.55 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:23.41 +57:57:12.0: 14.75 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 30 23.41 +57 57 12.0 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.6192+57.9493,2461247.8298,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.6192+57.9493 20260726.3298 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.11 23:59:03.31 +53:35:20.6
115.11667 -8.48595 galactic Cas Second-epoch detections are separated by 2.5" and 9.6 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 | 23:59:03.31 +53:35:20.6 (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 23:59:03.31 +53:35:20.6: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:59:03.31 +53:35:20.6: 15.80 +/- 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 26.3298* 23 59 03.31 +53 35 20.6 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.11CV 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 26.3298 2461247.8298 13.02 00:27:08.86 +50:01:08.3
118.93704 -12.66427 galactic Cas Second-epoch detections are separated by 3.8" and 9.5 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 J006.8007+50.0230 | 00:27:08.86 +50:01:08.3 (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 00:27:08.86 +50:01:08.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:27:08.86 +50:01:08.3: 15.62 +/- 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 26.3298* 00 27 08.86 +50 01 08.3 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J006.8007+50.0230,2461247.8298,13.02,0.05,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 J006.8007+50.0230 20260726.3298 13.02CV 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 26.3298 2461247.8298 13.42 23:10:52.33 +57:01:38.7
109.54155 -3.20669 galactic Cas Second-epoch detections are separated by 0.4" and 8.9 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 | 23:10:52.33 +57:01:38.7 (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 23:10:52.33 +57:01:38.7: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:52.33 +57:01:38.7: 15.62 +/- 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 26.3298* 23 10 52.33 +57 01 38.7 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.13 00:13:35.65 +56:24:23.9
117.68418 -6.07903 galactic Cas Second-epoch detections are separated by 5.2" and 9.5 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 | 00:13:35.65 +56:24:23.9 (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 00:13:35.65 +56:24:23.9: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:35.65 +56:24:23.9: 15.50 +/- 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 26.3298* 00 13 35.65 +56 24 23.9 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.13,0.05,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 20260726.3298 13.13CV 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 26.3298 2461247.8298 13.44 23:18:19.32 +53:13:24.1
109.13641 -7.13596 galactic Cas Second-epoch detections are separated by 3.2" and 9.1 pix
The object was found in VSX21" Gaia DR3 1995684080537352704
Type: ROT
# Max. Min./Amp. JD0 Period
14.580 G 14.620 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 23:18:19.32 +53:13:24.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:19.32 +53:13:24.1: 15.74 +/- 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 26.3298* 23 18 19.32 +53 13 24.1 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995684080537352704,2461247.8298,13.44,0.05,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
Gaia DR3 1995684080537352704 20260726.3298 13.44CV 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 26.3298 2461247.8298 13.14 00:12:55.37 +50:00:03.0
116.61198 -12.39770 galactic Cas Second-epoch detections are separated by 4.5" and 9.8 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 J003.2462+49.9966 | 00:12:55.37 +50:00:03.0 (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 00:12:55.37 +50:00:03.0: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:55.37 +50:00:03.0: 15.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 00 12 55.37 +50 00 03.0 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.2462+49.9966,2461247.8298,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J003.2462+49.9966 20260726.3298 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.16 23:58:50.05 +54:41:49.5
115.31294 -7.39463 galactic Cas Second-epoch detections are separated by 1.5" and 9.5 pix
The object was found in VSX23" Gaia DR3 1993663006370972800
Type:
# Max. Min./Amp. JD0 Period
13.300 G 13.340 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 23:58:50.05 +54:41:49.5: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:50.05 +54:41:49.5: 15.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 58 50.05 +54 41 49.5 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993663006370972800,2461247.8298,13.16,0.05,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 1993663006370972800 20260726.3298 13.16CV 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 26.3298 2461247.8298 13.20 00:07:09.81 +57:23:10.8
116.97014 -4.97203 galactic Cas Second-epoch detections are separated by 1.3" and 9.2 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 J001.7977+57.3855 | 00:07:09.81 +57:23:10.8 (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 00:07:09.81 +57:23:10.8: 14.92 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:09.81 +57:23:10.8: 15.28 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.06 +/- 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 26.3298* 00 07 09.81 +57 23 10.8 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.7977+57.3855,2461247.8298,13.20,0.05,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
ATO J001.7977+57.3855 20260726.3298 13.20CV 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 26.3298 2461247.8298 13.19 23:57:56.35 +50:30:59.5
114.30064 -11.45648 galactic Cas Second-epoch detections are separated by 4.8" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:57:56.35 +50:30:59.5 (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 23:57:56.35 +50:30:59.5: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:56.35 +50:30:59.5: 15.73 +/- 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 26.3298* 23 57 56.35 +50 30 59.5 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.19CV 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 26.3298 2461247.8298 13.08 00:20:02.82 +50:08:55.9
117.79203 -12.40935 galactic Cas Second-epoch detections are separated by 4.7" and 9.9 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 J005.0247+50.1555 | 00:20:02.82 +50:08:55.9 (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 00:20:02.82 +50:08:55.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:02.82 +50:08:55.9: 15.75 +/- 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 26.3298* 00 20 02.82 +50 08 55.9 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J005.0247+50.1555,2461247.8298,13.08,0.05,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 J005.0247+50.1555 20260726.3298 13.08CV 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 26.3298 2461247.8298 13.41 23:40:52.98 +57:50:35.7
113.63090 -3.74875 galactic Cas Second-epoch detections are separated by 3.7" and 9.2 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 | 23:40:52.98 +57:50:35.7 (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 23:40:52.98 +57:50:35.7: 15.19 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:40:52.98 +57:50:35.7: 15.02 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.09 +/- 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 26.3298* 23 40 52.98 +57 50 35.7 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.41,0.05,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 20260726.3298 13.41CV 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 26.3298 2461247.8298 13.34 23:56:31.15 +53:44:48.2
114.77862 -8.25338 galactic Cas Second-epoch detections are separated by 6.3" and 9.4 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 J359.1339+53.7382 | 23:56:31.15 +53:44:48.2 (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 23:56:31.15 +53:44:48.2: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:31.15 +53:44:48.2: 15.69 +/- 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 26.3298* 23 56 31.15 +53 44 48.2 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.1339+53.7382,2461247.8298,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.1339+53.7382 20260726.3298 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.33 23:49:45.14 +56:38:12.3
114.48759 -5.22026 galactic Cas Second-epoch detections are separated by 2.3" and 9.5 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 | 23:49:45.14 +56:38:12.3 (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 23:49:45.14 +56:38:12.3: 15.35 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:45.14 +56:38:12.3: 15.47 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.41 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 49 45.14 +56 38 12.3 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.09 00:24:49.00 +53:02:22.8
118.87897 -9.62246 galactic Cas Second-epoch detections are separated by 3.2" and 9.8 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 J006.1924+53.0294 | 00:24:49.00 +53:02:22.8 (user input) | CBH (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 00:24:49.00 +53:02:22.8: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:49.00 +53:02:22.8: 15.52 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.52 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 26.3298* 00 24 49.00 +53 02 22.8 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J006.1924+53.0294,2461247.8298,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.1924+53.0294 20260726.3298 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.28 00:12:13.11 +50:41:18.4
116.60643 -11.70099 galactic Cas Second-epoch detections are separated by 3.7" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:12:13.11 +50:41:18.4 (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 00:12:13.11 +50:41:18.4: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:13.11 +50:41:18.4: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 00 12 13.11 +50 41 18.4 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.28,0.05,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 20260726.3298 13.28CV 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 26.3298 2461247.8298 13.47 23:24:03.95 +54:35:38.9
110.41049 -6.13958 galactic Cas Second-epoch detections are separated by 3.4" and 9.3 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 | 23:24:03.95 +54:35:38.9 (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 23:24:03.95 +54:35:38.9: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:03.95 +54:35:38.9: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 24 03.95 +54 35 38.9 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.40 23:52:05.29 +50:10:17.3
113.29365 -11.58632 galactic Cas Second-epoch detections are separated by 2.9" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:52:05.29 +50:10:17.3 (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 23:52:05.29 +50:10:17.3: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:05.29 +50:10:17.3: 15.92 +/- 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 26.3298* 23 52 05.29 +50 10 17.3 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.40CV 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 26.3298 2461247.8298 13.61 23:29:40.53 +51:43:30.4
110.27559 -9.12614 galactic Cas Second-epoch detections are separated by 3.8" and 8.5 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 1991424984808964608 | 23:29:43.85 +51:43:31.9 (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 23:29:40.53 +51:43:30.4: 14.96 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:40.53 +51:43:30.4: 14.64 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 29 40.53 +51 43 30.4 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991424984808964608,2461247.8298,13.61,0.05,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 1991424984808964608 20260726.3298 13.61CV 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 26.3298 2461247.8298 13.54 23:18:33.45 +49:57:07.7
107.99476 -10.20659 galactic And Second-epoch detections are separated by 5.9" and 9.4 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 | 23:18:33.45 +49:57:07.7 (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 23:18:33.45 +49:57:07.7: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:33.45 +49:57:07.7: 15.73 +/- 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 26.3298* 23 18 33.45 +49 57 07.7 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.54,0.05,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
target 20260726.3298 13.54CV 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 26.3298 2461247.8298 13.40 23:43:23.69 +51:59:26.5
112.40792 -9.48525 galactic Cas Second-epoch detections are separated by 0.9" and 9.4 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 J355.8468+51.9807 | 23:43:23.69 +51:59:26.5 (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 23:43:23.69 +51:59:26.5: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:23.69 +51:59:26.5: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 43 23.69 +51 59 26.5 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.8468+51.9807,2461247.8298,13.40,0.05,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
ATO J355.8468+51.9807 20260726.3298 13.40CV 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 26.3298 2461247.8298 13.47 23:57:51.72 +56:29:02.3
115.54754 -5.61770 galactic Cas Second-epoch detections are separated by 4.5" and 9.5 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 | 23:57:51.72 +56:29:02.3 (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 23:57:51.72 +56:29:02.3: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:51.72 +56:29:02.3: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 57 51.72 +56 29 02.3 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.64 23:12:11.66 +55:19:43.6
109.07087 -4.84949 galactic Cas Second-epoch detections are separated by 4.3" and 9.8 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 | 23:12:11.66 +55:19:43.6 (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 23:12:11.66 +55:19:43.6: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:11.66 +55:19:43.6: 15.62 +/- 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 26.3298* 23 12 11.66 +55 19 43.6 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.64,0.05,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
target 20260726.3298 13.64CV 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 26.3298 2461247.8298 13.47 23:31:54.22 +55:26:00.4
111.74997 -5.70212 galactic Cas Second-epoch detections are separated by 2.1" and 9.4 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 | 23:31:54.22 +55:26:00.4 (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 23:31:54.22 +55:26:00.4: 14.68 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:54.22 +55:26:00.4: 14.64 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 26.3298* 23 31 54.22 +55 26 00.4 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.40 00:07:56.66 +53:41:08.0
116.44381 -8.63739 galactic Cas Second-epoch detections are separated by 4.1" and 9.6 pix
The object was found in VSX17" Gaia DR3 420056189628253696
Type: ROT
# Max. Min./Amp. JD0 Period
16.210 G 16.250 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 00:07:56.66 +53:41:08.0: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:56.66 +53:41:08.0: 15.76 +/- 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 26.3298* 00 07 56.66 +53 41 08.0 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420056189628253696,2461247.8298,13.40,0.05,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 420056189628253696 20260726.3298 13.40CV 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 26.3298 2461247.8298 13.66 23:21:31.14 +55:55:32.2
110.51844 -4.76376 galactic Cas Second-epoch detections are separated by 2.0" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.3845+55.9274 | 23:21:31.14 +55:55:32.2 (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 23:21:31.14 +55:55:32.2: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:31.14 +55:55:32.2: 15.03 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 21 31.14 +55 55 32.2 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.3845+55.9274,2461247.8298,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.3845+55.9274 20260726.3298 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.45 00:13:58.31 +55:15:52.0
117.56845 -7.21666 galactic Cas Second-epoch detections are separated by 6.3" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:13:58.31 +55:15:52.0 (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 00:13:58.31 +55:15:52.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:58.31 +55:15:52.0: 15.74 +/- 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 26.3298* 00 13 58.31 +55 15 52.0 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260726.3298 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 26.3298 2461247.8298 13.45 00:12:33.36 +57:13:41.7
117.66606 -5.24543 galactic Cas Second-epoch detections are separated by 2.6" and 9.7 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 J003.1286+57.2339 | 00:12:33.36 +57:13:41.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.935+/- (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:33.36 +57:13:41.7: 15.34 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:33.36 +57:13:41.7: 15.43 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.38 +/- 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 26.3298* 00 12 33.36 +57 13 41.7 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.1286+57.2339,2461247.8298,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J003.1286+57.2339 20260726.3298 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 26.3298 2461247.8298 13.61 23:12:32.05 +57:05:41.1
109.77659 -3.22920 galactic Cas Second-epoch detections are separated by 1.9" and 9.0 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 J348.1136+57.0997 | 23:12:32.05 +57:05:41.1 (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 23:12:32.05 +57:05:41.1: 15.00 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:32.05 +57:05:41.1: 14.97 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.98 +/- 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 26.3298* 23 12 32.05 +57 05 41.1 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.1136+57.0997,2461247.8298,13.61,0.05,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
ATO J348.1136+57.0997 20260726.3298 13.61CV 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 26.3298 2461247.8298 13.52 23:38:06.06 +50:59:35.0
111.32597 -10.21863 galactic Cas Second-epoch detections are separated by 0.8" and 9.5 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 | 23:38:06.06 +50:59:35.0 (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 23:38:06.06 +50:59:35.0: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:38:06.06 +50:59:35.0: 15.92 +/- 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 26.3298* 23 38 06.06 +50 59 35.0 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.60 23:32:47.26 +54:06:00.7
111.46581 -7.01134 galactic Cas Second-epoch detections are separated by 2.6" and 9.2 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 J353.2106+54.1062 | 23:32:47.26 +54:06:00.7 (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 23:32:47.26 +54:06:00.7: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:47.26 +54:06:00.7: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 32 47.26 +54 06 00.7 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.2106+54.1062,2461247.8298,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.2106+54.1062 20260726.3298 13.60CV 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 26.3298 2461247.8298 13.56 23:46:59.80 +57:24:39.0
114.31105 -4.37833 galactic Cas Second-epoch detections are separated by 1.0" and 9.2 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 | 23:46:59.80 +57:24:39.0 (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 23:46:59.80 +57:24:39.0: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:59.80 +57:24:39.0: 15.61 +/- 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 26.3298* 23 46 59.80 +57 24 39.0 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.56 23:45:14.10 +49:49:19.5
112.11610 -11.65428 galactic Cas Second-epoch detections are separated by 3.0" and 9.5 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 | 23:45:14.10 +49:49:19.5 (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 23:45:14.10 +49:49:19.5: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:14.10 +49:49:19.5: 15.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 45 14.10 +49 49 19.5 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.65 23:34:22.58 +51:39:22.8
110.95693 -9.41471 galactic Cas Second-epoch detections are separated by 5.0" and 9.3 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 | 23:34:22.58 +51:39:22.8 (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 23:34:22.58 +51:39:22.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:22.58 +51:39:22.8: 15.74 +/- 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 26.3298* 23 34 22.58 +51 39 22.8 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.65 23:30:03.04 +54:39:53.7
111.25821 -6.35166 galactic Cas Second-epoch detections are separated by 3.3" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:30:03.04 +54:39:53.7 (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 23:30:03.04 +54:39:53.7: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:03.04 +54:39:53.7: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 30 03.04 +54 39 53.7 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.68 23:32:41.94 +58:04:45.8
112.65623 -3.21281 galactic Cas Second-epoch detections are separated by 2.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:32:41.94 +58:04:45.8 (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 23:32:41.94 +58:04:45.8: 15.25 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:41.94 +58:04:45.8: 15.49 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.36 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 32 41.94 +58 04 45.8 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.61 00:20:13.49 +57:49:39.8
118.77159 -4.79167 galactic Cas Second-epoch detections are separated by 6.7" and 10.1 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 | 00:20:13.49 +57:49:39.8 (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 00:20:13.49 +57:49:39.8: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:13.49 +57:49:39.8: 15.59 +/- 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 26.3298* 00 20 13.49 +57 49 39.8 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.61,0.05,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 20260726.3298 13.61CV 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 26.3298 2461247.8298 13.80 23:15:13.26 +52:54:41.3
108.58519 -7.25918 galactic And Second-epoch detections are separated by 2.4" and 9.4 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 | 23:15:13.26 +52:54:41.3 (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 23:15:13.26 +52:54:41.3: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:13.26 +52:54:41.3: 15.73 +/- 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 26.3298* 23 15 13.26 +52 54 41.3 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.50 23:58:56.41 +53:17:11.7
115.03725 -8.77856 galactic Cas Second-epoch detections are separated by 2.2" and 9.6 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 | 23:58:56.41 +53:17:11.7 (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 23:58:56.41 +53:17:11.7: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:56.41 +53:17:11.7: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 58 56.41 +53 17 11.7 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260726.3298 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 26.3298 2461247.8298 13.69 23:34:19.66 +54:04:14.6
111.67409 -7.10697 galactic Cas Second-epoch detections are separated by 1.3" and 9.3 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 | 23:34:19.66 +54:04:14.6 (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 23:34:19.66 +54:04:14.6: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:19.66 +54:04:14.6: 15.57 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.57 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 26.3298* 23 34 19.66 +54 04 14.6 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.59 23:49:55.13 +52:10:38.2
113.43906 -9.55694 galactic Cas Second-epoch detections are separated by 3.7" and 9.4 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 | 23:49:55.13 +52:10:38.2 (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 23:49:55.13 +52:10:38.2: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:55.13 +52:10:38.2: 15.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 49 55.13 +52 10 38.2 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.73 23:29:37.56 +50:43:08.5
109.94637 -10.07845 galactic Cas Second-epoch detections are separated by 1.1" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:29:37.56 +50:43:08.5 (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 23:29:37.56 +50:43:08.5: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:37.56 +50:43:08.5: 15.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 29 37.56 +50 43 08.5 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.81 23:36:04.26 +51:21:42.2
111.12444 -9.77394 galactic Cas Second-epoch detections are separated by 4.2" and 8.5 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 J354.0234+51.3737 | 23:36:04.26 +51:21:42.2 (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 23:36:04.26 +51:21:42.2: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:04.26 +51:21:42.2: 15.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 36 04.26 +51 21 42.2 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.0234+51.3737,2461247.8298,13.81,0.05,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 J354.0234+51.3737 20260726.3298 13.81CV 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 26.3298 2461247.8298 13.88 23:23:44.71 +53:48:00.6
110.09920 -6.87234 galactic Cas Second-epoch detections are separated by 6.7" and 10.0 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 | 23:23:44.71 +53:48:00.6 (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 23:23:44.71 +53:48:00.6: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:44.71 +53:48:00.6: 15.85 +/- 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 26.3298* 23 23 44.71 +53 48 00.6 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.53 00:03:25.85 +55:39:18.2
116.14980 -6.58325 galactic Cas Second-epoch detections are separated by 0.9" and 9.4 pix
The object was found in VSX12" ZTF J000324.91+553909.1
Type: EW
# Max. Min./Amp. JD0 Period
17.392 r Y 0.286 r 2458301.95090 0.387408800000
ATTENTION: measured mag 13.53 is 3.6 mag brighter than the VSX record maximum brightness 17.11 - 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 00:03:25.85 +55:39:18.2: 14.53 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:25.85 +55:39:18.2: 14.55 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 00 03 25.85 +55 39 18.2 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J000324.91+553909.1,2461247.8298,13.53,0.05,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
ZTF J000324.91+553909.1 20260726.3298 13.53CV 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 26.3298 2461247.8298 13.85 23:23:26.73 +57:10:13.4
111.19059 -3.68181 galactic Cas Second-epoch detections are separated by 2.9" and 9.4 pix
The object was found in VSX24" Gaia DR3 2009326408499095680
Type: L
# Max. Min./Amp. JD0 Period
13.360 G 13.490 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 23:23:26.73 +57:10:13.4: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:26.73 +57:10:13.4: 15.58 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.58 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 26.3298* 23 23 26.73 +57 10 13.4 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009326408499095680,2461247.8298,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009326408499095680 20260726.3298 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.54 00:19:39.43 +50:48:15.0
117.81289 -11.75143 galactic Cas Second-epoch detections are separated by 5.4" and 10.0 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 | 00:19:39.43 +50:48:15.0 (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 00:19:39.43 +50:48:15.0: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:39.43 +50:48:15.0: 15.88 +/- 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 26.3298* 00 19 39.43 +50 48 15.0 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.54,0.05,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
target 20260726.3298 13.54CV 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 26.3298 2461247.8298 13.62 00:00:20.87 +56:49:48.3
115.95397 -5.34788 galactic Cas Second-epoch detections are separated by 1.5" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:00:20.87 +56:49:48.3 (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 00:00:20.87 +56:49:48.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:20.87 +56:49:48.3: 15.74 +/- 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 26.3298* 00 00 20.87 +56 49 48.3 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.62,0.05,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 20260726.3298 13.62CV 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 26.3298 2461247.8298 13.67 00:08:13.12 +54:03:49.3
116.54879 -8.27155 galactic Cas Second-epoch detections are separated by 6.7" and 9.6 pix
The object was found in VSX19" Gaia DR3 420091202202338048
Type: VAR
# Max. Min./Amp. JD0 Period
15.810 G 15.860 G 0.018077600000 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 00:08:13.12 +54:03:49.3: 15.23 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:13.12 +54:03:49.3: 15.09 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.14 +/- 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 26.3298* 00 08 13.12 +54 03 49.3 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 420091202202338048,2461247.8298,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 420091202202338048 20260726.3298 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.79 23:44:18.13 +57:20:24.7
113.94074 -4.35490 galactic Cas Second-epoch detections are separated by 4.0" and 9.3 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 J356.0545+57.3462 | 23:44:18.13 +57:20:24.7 (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 23:44:18.13 +57:20:24.7: 15.00 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:18.13 +57:20:24.7: 15.02 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.01 +/- 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 26.3298* 23 44 18.13 +57 20 24.7 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.0545+57.3462,2461247.8298,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.0545+57.3462 20260726.3298 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.66 00:02:25.22 +54:32:44.9
115.79610 -7.64539 galactic Cas Second-epoch detections are separated by 5.6" and 9.3 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 | 00:02:25.22 +54:32:44.9 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:02:25.22 +54:32:44.9: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:25.22 +54:32:44.9: 15.85 +/- 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 26.3298* 00 02 25.22 +54 32 44.9 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.72 23:56:15.70 +56:09:37.5
115.26118 -5.88737 galactic Cas Second-epoch detections are separated by 2.3" and 9.2 pix
The object was found in VSX 4" Gaia DR3 1994796976516507264
Type: S
# Max. Min./Amp. JD0 Period
17.260 G 18.700 G
ATTENTION: measured mag 13.72 is 3.5 mag brighter than the VSX record maximum brightness 17.26 - 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 23:56:15.70 +56:09:37.5: 15.57 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:15.70 +56:09:37.5: 15.60 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.59 +/- 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 26.3298* 23 56 15.70 +56 09 37.5 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1994796976516507264,2461247.8298,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994796976516507264 20260726.3298 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.79 23:20:45.16 +55:33:00.2
110.28748 -5.07955 galactic Cas Second-epoch detections are separated by 4.6" and 9.1 pix
The object was found in VSX15" Gaia DR3 1996905053844228352
Type: ROT
# Max. Min./Amp. JD0 Period
15.200 G 15.240 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 23:20:45.16 +55:33:00.2: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:45.16 +55:33:00.2: 15.66 +/- 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 26.3298* 23 20 45.16 +55 33 00.2 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996905053844228352,2461247.8298,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996905053844228352 20260726.3298 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.93 23:21:19.87 +55:56:11.3
110.49736 -4.74456 galactic Cas Second-epoch detections are separated by 2.2" and 9.2 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 | 23:21:19.87 +55:56:11.3 (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 23:21:19.87 +55:56:11.3: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:19.87 +55:56:11.3: 15.70 +/- 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 26.3298* 23 21 19.87 +55 56 11.3 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.74 23:47:39.62 +56:51:37.1
114.26242 -4.93406 galactic Cas Second-epoch detections are separated by 1.9" and 9.3 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 J356.9155+56.8753 | 23:47:38.48 +56:52:13.3 (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 23:47:39.62 +56:51:37.1: 15.28 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:47:39.62 +56:51:37.1: 15.34 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 26.3298* 23 47 39.62 +56 51 37.1 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.9155+56.8753,2461247.8298,13.74,0.05,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 J356.9155+56.8753 20260726.3298 13.74CV 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 26.3298 2461247.8298 13.81 23:26:29.66 +55:06:24.3
110.91173 -5.77025 galactic Cas Second-epoch detections are separated by 3.3" and 9.2 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 | 23:26:29.66 +55:06:24.3 (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 23:26:29.66 +55:06:24.3: 15.45 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:29.66 +55:06:24.3: 15.81 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.60 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 26 29.66 +55 06 24.3 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.81,0.05,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 20260726.3298 13.81CV 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 26.3298 2461247.8298 13.71 23:58:56.00 +56:57:59.6
115.79140 -5.17550 galactic Cas Second-epoch detections are separated by 4.3" and 9.4 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 | 23:58:56.00 +56:57:59.6 (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 23:58:56.00 +56:57:59.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:56.00 +56:57:59.6: 15.65 +/- 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 26.3298* 23 58 56.00 +56 57 59.6 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.59 00:12:01.35 +53:36:40.1
117.03493 -8.80871 galactic Cas Second-epoch detections are separated by 5.1" and 9.7 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 J003.0116+53.6176 | 00:12:01.35 +53:36:40.1 (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 00:12:01.35 +53:36:40.1: 15.10 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:01.35 +53:36:40.1: 15.39 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.21 +/- 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 26.3298* 00 12 01.35 +53 36 40.1 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.0116+53.6176,2461247.8298,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J003.0116+53.6176 20260726.3298 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.80 23:50:58.54 +54:43:02.9
114.20103 -7.12609 galactic Cas Second-epoch detections are separated by 1.1" and 9.6 pix
The object was found in VSX22" Gaia DR3 1993806526997829120
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.980 G 14.010 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 23:50:58.54 +54:43:02.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:58.54 +54:43:02.9: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 50 58.54 +54 43 02.9 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993806526997829120,2461247.8298,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993806526997829120 20260726.3298 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.75 00:06:11.22 +51:25:18.4
115.77780 -10.82031 galactic Cas Second-epoch detections are separated by 2.8" and 9.5 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 | 00:06:11.22 +51:25:18.4 (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 00:06:11.22 +51:25:18.4: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:11.22 +51:25:18.4: 15.92 +/- 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 26.3298* 00 06 11.22 +51 25 18.4 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260726.3298 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 26.3298 2461247.8298 14.04 23:28:42.42 +53:51:09.6
110.81379 -7.06119 galactic Cas Second-epoch detections are separated by 1.7" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:28:42.42 +53:51:09.6 (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 23:28:42.42 +53:51:09.6: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:42.42 +53:51:09.6: 15.78 +/- 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 26.3298* 23 28 42.42 +53 51 09.6 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 14.04CV 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 26.3298 2461247.8298 13.66 00:25:00.05 +52:51:11.0
118.88722 -9.81095 galactic Cas Second-epoch detections are separated by 1.9" and 9.5 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 J006.2681+52.8492 | 00:25:00.05 +52:51:11.0 (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 00:25:00.05 +52:51:11.0: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:00.05 +52:51:11.0: 15.72 +/- 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 26.3298* 00 25 00.05 +52 51 11.0 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J006.2681+52.8492,2461247.8298,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.2681+52.8492 20260726.3298 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.89 00:00:52.63 +53:17:23.0
115.32485 -8.83361 galactic Cas Second-epoch detections are separated by 4.0" and 9.1 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 | 00:00:52.63 +53:17:23.0 (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 00:00:52.63 +53:17:23.0: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:52.63 +53:17:23.0: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 00 00 52.63 +53 17 23.0 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.89,0.05,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
target 20260726.3298 13.89CV 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 26.3298 2461247.8298 13.85 00:12:49.78 +55:50:22.8
117.49337 -6.62386 galactic Cas Second-epoch detections are separated by 8.8" and 9.6 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 | 00:12:49.78 +55:50:22.8 (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 00:12:49.78 +55:50:22.8: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:49.78 +55:50:22.8: 15.67 +/- 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 26.3298* 00 12 49.78 +55 50 22.8 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.86 23:42:23.25 +51:48:08.2
112.20520 -9.62555 galactic Cas Second-epoch detections are separated by 1.2" and 9.4 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 1944868634531549056 | 23:42:26.00 +51:48:29.8 (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 23:42:23.25 +51:48:08.2: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:23.25 +51:48:08.2: 15.83 +/- 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 26.3298* 23 42 23.25 +51 48 08.2 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944868634531549056,2461247.8298,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944868634531549056 20260726.3298 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.94 23:25:08.93 +54:30:24.1
110.53041 -6.27409 galactic Cas Second-epoch detections are separated by 5.2" and 8.9 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 | 23:25:08.93 +54:30:24.1 (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 23:25:08.93 +54:30:24.1: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:08.93 +54:30:24.1: 15.63 +/- 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 26.3298* 23 25 08.93 +54 30 24.1 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.94,0.05,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
target 20260726.3298 13.94CV 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 26.3298 2461247.8298 13.81 00:09:58.09 +50:49:56.8
116.27116 -11.50220 galactic Cas Second-epoch detections are separated by 7.9" and 10.5 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 | 00:09:58.09 +50:49:56.8 (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 00:09:58.09 +50:49:56.8: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:58.09 +50:49:56.8: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 00 09 58.09 +50 49 56.8 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.81,0.05,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 20260726.3298 13.81CV 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 26.3298 2461247.8298 14.09 23:55:51.58 +54:53:32.4
114.93169 -7.11379 galactic Cas Second-epoch detections are separated by 2.9" and 9.5 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 | 23:55:51.58 +54:53:32.4 (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 23:55:51.58 +54:53:32.4: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:51.58 +54:53:32.4: 15.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 55 51.58 +54 53 32.4 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.99 23:43:20.49 +55:42:18.9
113.38577 -5.89927 galactic Cas Second-epoch detections are separated by 1.7" and 9.3 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 | ZTF J234321.98+554245.0 | 23:43:21.97 +55:42:45.0 (Gaia DR3) | SR (local) | 66.604006500000 (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:20.49 +55:42:18.9: 15.19 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:20.49 +55:42:18.9: 15.11 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.14 +/- 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 26.3298* 23 43 20.49 +55 42 18.9 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J234321.98+554245.0,2461247.8298,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J234321.98+554245.0 20260726.3298 13.99CV 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 26.3298 2461247.8298 14.01 00:07:38.40 +57:11:00.6
116.99909 -5.18287 galactic Cas Second-epoch detections are separated by 3.5" and 9.6 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 J001.9292+57.1854 | 00:07:38.40 +57:11:00.6 (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 00:07:38.40 +57:11:00.6: 15.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:38.40 +57:11:00.6: 15.11 +/- 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 26.3298* 00 07 38.40 +57 11 00.6 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.9292+57.1854,2461247.8298,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J001.9292+57.1854 20260726.3298 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 14.13 23:26:45.28 +53:47:42.1
110.52019 -7.02351 galactic Cas Second-epoch detections are separated by 1.4" and 9.5 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 | 23:26:45.28 +53:47:42.1 (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 23:26:45.28 +53:47:42.1: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:45.28 +53:47:42.1: 15.81 +/- 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 26.3298* 23 26 45.28 +53 47 42.1 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,14.13,0.05,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 20260726.3298 14.13CV 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 26.3298 2461247.8298 14.11 23:43:03.76 +52:46:21.9
112.56776 -8.71761 galactic Cas Second-epoch detections are separated by 2.7" and 9.0 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 J355.7806+52.7790 | 23:43:03.76 +52:46:21.9 (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 23:43:03.76 +52:46:21.9: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:03.76 +52:46:21.9: 15.85 +/- 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 26.3298* 23 43 03.76 +52 46 21.9 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.7806+52.7790,2461247.8298,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.7806+52.7790 20260726.3298 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 14.07 00:14:46.44 +53:48:10.2
117.47115 -8.67972 galactic Cas Second-epoch detections are separated by 8.5" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:14:46.44 +53:48:10.2 (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 00:14:46.44 +53:48:10.2: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:46.44 +53:48:10.2: 15.66 +/- 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 26.3298* 00 14 46.44 +53 48 10.2 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.98 00:09:11.07 +57:36:12.5
117.27532 -4.80347 galactic Cas Second-epoch detections are separated by 1.0" and 9.6 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 J002.2895+57.6029 | 00:09:11.07 +57:36:12.5 (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 00:09:11.07 +57:36:12.5: 15.45 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:11.07 +57:36:12.5: 15.77 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.45 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 00 09 11.07 +57 36 12.5 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.2895+57.6029,2461247.8298,13.98,0.05,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 J002.2895+57.6029 20260726.3298 13.98CV 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 26.3298 2461247.8298 14.34 23:15:23.66 +53:33:30.5
108.84752 -6.66632 galactic Cas Second-epoch detections are separated by 3.0" and 9.1 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 | 23:15:23.66 +53:33:30.5 (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 23:15:23.66 +53:33:30.5: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:23.66 +53:33:30.5: 15.74 +/- 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 26.3298* 23 15 23.66 +53 33 30.5 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 13.96 00:13:29.83 +56:53:48.5
117.74348 -5.59224 galactic Cas Second-epoch detections are separated by 8.8" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:13:29.83 +56:53:48.5 (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 00:13:29.83 +56:53:48.5: 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 00:13:29.83 +56:53:48.5: 15.68 +/- 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 26.3298* 00 13 29.83 +56 53 48.5 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.96,0.05,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 20260726.3298 13.96CV 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 26.3298 2461247.8298 14.12 23:48:00.94 +51:54:05.2
113.08309 -9.75337 galactic Cas Second-epoch detections are separated by 5.2" and 9.6 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 J356.9943+51.8907 | 23:48:00.94 +51:54:05.2 (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 23:48:00.94 +51:54:05.2: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:48:00.94 +51:54:05.2: 15.72 +/- 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 26.3298* 23 48 00.94 +51 54 05.2 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.9943+51.8907,2461247.8298,14.12,0.05,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
ATO J356.9943+51.8907 20260726.3298 14.12CV 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 26.3298 2461247.8298 14.30 23:52:42.84 +55:29:51.2
114.62566 -6.42429 galactic Cas Second-epoch detections are separated by 2.7" and 9.6 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 J358.2101+55.4878 | 23:52:47.19 +55:29:50.9 (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 23:52:42.84 +55:29:51.2: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:42.84 +55:29:51.2: 15.83 +/- 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 26.3298* 23 52 42.84 +55 29 51.2 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.2101+55.4878,2461247.8298,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.2101+55.4878 20260726.3298 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 14.40 23:34:08.47 +51:33:33.8
110.89230 -9.49636 galactic Cas Second-epoch detections are separated by 5.5" and 9.5 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 1992853143035856640 | 23:34:05.22 +51:33:05.5 (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 23:34:08.47 +51:33:33.8: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:08.47 +51:33:33.8: 15.78 +/- 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 26.3298* 23 34 08.47 +51 33 33.8 14.4 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 1992853143035856640,2461247.8298,14.40,0.05,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 1992853143035856640 20260726.3298 14.40CV 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 26.3298 2461247.8298 13.63 23:27:27.27 +53:55:25.9
110.66046 -6.93485 galactic Cas Second-epoch detections are separated by 2.4" and 9.3 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 | 23:27:27.27 +53:55:25.9 (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 23:27:27.27 +53:55:25.9: 14.73 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:27.27 +53:55:25.9: 14.50 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 27 27.27 +53 55 25.9 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461247.8298,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 12.14 23:59:52.81 +56:58:28.5
115.91993 -5.19359 galactic Cas Second-epoch detections are separated by 1.9" and 9.4 pix
The object was found in VSX22" V0533 Cas
Type: M
# Max. Min./Amp. JD0 Period
15.361 g Y 2.943 g 2458396.91440 296.168262100000 C(N)
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 23:59:52.81 +56:58:28.5: 14.99 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:59:52.81 +56:58:28.5: 14.87 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 26.3298* 23 59 52.81 +56 58 28.5 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
V0533 Cas,2461247.8298,12.14,0.05,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
V0533 Cas 20260726.3298 12.14CV 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 26.3298 2461247.8298 12.32 00:15:48.73 +57:32:19.4
118.14704 -5.00167 galactic Cas Second-epoch detections are separated by 2.3" and 9.5 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 | FN Cas | 00:15:50.54 +57:32:39.3 (Gaia DR3) | M (local) | 173.900000000000 (local) | Gaia3var=VARIABLE SpType: M6 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:48.73 +57:32:19.4: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:48.73 +57:32:19.4: 15.78 +/- 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 26.3298* 00 15 48.73 +57 32 19.4 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
FN Cas,2461247.8298,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FN Cas 20260726.3298 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 26.3298 2461247.8298 12.36 23:21:38.29 +50:06:23.1
108.52053 -10.23576 galactic And Second-epoch detections are separated by 0.7" and 9.4 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 | 23:21:38.29 +50:06:23.1 (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 23:21:38.29 +50:06:23.1: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:38.29 +50:06:23.1: 15.63 +/- 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 26.3298* 23 21 38.29 +50 06 23.1 12.4 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,2461247.8298,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260726.3298 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
## 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: 2461247.83018921 26.07.2026 07:55:18.348 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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: 11 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): 21455
Objects passed selection criteria: 21415
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: 18438.5
Average stars matched: 17537.5 (95.1135 %)
Memory usage VmPeak: 248496 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 26 10:08:23 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: 2461247.83018921 26.07.2026 07:55:18.348 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 310
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: 163 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): 161890
Objects passed selection criteria: 161534
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: 146032
Average stars matched: 139548 (95.56 %)
Memory usage VmPeak: 2115356 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 26 10:18:12 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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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: 2461247.82942575
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_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits'
wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.059 +54:00:13.58 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Image size: 926.6'x616.2' 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: 23:59:56.624 +54:01:36.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.059 +54:00:13.58
Second-epoch image center 23:59:56.624 +54:01:36.61
Angular distance between the image centers 0.0245 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
Image size: 926.6'x616.2' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:00.577 +54:02:20.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.059 +54:00:13.58
Second-epoch image center 00:00:00.577 +54:02:20.48
Angular distance between the image centers 0.0353 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 23:59:56.624 +54:01:36.61
Second-epoch second image center 00:00:00.577 +54:02:20.48
Angular distance between the image centers 0.01556 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.X7wk6XTCJD
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.8JeTgQYVYc
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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits &> /tmp/tmp.tQ7eacLtKy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits &> /tmp/tmp.fCRMHYov5B
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0161 to 14.8837 deg, Dec +48.1259 to +59.2680 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 345.0161 to 14.8837 deg, Dec 48.1259 to 59.2680 deg
Loaded 25395 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): 16157 out of 17527 total matches.
Matched with Tycho-2 17527 out of 28951 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.643500
a=0.000000 b=1.000000 c=22.643500
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.97
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.97
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 28951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0161 to 14.8837 deg, Dec +48.1259 to +59.2680 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 345.0161 to 14.8837 deg, Dec 48.1259 to 59.2680 deg
Loaded 25395 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): 16157 out of 17527 total matches.
Matched with Tycho-2 17527 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)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 32399 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.0247 to 14.8783 deg, Dec +48.1255 to +59.2627 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 345.0247 to 14.8783 deg, Dec 48.1255 to 59.2627 deg
Loaded 25378 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): 15455 out of 16923 total matches.
Matched with Tycho-2 16923 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 2 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_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
2.2 pix fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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:
15.0 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
15.1 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
14.4 mag. fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
14.4 mag. fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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.X7wk6XTCJD (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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/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'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_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: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 345.0161 through 0 to 14.8837, gap 14.8837 to 345.0161
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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: 971 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 22877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 345.0144 through 0 to 14.8842, gap 14.8842 to 345.0144
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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: 971 matched stars entering correct_measured_positions(), 22877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 22877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=971 sigma_overall_arcsec=0.535 sigma_q1_arcsec=0.486 sigma_q2_arcsec=0.579 sigma_q3_arcsec=0.528 sigma_q4_arcsec=0.520 n_q1=294 n_q2=204 n_q3=273 n_q4=200 worst_quadrant_to_overall_ratio=1.084
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.8JeTgQYVYc (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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/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'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_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: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 345.0247 through 0 to 14.8783, gap 14.8783 to 345.0247
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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: 972 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 25959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0167 through 0 to 14.8780, gap 14.8780 to 345.0167
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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: 972 matched stars entering correct_measured_positions(), 25959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 25958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=972 sigma_overall_arcsec=0.568 sigma_q1_arcsec=0.515 sigma_q2_arcsec=0.684 sigma_q3_arcsec=0.541 sigma_q4_arcsec=0.599 n_q1=294 n_q2=214 n_q3=258 n_q4=206 worst_quadrant_to_overall_ratio=1.204
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.tQ7eacLtKy (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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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=1229, bad_region=3407, passed=17135
Got 17135 stars (including 12670 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat
util/solve_plate_with_UCAC5 got 17135 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.6'
Seting catalog search parameters based on the expected field of view 926.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012869 (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 0.010296 (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 345.0827 through 0 to 14.8807, gap 14.8807 to 345.0827
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 307 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(), 159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 227 matched stars entering correct_measured_positions(), 3983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.30"
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 345.0707 through 0 to 14.9046, gap 14.9046 to 345.0707
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 385 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 328 matched stars entering correct_measured_positions(), 4041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.15"
Accuracy estimation diagnostic: 322 matched stars entering correct_measured_positions(), 5299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.52"
Excluding outliers - 322 stars left (next iteration limit 249)
SIP_REFIT: SIP order 2 trial: matched=322 robust_rms=22.360 arcsec
SIP_REFIT: SIP order 3 trial: matched=322 robust_rms=2.638 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=322 robust_rms_before=39.386 arcsec robust_rms_before_corrected=17.190 arcsec robust_rms_after=2.638 arcsec
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Image size: 925.2'x621.7' 15.4(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.80"/pix along the X axis and 5.84"/pix along the Y axis
Image center: 23:59:59.664 +54:00:42.24 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 17135 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/correct_sextractor_wcs_catalog_usingxy2sky1785399.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 39.386 -> 2.638 arcsec)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits N_match=322 sigma_overall_arcsec=3.309 sigma_q1_arcsec=98.122 sigma_q2_arcsec=55.340 sigma_q3_arcsec=4.697 sigma_q4_arcsec=1.822 n_q1=40 n_q2=26 n_q3=112 n_q4=144 worst_quadrant_to_overall_ratio=29.655
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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.fCRMHYov5B (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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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=1202, bad_region=3364, passed=16627
Got 16627 stars (including 12240 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat
util/solve_plate_with_UCAC5 got 16627 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.6'
Seting catalog search parameters based on the expected field of view 926.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012869 (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 0.010296 (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 345.0825 through 0 to 14.8804, gap 14.8804 to 345.0825
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 314 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 155 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 223 matched stars entering correct_measured_positions(), 3738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.33"
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 345.0722 through 0 to 14.9040, gap 14.9040 to 345.0722
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(), 3816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.17"
Accuracy estimation diagnostic: 336 matched stars entering correct_measured_positions(), 5267 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.51"
Excluding outliers - 336 stars left (next iteration limit 245)
SIP_REFIT: SIP order 2 trial: matched=336 robust_rms=22.186 arcsec
SIP_REFIT: SIP order 3 trial: matched=336 robust_rms=2.946 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=336 robust_rms_before=41.460 arcsec robust_rms_before_corrected=17.980 arcsec robust_rms_after=2.946 arcsec
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
Image size: 923.5'x618.1' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.79"/pix along the X axis and 5.81"/pix along the Y axis
Image center: 00:00:03.245 +54:01:36.70 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 16627 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/correct_sextractor_wcs_catalog_usingxy2sky1785398.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 41.460 -> 2.946 arcsec)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits N_match=336 sigma_overall_arcsec=3.724 sigma_q1_arcsec=52.428 sigma_q2_arcsec=44.621 sigma_q3_arcsec=6.395 sigma_q4_arcsec=1.992 n_q1=39 n_q2=22 n_q3=113 n_q4=162 worst_quadrant_to_overall_ratio=14.078
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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=0.535 worst_q_ratio=1.084
ref2=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits sigma_overall=0.568 worst_q_ratio=1.204
new1=fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits sigma_overall=3.309 worst_q_ratio=29.655
new2=fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits sigma_overall=3.724 worst_q_ratio=14.078
reference average sigma_overall=0.5515 worst_q_ratio=1.144
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits) flagged: sigma=3.309 (ref avg 0.5515), ratio=29.655 (ref avg 1.144), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/lib/make_outxyls_for_astrometric_calibration found 16520 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out1830107.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1830107.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 28.3877 (2.13121e+12), 8 match, 0 conflict, 19 distractors, 24 index.
RA,Dec = (359.983,54.0252), pixel scale 5.93014 arcsec/pix.
Hit/miss: Hit/miss: ----++----+--+--+---+---+-+(best)-------------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1830107.solved to indicate this.
Field: out1830107.xyls
Field center: (RA,Dec) = (359.984545, 54.026015) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:56.291, +54:01:33.655).
Field size: 15.6029 x 10.4309 degrees
Field rotation angle: up is 3.99914 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits' -> 'fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 26 10:12 fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
-rw-r--r-- 1 apache apache 8.5K Jul 26 10:12 out1830107.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits (fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out1830107.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1830107.axy"...
Only searching for solutions within 15.4433 degrees of RA,Dec (359.986,54.0268)
log-odds ratio 28.3877 (2.13121e+12), 8 match, 0 conflict, 19 distractors, 24 index.
RA,Dec = (359.983,54.0252), pixel scale 5.93014 arcsec/pix.
Hit/miss: Hit/miss: ----++----+--+--+---+---+-+(best)-------------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1830107.solved to indicate this.
Field: out1830107.xyls
Field center: (RA,Dec) = (359.984545, 54.026015) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:56.291, +54:01:33.655).
Field size: 15.6029 x 10.4309 degrees
Field rotation angle: up is 3.99914 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 26 10:12 fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
-rw-r--r-- 1 apache apache 8.5K Jul 26 10:12 out1830107.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat from image00003.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Image size: 926.6'x616.2' 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: 23:59:56.624 +54:01:36.61 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 17135 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/correct_sextractor_wcs_catalog_usingxy2sky1833025.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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=1229, bad_region=3407, passed=17135
Got 17135 stars (including 12670 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat
util/solve_plate_with_UCAC5 got 17135 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.6'
Seting catalog search parameters based on the expected field of view 926.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012869 (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 0.010296 (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 345.0827 through 0 to 14.8807, gap 14.8807 to 345.0827
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 307 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(), 159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 227 matched stars entering correct_measured_positions(), 3983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.30"
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 345.0707 through 0 to 14.9046, gap 14.9046 to 345.0707
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 385 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 328 matched stars entering correct_measured_positions(), 4041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.15"
Accuracy estimation diagnostic: 322 matched stars entering correct_measured_positions(), 5299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.52"
Excluding outliers - 322 stars left (next iteration limit 249)
SIP_REFIT: SIP order 2 trial: matched=322 robust_rms=22.360 arcsec
SIP_REFIT: SIP order 3 trial: matched=322 robust_rms=2.638 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=322 robust_rms_before=39.386 arcsec robust_rms_before_corrected=17.190 arcsec robust_rms_after=2.638 arcsec
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Image size: 925.2'x621.7' 15.4(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.80"/pix along the X axis and 5.84"/pix along the Y axis
Image center: 23:59:59.664 +54:00:42.24 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 17135 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/correct_sextractor_wcs_catalog_usingxy2sky1840202.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 39.386 -> 2.638 arcsec)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits N_match=322 sigma_overall_arcsec=3.309 sigma_q1_arcsec=98.122 sigma_q2_arcsec=55.340 sigma_q3_arcsec=4.697 sigma_q4_arcsec=1.822 n_q1=40 n_q2=26 n_q3=112 n_q4=144 worst_quadrant_to_overall_ratio=29.655
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits): sigma 3.309->3.309, ratio 29.655->29.655; reverting to order 3
WCS_QUALITY_RETRY: 2nd new image (fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits) flagged: sigma=3.724 (ref avg 0.5515), ratio=14.078 (ref avg 1.144), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/lib/make_outxyls_for_astrometric_calibration found 16026 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out1840355.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1840355.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 26.4293 (3.00665e+11), 7 match, 0 conflict, 18 distractors, 24 index.
RA,Dec = (360,54.0374), pixel scale 5.93031 arcsec/pix.
Hit/miss: Hit/miss: ----+++----+----+---+---+(best)-------+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1840355.solved to indicate this.
Field: out1840355.xyls
Field center: (RA,Dec) = (0.001016, 54.038202) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:00.244, +54:02:17.527).
Field size: 15.6038 x 10.4316 degrees
Field rotation angle: up is 3.99177 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits' -> 'fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 26 10:13 fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
-rw-r--r-- 1 apache apache 8.5K Jul 26 10:13 out1840355.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits (fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out1840355.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1840355.axy"...
Only searching for solutions within 15.4433 degrees of RA,Dec (0.00240417,54.039)
log-odds ratio 26.4293 (3.00665e+11), 7 match, 0 conflict, 18 distractors, 24 index.
RA,Dec = (360,54.0374), pixel scale 5.93031 arcsec/pix.
Hit/miss: Hit/miss: ----+++----+----+---+---+(best)-------+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1840355.solved to indicate this.
Field: out1840355.xyls
Field center: (RA,Dec) = (0.001016, 54.038202) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:00.244, +54:02:17.527).
Field size: 15.6038 x 10.4316 degrees
Field rotation angle: up is 3.99177 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Jul 26 10:13 fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
-rw-r--r-- 1 apache apache 8.5K Jul 26 10:13 out1840355.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat from image00004.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
Image size: 926.6'x616.2' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:00.577 +54:02:20.48 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 16627 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/correct_sextractor_wcs_catalog_usingxy2sky1840986.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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=1202, bad_region=3364, passed=16627
Got 16627 stars (including 12240 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat
util/solve_plate_with_UCAC5 got 16627 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.6'
Seting catalog search parameters based on the expected field of view 926.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012869 (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 0.010296 (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 345.0825 through 0 to 14.8804, gap 14.8804 to 345.0825
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 314 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 233 matched stars entering correct_measured_positions(), 155 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 223 matched stars entering correct_measured_positions(), 3738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.33"
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 345.0722 through 0 to 14.9040, gap 14.9040 to 345.0722
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(), 3816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.17"
Accuracy estimation diagnostic: 336 matched stars entering correct_measured_positions(), 5267 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.51"
Excluding outliers - 336 stars left (next iteration limit 245)
SIP_REFIT: SIP order 2 trial: matched=336 robust_rms=22.186 arcsec
SIP_REFIT: SIP order 3 trial: matched=336 robust_rms=2.946 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=336 robust_rms_before=41.460 arcsec robust_rms_before_corrected=17.980 arcsec robust_rms_after=2.946 arcsec
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
Image size: 923.5'x618.1' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.79"/pix along the X axis and 5.81"/pix along the Y axis
Image center: 00:00:03.245 +54:01:36.70 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 16627 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/correct_sextractor_wcs_catalog_usingxy2sky1885847.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 41.460 -> 2.946 arcsec)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits N_match=336 sigma_overall_arcsec=3.724 sigma_q1_arcsec=52.428 sigma_q2_arcsec=44.621 sigma_q3_arcsec=6.395 sigma_q4_arcsec=1.992 n_q1=39 n_q2=22 n_q3=113 n_q4=162 worst_quadrant_to_overall_ratio=14.078
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 2nd new image (fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits): sigma 3.724->3.724, ratio 14.078->14.078; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=3.309 -- 6.00x the reference average (0.5515); plate solution may be of low accuracy
WARNING: 2nd new image has sigma_overall_arcsec=3.724 -- 6.75x the reference average (0.5515); plate solution may be of low accuracy
WARNING: 1st new image has worst_quadrant_to_overall_ratio=29.655 -- 25.92x the reference average (1.144); plate solution may be of low accuracy
WARNING: 2nd new image has worst_quadrant_to_overall_ratio=14.078 -- 12.31x the reference average (1.144); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468_astrometric_residuals.png (971 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 0.49 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 (972 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 0.52 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089_astrometric_residuals.png (322 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 2.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090_astrometric_residuals.png (336 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 2.67 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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 23:44:32.67 +56:34:54.3: 11.54 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:32.67 +56:34:54.3: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Forced photometry filter KEPT candidate at 23:44:32.67 +56:34:54.3: ref_mag=11.46 +/- 0.01 new_mean_mag=9.7892 delta=1.67 (need > 0.90)
Adding exclusion_list_local.txt__out21482.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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 21482_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 21482_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07077_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 07077_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (87.1") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:44:32.67 +56:34:54.3
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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.059 +54:00:13.58 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Image size: 926.6'x616.2' 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: 23:59:56.624 +54:01:36.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.059 +54:00:13.58
Second-epoch image center 23:59:56.624 +54:01:36.61
Angular distance between the image centers 0.0245 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
Image size: 926.6'x616.2' 15.4(deg)x10.3(deg) 9576x6388 pix
Image scale: 5.81"/pix along the X axis and 5.79"/pix along the Y axis
Image center: 00:00:00.577 +54:02:20.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.059 +54:00:13.58
Second-epoch image center 00:00:00.577 +54:02:20.48
Angular distance between the image centers 0.0353 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 23:59:56.624 +54:01:36.61
Second-epoch second image center 00:00:00.577 +54:02:20.48
Angular distance between the image centers 0.01556 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.GCXqqoUrml
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.VbAQMJhnWi
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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits &> /tmp/tmp.bGKLEAvjOQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits &> /tmp/tmp.M8OirzZoyT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 344.9469 to 14.9293 deg, Dec +48.1259 to +59.2679 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 344.9469 to 14.9293 deg, Dec 48.1259 to 59.2679 deg
Loaded 25504 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): 13217 out of 18826 total matches.
Matched with Tycho-2 18826 out of 200953 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.479600
a=0.000000 b=1.000000 c=22.479600
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 200953 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 344.9469 to 14.9293 deg, Dec +48.1259 to +59.2679 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 344.9469 to 14.9293 deg, Dec 48.1259 to 59.2679 deg
Loaded 25504 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): 13217 out of 18826 total matches.
Matched with Tycho-2 18826 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)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 213202 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 344.9557 to 14.9265 deg, Dec +48.1255 to +59.2648 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 344.9557 to 14.9265 deg, Dec 48.1255 to 59.2648 deg
Loaded 25491 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): 12093 out of 17553 total matches.
Matched with Tycho-2 17553 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 247 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_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
2.0 pix fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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:
15.2 mag. Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits
15.3 mag. Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits
14.6 mag. fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
14.6 mag. fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (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.GCXqqoUrml (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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/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'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-20_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: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 344.9469 through 0 to 14.9293, gap 14.9293 to 344.9469
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 174760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 344.9450 through 0 to 14.9299, gap 14.9299 to 344.9450
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 174760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 174760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits N_match=977 sigma_overall_arcsec=0.535 sigma_q1_arcsec=0.515 sigma_q2_arcsec=0.571 sigma_q3_arcsec=0.509 sigma_q4_arcsec=0.515 n_q1=275 n_q2=220 n_q3=262 n_q4=220 worst_quadrant_to_overall_ratio=1.066
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.VbAQMJhnWi (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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/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'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-06-21_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: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 344.9557 through 0 to 14.9265, gap 14.9265 to 344.9557
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 188817 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 344.9477 through 0 to 14.9262, gap 14.9262 to 344.9477
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.1 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(), 188817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 188816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits N_match=975 sigma_overall_arcsec=0.588 sigma_q1_arcsec=0.537 sigma_q2_arcsec=0.678 sigma_q3_arcsec=0.584 sigma_q4_arcsec=0.617 n_q1=276 n_q2=220 n_q3=267 n_q4=212 worst_quadrant_to_overall_ratio=1.153
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.bGKLEAvjOQ (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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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=1, no_mag_err=0, low_SNR=19, blended=13052, bad_region=16516, passed=133394
Got 133394 stars (including 105320 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat
util/solve_plate_with_UCAC5 got 133394 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.6'
Seting catalog search parameters based on the expected field of view 926.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012869 (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 0.010296 (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 345.0124 through 0 to 15.0327, gap 15.0327 to 345.0124
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 307 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 222 matched stars entering correct_measured_positions(), 161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.00"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 216 matched stars entering correct_measured_positions(), 32344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.05"
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 345.0040 through 0 to 15.0605, gap 15.0605 to 345.0040
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 389 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 321 matched stars entering correct_measured_positions(), 32391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.05"
Accuracy estimation diagnostic: 313 matched stars entering correct_measured_positions(), 42562 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.91"
Excluding outliers - 313 stars left (next iteration limit 237)
SIP_REFIT: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits N_match=313 sigma_overall_arcsec=10.112 sigma_q1_arcsec=27.893 sigma_q2_arcsec=33.724 sigma_q3_arcsec=8.903 sigma_q4_arcsec=9.179 n_q1=36 n_q2=23 n_q3=119 n_q4=135 worst_quadrant_to_overall_ratio=3.335
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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.M8OirzZoyT (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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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=18, blended=12747, bad_region=16520, passed=132795
Got 132795 stars (including 105130 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat
util/solve_plate_with_UCAC5 got 132795 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.6'
Seting catalog search parameters based on the expected field of view 926.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012869 (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 0.010296 (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 345.0161 through 0 to 15.0269, gap 15.0269 to 345.0161
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 312 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 226 matched stars entering correct_measured_positions(), 160 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 221 matched stars entering correct_measured_positions(), 29814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.88"
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 345.0067 through 0 to 15.0522, gap 15.0522 to 345.0067
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 386 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 321 matched stars entering correct_measured_positions(), 29853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.86"
Accuracy estimation diagnostic: 319 matched stars entering correct_measured_positions(), 42161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.36"
Excluding outliers - 319 stars left (next iteration limit 243)
SIP_REFIT: wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits N_match=319 sigma_overall_arcsec=9.737 sigma_q1_arcsec=28.646 sigma_q2_arcsec=27.346 sigma_q3_arcsec=7.628 sigma_q4_arcsec=8.238 n_q1=37 n_q2=25 n_q3=123 n_q4=134 worst_quadrant_to_overall_ratio=2.942
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits -region wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-54-12_20.00sec_5.00C_LIGHT_0089.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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_2026-07-26_CI_Cas-04-Q2b1x1_060548_TTUQ2b1x1_1114740_F5geupGd/wcs_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090.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 00:03:18.68 +53:36:05.5: 15.11 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:02:53.27 +56:47:56.8: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:02:37.40 +55:49:29.5: 15.52 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:35:05.74 +56:37:22.4: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:44.76 +53:03:00.1: 13.40 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:11.54 +50:29:26.2: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:00.89 +55:10:15.3: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:29:49.87 +57:44:24.4: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:47.68 +55:42:05.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:18.68 +53:36:05.5: 14.94 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.12
Forced photometry filter REJECTED candidate at 00:03:18.68 +53:36:05.5: ref_mag=15.00 +/- 0.12 new_mean_mag=14.1897 delta=0.81 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:53.27 +56:47:56.8: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:35:05.74 +56:37:22.4: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:37.40 +55:49:29.5: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:44.76 +53:03:00.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 15.52 +/- 0.31
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:47:00.89 +55:10:15.3: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:29:49.87 +57:44:24.4: 15.81 +/- 99.00 upperlimit
Forced photometry filter KEPT candidate at 00:02:37.40 +55:49:29.5: ref_mag=15.52 +/- 0.31 new_mean_mag=14.5131 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:11.54 +50:29:26.2: 15.83 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 00:11:44.76 +53:03:00.1: ref_mag=13.29 +/- 0.02 new_mean_mag=14.5018 delta=-1.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:47.68 +55:42:05.1: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:52.73 +55:03:44.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:39.20 +55:18:48.8: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:40.09 +53:04:18.5: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:52.73 +55:03:44.2: 15.71 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.71 +/- 0.29
Forced photometry filter KEPT candidate at 23:56:52.73 +55:03:44.2: ref_mag=15.71 +/- 0.29 new_mean_mag=13.9793 delta=1.73 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:39.20 +55:18:48.8: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:40.09 +53:04:18.5: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:48:20.18 +55:11:05.3: 15.52 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:48:20.18 +55:11:05.3: 15.67 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.59 +/- 0.21
Forced photometry filter KEPT candidate at 23:48:20.18 +55:11:05.3: ref_mag=15.59 +/- 0.21 new_mean_mag=13.8861 delta=1.70 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:07.59 +57:29:56.1: 14.56 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:07.59 +57:29:56.1: 14.60 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.09
Forced photometry filter REJECTED candidate at 23:49:07.59 +57:29:56.1: ref_mag=14.58 +/- 0.09 new_mean_mag=14.0001 delta=0.58 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:11:00.58 +52:48:13.1: 14.64 +/- 0.12 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:00.58 +52:48:13.1: 15.06 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.10
Forced photometry filter KEPT candidate at 00:11:00.58 +52:48:13.1: ref_mag=14.78 +/- 0.10 new_mean_mag=13.6933 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:14.23 +57:10:04.3: 13.16 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:14.23 +57:10:04.3: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Forced photometry filter REJECTED candidate at 23:23:14.23 +57:10:04.3: ref_mag=13.17 +/- 0.03 new_mean_mag=14.1441 delta=-0.97 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:20.84 +57:27:25.3: 14.66 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:20.84 +57:27:25.3: 14.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.07
Forced photometry filter REJECTED candidate at 23:43:20.84 +57:27:25.3: ref_mag=14.46 +/- 0.07 new_mean_mag=14.0142 delta=0.45 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:35.15 +56:39:17.8: 12.62 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:35.15 +56:39:17.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter REJECTED candidate at 00:00:35.15 +56:39:17.8: ref_mag=12.67 +/- 0.01 new_mean_mag=13.7814 delta=-1.12 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:09.88 +57:06:07.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:45.38 +57:15:51.9: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:32.13 +54:07:42.3: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:09.88 +57:06:07.9: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:25.71 +57:02:54.6: 15.76 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:45.38 +57:15:51.9: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:32.13 +54:07:42.3: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:01:41.42 +55:30:22.1: 12.73 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:25.71 +57:02:54.6: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:14.74 +56:24:08.4: 15.62 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.76 +/- 0.35
Forced photometry filter KEPT candidate at 00:15:25.71 +57:02:54.6: ref_mag=15.76 +/- 0.35 new_mean_mag=13.8757 delta=1.89 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:22.47 +52:21:55.0: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:01:41.42 +55:30:22.1: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter REJECTED candidate at 00:01:41.42 +55:30:22.1: ref_mag=12.75 +/- 0.01 new_mean_mag=13.8378 delta=-1.09 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:14.74 +56:24:08.4: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:22.47 +52:21:55.0: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:35.07 +55:18:05.3: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:35.07 +55:18:05.3: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:38:03.17 +51:03:31.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:38:03.17 +51:03:31.7: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:35.16 +54:22:00.3: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:35.16 +54:22:00.3: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:49.80 +52:35:26.1: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:41.19 +53:38:23.8: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:49.80 +52:35:26.1: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:41.19 +53:38:23.8: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:52.09 +55:47:52.0: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:52.09 +55:47:52.0: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:08:31.06 +56:46:19.6: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:31.06 +56:46:19.6: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:36.82 +50:24:58.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:36.82 +50:24:58.0: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:23.28 +51:58:06.5: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:23.28 +51:58:06.5: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:44.85 +55:12:16.6: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:57.58 +51:38:37.7: 14.01 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:05.34 +55:19:44.4: 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 23:37:44.85 +55:12:16.6: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:57.58 +51:38:37.7: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:05.34 +55:19:44.4: 15.72 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:30:57.58 +51:38:37.7: ref_mag=14.02 +/- 0.05 new_mean_mag=13.7549 delta=0.26 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:22.00 +52:30:46.5: 15.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:48.56 +53:38:09.1: 13.77 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:22.00 +52:30:46.5: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:48.56 +53:38:09.1: 13.64 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Forced photometry filter REJECTED candidate at 23:28:48.56 +53:38:09.1: ref_mag=13.70 +/- 0.04 new_mean_mag=13.7321 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 23:25:38.82 +57:34:19.1: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:22.56 +56:55:30.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:52.86 +52:08:27.7: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:38.82 +57:34:19.1: 15.55 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.55 +/- 0.29
Forced photometry filter KEPT candidate at 23:25:38.82 +57:34:19.1: ref_mag=15.55 +/- 0.29 new_mean_mag=13.6576 delta=1.89 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:22.56 +56:55:30.8: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:52.86 +52:08:27.7: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:56.59 +57:29:20.6: 13.76 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:56.59 +57:29:20.6: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter REJECTED candidate at 23:41:56.59 +57:29:20.6: ref_mag=13.79 +/- 0.04 new_mean_mag=13.6815 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 00:11:44.19 +54:49:05.1: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:11:44.19 +54:49:05.1: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:46.67 +54:41:49.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:46.67 +54:41:49.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:38.30 +56:24:23.5: 15.68 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:44.00 +54:04:10.8: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:38.30 +56:24:23.5: 15.54 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.60 +/- 0.22
Forced photometry filter KEPT candidate at 23:56:38.30 +56:24:23.5: ref_mag=15.60 +/- 0.22 new_mean_mag=13.4261 delta=2.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:50:35.75 +57:09:06.4: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:44.00 +54:04:10.8: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:35.75 +57:09:06.4: 15.49 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.49 +/- 0.36
Forced photometry filter KEPT candidate at 23:50:35.75 +57:09:06.4: ref_mag=15.49 +/- 0.36 new_mean_mag=13.5110 delta=1.98 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:57.46 +54:34:29.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:57.46 +54:34:29.6: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:08.26 +53:39:22.1: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:31.37 +56:31:47.0: 15.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:08.26 +53:39:22.1: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:31.37 +56:31:47.0: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:28.59 +57:43:47.1: 11.83 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:45.99 +53:19:15.9: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:28.59 +57:43:47.1: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Forced photometry filter REJECTED candidate at 00:24:28.59 +57:43:47.1: ref_mag=11.76 +/- 0.01 new_mean_mag=13.3306 delta=-1.57 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:45.99 +53:19:15.9: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:26.14 +56:13:16.2: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:37:15.03 +56:33:09.8: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:26.14 +56:13:16.2: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:37:15.03 +56:33:09.8: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:14.17 +56:29:46.7: 13.89 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:14.17 +56:29:46.7: 14.25 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.06
Forced photometry filter REJECTED candidate at 23:57:14.17 +56:29:46.7: ref_mag=14.04 +/- 0.06 new_mean_mag=13.2956 delta=0.74 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:30.10 +54:53:43.2: 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 23:30:30.10 +54:53:43.2: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:57.48 +54:10:54.8: 14.92 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:57.48 +54:10:54.8: 15.26 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.92 +/- 0.28
Forced photometry filter KEPT candidate at 23:31:57.48 +54:10:54.8: ref_mag=14.92 +/- 0.28 new_mean_mag=13.3545 delta=1.57 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:01.09 +54:18:02.6: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:58.11 +56:44:18.6: 14.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:01.09 +54:18:02.6: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:58.11 +56:44:18.6: 14.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:53.68 +56:42:23.9: 11.22 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:53.68 +56:42:23.9: 11.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Forced photometry filter REJECTED candidate at 23:57:53.68 +56:42:23.9: ref_mag=11.20 +/- 0.01 new_mean_mag=13.1361 delta=-1.94 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:37.14 +53:54:47.1: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:57.02 +56:53:10.3: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:37.14 +53:54:47.1: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:57.02 +56:53:10.3: 15.70 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.70 +/- 0.35
Forced photometry filter KEPT candidate at 23:45:57.02 +56:53:10.3: ref_mag=15.70 +/- 0.35 new_mean_mag=13.1392 delta=2.56 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:39:40.85 +57:15:46.7: 14.16 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:39:40.85 +57:15:46.7: 14.27 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.06
Forced photometry filter KEPT candidate at 23:39:40.85 +57:15:46.7: ref_mag=14.21 +/- 0.06 new_mean_mag=13.0760 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:30.79 +57:13:04.9: 14.53 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:30.79 +57:13:04.9: 14.26 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.08
Forced photometry filter KEPT candidate at 23:28:30.79 +57:13:04.9: ref_mag=14.35 +/- 0.08 new_mean_mag=13.1446 delta=1.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:13:55.36 +55:22:07.2: 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 23:13:55.36 +55:22:07.2: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:18.68 +53:23:10.0: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:18.68 +53:23:10.0: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:18.23 +56:52:14.2: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:18.23 +56:52:14.2: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:31.43 +56:44:11.0: 13.14 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:31.43 +56:44:11.0: 13.19 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.04
Forced photometry filter REJECTED candidate at 23:56:31.43 +56:44:11.0: ref_mag=13.17 +/- 0.04 new_mean_mag=12.8001 delta=0.37 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:54.60 +56:27:28.4: 14.72 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:54.60 +56:27:28.4: 14.46 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.13
Forced photometry filter KEPT candidate at 23:11:54.60 +56:27:28.4: ref_mag=14.55 +/- 0.13 new_mean_mag=13.0240 delta=1.53 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:03.46 +56:00:09.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:03.46 +56:00:09.2: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:30.45 +55:24:07.9: 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 23:21:30.45 +55:24:07.9: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:51:58.61 +53:09:19.2: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:14:33.63 +54:33:11.9: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:51:58.61 +53:09:19.2: 15.71 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.71 +/- 0.36
Forced photometry filter KEPT candidate at 23:51:58.61 +53:09:19.2: ref_mag=15.71 +/- 0.36 new_mean_mag=12.6984 delta=3.01 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:14:33.63 +54:33:11.9: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:11:29.55 +56:00:28.5: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:11:29.55 +56:00:28.5: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:16.91 +52:28:06.7: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:16.91 +52:28:06.7: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:19:14.05 +56:28:30.4: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:19:14.05 +56:28:30.4: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:04.37 +54:51:00.3: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:04.37 +54:51:00.3: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:48.98 +53:52:50.1: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:48.73 +49:42:25.7: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:48.98 +53:52:50.1: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:48.73 +49:42:25.7: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:47.40 +50:45:10.4: 15.73 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:47.40 +50:45:10.4: 15.73 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.73 +/- 0.23
Forced photometry filter KEPT candidate at 23:36:47.40 +50:45:10.4: ref_mag=15.73 +/- 0.23 new_mean_mag=11.9345 delta=3.80 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:13.25 +55:40:59.4: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:13.25 +55:40:59.4: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:54:34.65 +57:28:04.2: 14.41 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:54:34.65 +57:28:04.2: 14.26 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.08
Forced photometry filter KEPT candidate at 23:54:34.65 +57:28:04.2: ref_mag=14.32 +/- 0.08 new_mean_mag=12.5812 delta=1.74 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:22:57.69 +55:45:15.2: 15.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:22:57.69 +55:45:15.2: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:48.61 +53:19:00.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:48.61 +53:19:00.9: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:55.17 +56:19:46.5: 14.59 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:12.74 +57:25:28.7: 14.36 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:55.17 +56:19:46.5: 14.63 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.11
Forced photometry filter KEPT candidate at 23:43:55.17 +56:19:46.5: ref_mag=14.61 +/- 0.11 new_mean_mag=12.6178 delta=1.99 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:47:12.74 +57:25:28.7: 14.38 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.08
Forced photometry filter KEPT candidate at 23:47:12.74 +57:25:28.7: ref_mag=14.38 +/- 0.08 new_mean_mag=12.7131 delta=1.66 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:45.78 +57:23:00.7: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:45.78 +57:23:00.7: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:38.33 +53:47:40.3: 15.59 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:38.33 +53:47:40.3: 15.68 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.59 +/- 0.36
Forced photometry filter KEPT candidate at 23:26:38.33 +53:47:40.3: ref_mag=15.59 +/- 0.36 new_mean_mag=12.8517 delta=2.74 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:26.68 +54:23:40.1: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:22:02.31 +55:43:41.1: 15.00 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:26.68 +54:23:40.1: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:22:02.31 +55:43:41.1: 15.77 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.00 +/- 0.20
Forced photometry filter KEPT candidate at 23:22:02.31 +55:43:41.1: ref_mag=15.00 +/- 0.20 new_mean_mag=13.0213 delta=1.98 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:53:36.03 +56:58:47.5: 12.72 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:49.01 +54:46:38.0: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:53:36.03 +56:58:47.5: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Forced photometry filter REJECTED candidate at 23:53:36.03 +56:58:47.5: ref_mag=12.73 +/- 0.02 new_mean_mag=12.9568 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:49.01 +54:46:38.0: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:57.64 +50:30:08.3: 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 23:57:57.64 +50:30:08.3: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:54.05 +56:28:12.2: 14.15 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:54.05 +56:28:12.2: 14.06 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.11
Forced photometry filter KEPT candidate at 23:57:54.05 +56:28:12.2: ref_mag=14.10 +/- 0.11 new_mean_mag=13.0209 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:16:43.64 +53:37:41.2: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:16:43.64 +53:37:41.2: 15.12 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.22
Forced photometry filter KEPT candidate at 23:16:43.64 +53:37:41.2: ref_mag=15.12 +/- 0.22 new_mean_mag=13.3195 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 23:25:19.53 +55:06:28.9: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:19.53 +55:06:28.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:23.41 +57:57:12.0: 14.55 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:23.41 +57:57:12.0: 14.75 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.11
Forced photometry filter KEPT candidate at 23:30:23.41 +57:57:12.0: ref_mag=14.64 +/- 0.11 new_mean_mag=13.3196 delta=1.32 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:59:03.31 +53:35:20.6: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:59:03.31 +53:35:20.6: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:27:08.86 +50:01:08.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:27:08.86 +50:01:08.3: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:10:52.33 +57:01:38.7: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:10:52.33 +57:01:38.7: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:23:19.84 +55:48:54.7: 13.27 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:23:19.84 +55:48:54.7: 13.33 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.04
Forced photometry filter REJECTED candidate at 00:23:19.84 +55:48:54.7: ref_mag=13.30 +/- 0.04 new_mean_mag=13.1000 delta=0.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:35.65 +56:24:23.9: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:35.65 +56:24:23.9: 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 23:18:19.32 +53:13:24.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:55.37 +50:00:03.0: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:19.32 +53:13:24.1: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:55.37 +50:00:03.0: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:50.05 +54:41:49.5: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:50.05 +54:41:49.5: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:09.81 +57:23:10.8: 14.92 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:09.81 +57:23:10.8: 15.28 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.16
Forced photometry filter KEPT candidate at 00:07:09.81 +57:23:10.8: ref_mag=15.06 +/- 0.16 new_mean_mag=13.1985 delta=1.86 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:56.35 +50:30:59.5: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:56.35 +50:30:59.5: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:20:02.82 +50:08:55.9: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:34.56 +54:49:21.5: 12.86 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:02.82 +50:08:55.9: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:40:52.98 +57:50:35.7: 15.19 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:34.56 +54:49:21.5: 13.00 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.03
Forced photometry filter REJECTED candidate at 23:28:34.56 +54:49:21.5: ref_mag=12.93 +/- 0.03 new_mean_mag=13.4276 delta=-0.50 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:40:52.98 +57:50:35.7: 15.02 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.16
Forced photometry filter KEPT candidate at 23:40:52.98 +57:50:35.7: ref_mag=15.09 +/- 0.16 new_mean_mag=13.4074 delta=1.68 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:31.15 +53:44:48.2: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:31.15 +53:44:48.2: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:45.14 +56:38:12.3: 15.35 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:45.14 +56:38:12.3: 15.47 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.41 +/- 0.22
Forced photometry filter KEPT candidate at 23:49:45.14 +56:38:12.3: ref_mag=15.41 +/- 0.22 new_mean_mag=13.3342 delta=2.07 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:24:49.00 +53:02:22.8: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:24:49.00 +53:02:22.8: 15.52 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.52 +/- 0.32
Forced photometry filter KEPT candidate at 00:24:49.00 +53:02:22.8: ref_mag=15.52 +/- 0.32 new_mean_mag=13.0889 delta=2.43 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:13.11 +50:41:18.4: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:03.95 +54:35:38.9: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:13.11 +50:41:18.4: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:03.95 +54:35:38.9: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:05.29 +50:10:17.3: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:05.29 +50:10:17.3: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:40.53 +51:43:30.4: 14.96 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:40.53 +51:43:30.4: 14.64 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.12
Forced photometry filter KEPT candidate at 23:29:40.53 +51:43:30.4: ref_mag=14.74 +/- 0.12 new_mean_mag=13.5949 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:18:33.45 +49:57:07.7: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:18:33.45 +49:57:07.7: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:23.69 +51:59:26.5: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:23.69 +51:59:26.5: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:57:51.72 +56:29:02.3: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:11.66 +55:19:43.6: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:57:51.72 +56:29:02.3: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:11.66 +55:19:43.6: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:54.22 +55:26:00.4: 14.68 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:54.22 +55:26:00.4: 14.64 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.10
Forced photometry filter KEPT candidate at 23:31:54.22 +55:26:00.4: ref_mag=14.65 +/- 0.10 new_mean_mag=13.4715 delta=1.18 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:41:54.02 +54:40:53.6: 13.80 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:41:54.02 +54:40:53.6: 13.97 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Forced photometry filter REJECTED candidate at 23:41:54.02 +54:40:53.6: ref_mag=13.88 +/- 0.05 new_mean_mag=13.5174 delta=0.37 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:56.66 +53:41:08.0: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:56.66 +53:41:08.0: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:31.14 +55:55:32.2: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:31.14 +55:55:32.2: 15.03 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.21
Forced photometry filter KEPT candidate at 23:21:31.14 +55:55:32.2: ref_mag=15.03 +/- 0.21 new_mean_mag=13.6563 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 00:13:58.31 +55:15:52.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:33.36 +57:13:41.7: 15.34 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:58.31 +55:15:52.0: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:33.36 +57:13:41.7: 15.43 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.38 +/- 0.24
Forced photometry filter KEPT candidate at 00:12:33.36 +57:13:41.7: ref_mag=15.38 +/- 0.24 new_mean_mag=13.4421 delta=1.94 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:12:32.05 +57:05:41.1: 15.00 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:12:32.05 +57:05:41.1: 14.97 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.16
Forced photometry filter KEPT candidate at 23:12:32.05 +57:05:41.1: ref_mag=14.98 +/- 0.16 new_mean_mag=13.5943 delta=1.39 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:38:06.06 +50:59:35.0: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:38:06.06 +50:59:35.0: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:47.26 +54:06:00.7: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:47.26 +54:06:00.7: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:59.80 +57:24:39.0: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:59.80 +57:24:39.0: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:14.10 +49:49:19.5: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:14.10 +49:49:19.5: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:22.58 +51:39:22.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:22.58 +51:39:22.8: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:30:03.04 +54:39:53.7: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:30:03.04 +54:39:53.7: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:05:59.50 +53:17:07.1: 14.00 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:41.94 +58:04:45.8: 15.25 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:05:59.50 +53:17:07.1: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.05
Forced photometry filter REJECTED candidate at 00:05:59.50 +53:17:07.1: ref_mag=14.08 +/- 0.05 new_mean_mag=13.4408 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 00:20:13.49 +57:49:39.8: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:41.94 +58:04:45.8: 15.49 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.36 +/- 0.21
Forced photometry filter KEPT candidate at 23:32:41.94 +58:04:45.8: ref_mag=15.36 +/- 0.21 new_mean_mag=13.6738 delta=1.69 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:20:13.49 +57:49:39.8: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:15:13.26 +52:54:41.3: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:56.41 +53:17:11.7: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:13.26 +52:54:41.3: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:56.41 +53:17:11.7: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:31:53.20 +54:10:53.3: 12.35 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:31:53.20 +54:10:53.3: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Forced photometry filter REJECTED candidate at 23:31:53.20 +54:10:53.3: ref_mag=12.47 +/- 0.02 new_mean_mag=13.6263 delta=-1.16 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:19.66 +54:04:14.6: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:19.66 +54:04:14.6: 15.57 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.57 +/- 0.32
Forced photometry filter KEPT candidate at 23:34:19.66 +54:04:14.6: ref_mag=15.57 +/- 0.32 new_mean_mag=13.6898 delta=1.88 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:49:55.13 +52:10:38.2: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:49:55.13 +52:10:38.2: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:29:37.56 +50:43:08.5: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:29:37.56 +50:43:08.5: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:36:04.26 +51:21:42.2: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:36:04.26 +51:21:42.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:44.71 +53:48:00.6: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:44.71 +53:48:00.6: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:25.85 +55:39:18.2: 14.53 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:25.85 +55:39:18.2: 14.55 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.11
Forced photometry filter KEPT candidate at 00:03:25.85 +55:39:18.2: ref_mag=14.54 +/- 0.11 new_mean_mag=13.5123 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:23:26.73 +57:10:13.4: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:23:26.73 +57:10:13.4: 15.58 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.58 +/- 0.33
Forced photometry filter KEPT candidate at 23:23:26.73 +57:10:13.4: ref_mag=15.58 +/- 0.33 new_mean_mag=13.8464 delta=1.74 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:19:39.43 +50:48:15.0: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:19:39.43 +50:48:15.0: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:20.87 +56:49:48.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:20.87 +56:49:48.3: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:11.82 +54:21:34.3: 13.56 +/- 0.06 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:11.82 +54:21:34.3: 13.63 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry filter REJECTED candidate at 23:52:11.82 +54:21:34.3: ref_mag=13.60 +/- 0.04 new_mean_mag=13.7336 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:08:13.12 +54:03:49.3: 15.23 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:44:18.13 +57:20:24.7: 15.00 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:02:25.22 +54:32:44.9: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:08:13.12 +54:03:49.3: 15.09 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.15
Forced photometry filter KEPT candidate at 00:08:13.12 +54:03:49.3: ref_mag=15.14 +/- 0.15 new_mean_mag=13.6644 delta=1.48 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:44:18.13 +57:20:24.7: 15.02 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.15
Forced photometry filter KEPT candidate at 23:44:18.13 +57:20:24.7: ref_mag=15.01 +/- 0.15 new_mean_mag=13.7967 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:02:25.22 +54:32:44.9: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:56:15.70 +56:09:37.5: 15.57 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:56:15.70 +56:09:37.5: 15.60 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.59 +/- 0.24
Forced photometry filter KEPT candidate at 23:56:15.70 +56:09:37.5: ref_mag=15.59 +/- 0.24 new_mean_mag=13.7231 delta=1.86 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:20:45.16 +55:33:00.2: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:19.87 +55:56:11.3: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:20:45.16 +55:33:00.2: 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 23:21:19.87 +55:56:11.3: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:47:39.62 +56:51:37.1: 15.28 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:47:39.62 +56:51:37.1: 15.34 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.18
Forced photometry filter KEPT candidate at 23:47:39.62 +56:51:37.1: ref_mag=15.31 +/- 0.18 new_mean_mag=13.7406 delta=1.57 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:29.66 +55:06:24.3: 15.45 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:29.66 +55:06:24.3: 15.81 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.60 +/- 0.23
Forced photometry filter KEPT candidate at 23:26:29.66 +55:06:24.3: ref_mag=15.60 +/- 0.23 new_mean_mag=13.8082 delta=1.79 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:58:56.00 +56:57:59.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:58:56.00 +56:57:59.6: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:01.35 +53:36:40.1: 15.10 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:24:41.13 +57:07:10.6: 12.87 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:01.35 +53:36:40.1: 15.39 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.17
Forced photometry filter KEPT candidate at 00:12:01.35 +53:36:40.1: ref_mag=15.21 +/- 0.17 new_mean_mag=13.5797 delta=1.63 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:24:41.13 +57:07:10.6: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter REJECTED candidate at 23:24:41.13 +57:07:10.6: ref_mag=12.85 +/- 0.02 new_mean_mag=13.7704 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 23:50:58.54 +54:43:02.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:50:58.54 +54:43:02.9: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:06:11.22 +51:25:18.4: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:06:11.22 +51:25:18.4: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:26:30.35 +54:30:29.8: 11.57 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:26:30.35 +54:30:29.8: 11.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Forced photometry filter REJECTED candidate at 00:26:30.35 +54:30:29.8: ref_mag=11.60 +/- 0.01 new_mean_mag=13.6063 delta=-2.01 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:42.42 +53:51:09.6: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:34.35 +52:44:22.2: 8.71 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:42.42 +53:51:09.6: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:34.35 +52:44:22.2: 8.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 8.80 +/- 0.00
Forced photometry filter REJECTED candidate at 23:55:34.35 +52:44:22.2: ref_mag=8.80 +/- 0.00 new_mean_mag=13.7838 delta=-4.98 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:45:52.70 +56:56:34.1: 13.05 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:45:52.70 +56:56:34.1: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Forced photometry filter REJECTED candidate at 23:45:52.70 +56:56:34.1: ref_mag=13.11 +/- 0.03 new_mean_mag=13.8380 delta=-0.73 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:25:00.05 +52:51:11.0: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:00:52.63 +53:17:23.0: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:12:49.78 +55:50:22.8: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:25:00.05 +52:51:11.0: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:00:52.63 +53:17:23.0: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:12:49.78 +55:50:22.8: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:03:36.54 +53:56:49.8: 13.28 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:03:36.54 +53:56:49.8: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter REJECTED candidate at 00:03:36.54 +53:56:49.8: ref_mag=13.33 +/- 0.03 new_mean_mag=13.9057 delta=-0.58 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:42:23.25 +51:48:08.2: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:42:23.25 +51:48:08.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:25:08.93 +54:30:24.1: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:25:08.93 +54:30:24.1: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:58.09 +50:49:56.8: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:58.09 +50:49:56.8: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:46:08.13 +49:59:09.7: 14.33 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:55:51.58 +54:53:32.4: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:46:08.13 +49:59:09.7: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.05
Forced photometry filter REJECTED candidate at 23:46:08.13 +49:59:09.7: ref_mag=14.04 +/- 0.05 new_mean_mag=13.9218 delta=0.12 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:55:51.58 +54:53:32.4: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:20.49 +55:42:18.9: 15.19 +/- 0.22 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:20.49 +55:42:18.9: 15.11 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.15
Forced photometry filter KEPT candidate at 23:43:20.49 +55:42:18.9: ref_mag=15.14 +/- 0.15 new_mean_mag=13.9894 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:07:38.40 +57:11:00.6: 15.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:07:38.40 +57:11:00.6: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:26:45.28 +53:47:42.1: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:43:03.76 +52:46:21.9: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:26:45.28 +53:47:42.1: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:43:03.76 +52:46:21.9: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:14:46.44 +53:48:10.2: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:14:46.44 +53:48:10.2: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:09:11.07 +57:36:12.5: 15.45 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:09:11.07 +57:36:12.5: 15.77 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.45 +/- 0.29
Forced photometry filter KEPT candidate at 00:09:11.07 +57:36:12.5: ref_mag=15.45 +/- 0.29 new_mean_mag=13.9780 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 23:15:23.66 +53:33:30.5: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:15:23.66 +53:33:30.5: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:13:29.83 +56:53:48.5: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:48:00.94 +51:54:05.2: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:13:29.83 +56:53:48.5: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:48:00.94 +51:54:05.2: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:28:38.22 +54:05:19.4: 14.83 +/- 0.16 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:28:38.22 +54:05:19.4: 14.77 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.11
Forced photometry filter REJECTED candidate at 23:28:38.22 +54:05:19.4: ref_mag=14.80 +/- 0.11 new_mean_mag=14.2289 delta=0.57 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:32:50.56 +53:53:26.6: 12.73 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:32:50.56 +53:53:26.6: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter REJECTED candidate at 23:32:50.56 +53:53:26.6: ref_mag=12.82 +/- 0.02 new_mean_mag=14.3814 delta=-1.57 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:52:42.84 +55:29:51.2: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:52:42.84 +55:29:51.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:40:33.82 +53:55:52.3: 14.33 +/- 0.10 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:40:33.82 +53:55:52.3: 14.52 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.07
Forced photometry filter REJECTED candidate at 23:40:33.82 +53:55:52.3: ref_mag=14.41 +/- 0.07 new_mean_mag=14.3710 delta=0.04 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:34:08.47 +51:33:33.8: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:34:08.47 +51:33:33.8: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:27:27.27 +53:55:25.9: 14.73 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:27:27.27 +53:55:25.9: 14.50 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.11
Forced photometry filter KEPT candidate at 23:27:27.27 +53:55:25.9: ref_mag=14.57 +/- 0.11 new_mean_mag=13.6251 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:59:52.81 +56:58:28.5: 14.99 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:59:52.81 +56:58:28.5: 14.87 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.11
Forced photometry filter KEPT candidate at 23:59:52.81 +56:58:28.5: ref_mag=14.91 +/- 0.11 new_mean_mag=12.1442 delta=2.77 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 00:15:48.73 +57:32:19.4: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 00:15:48.73 +57:32:19.4: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-20_05-09-15_20.00sec_5.00C_LIGHT_0468.fits at 23:21:38.29 +50:06:23.1: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-06-21_04-58-19_20.00sec_4.90C_LIGHT_0450.fits at 23:21:38.29 +50:06:23.1: 15.63 +/- 99.00 upperlimit
Adding exclusion_list_gaiadr2.txt__out235843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out179100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236177.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): 254s
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: 114s
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Considering the candidate 235410_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235410_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235411_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235411_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235428_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235428_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235429_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235429_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235441_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235441_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235444_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235444_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235451_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235451_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235458_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235458_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 235470_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235470_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235473_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235473_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235480_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235480_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 235490_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235490_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235494_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235494_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235500_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235500_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235508_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235508_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235510_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235510_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 235516_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235516_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235519_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235519_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235524_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235524_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235526_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235526_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235528_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235528_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235531_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235531_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 235538_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235538_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235541_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235541_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235546_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235546_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235549_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235549_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235550_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235550_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235554_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235554_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235559_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235559_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235568_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235568_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 235574_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235574_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235577_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235577_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235586_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235586_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235589_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235589_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235591_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235591_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235596_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235596_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235597_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235597_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 235601_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235601_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235611_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235611_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 235612_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235612_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235613_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235613_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235615_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235615_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235622_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235622_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235625_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235625_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235626_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235626_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235629_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235629_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235630_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235630_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 235634_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235634_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235635_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235635_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235640_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235640_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235644_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235644_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235650_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235650_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 235656_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235656_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235657_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235657_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235659_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235659_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235664_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235664_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235665_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235665_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235669_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235669_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235674_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235674_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235675_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235675_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235679_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235679_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235681_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235681_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235684_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235684_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 235687_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235687_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235688_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235688_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235690_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235690_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235696_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235696_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 235697_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235697_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 235698_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235698_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235701_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235701_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 235702_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235702_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235704_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235704_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 235705_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235705_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235708_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235708_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235712_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235712_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235714_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235714_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235717_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235717_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235718_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235718_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235721_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235721_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 235725_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235725_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235728_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235728_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235729_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235729_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 235732_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235732_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235733_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235733_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235736_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235736_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235737_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235737_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235738_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235738_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235739_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235739_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235740_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235740_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 235743_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235743_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235744_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235744_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235746_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235746_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235747_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235747_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235753_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235753_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235755_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235755_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235756_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235756_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235759_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235759_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235762_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235762_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235783_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235783_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235795_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235795_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
**** FOUND 23:13:25.87 +57:11:38.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235799_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235799_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235800_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235800_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235801_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235801_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
**** FOUND 23:42:04.29 +57:15:53.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235802_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235802_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235803_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235803_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235806_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235806_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235812_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235812_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235814_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235814_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235815_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235815_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
**** FOUND 23:42:05.62 +57:15:21.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235816_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235816_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 235822_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235822_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235825_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235825_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235827_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235827_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 235829_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235829_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235833_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235833_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235835_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235835_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235841_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235841_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235842_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235842_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 235843_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235843_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
**** FOUND 23:16:43.64 +53:37:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.485 1995751769223127936 349.18260880038 +53.62695325180 14.3153 13.3617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235852_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235852_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
**** FOUND 23:43:28.22 +50:59:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235853_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235853_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235854_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235854_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235855_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235855_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235857_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235857_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235860_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235860_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235862_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235862_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235865_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235865_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235868_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235868_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235869_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235869_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235871_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235871_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235872_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235872_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235873_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235873_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235875_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235875_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 235876_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235876_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235878_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235878_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235879_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235879_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235880_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235880_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 235882_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235882_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235883_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235883_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235887_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235887_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235889_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235889_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 235897_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235897_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235898_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235898_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235899_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235899_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235902_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235902_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235903_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235903_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235905_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235905_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 235907_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235907_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235908_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235908_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235909_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235909_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235910_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235910_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235911_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235911_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 235912_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235912_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235914_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235914_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235916_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235916_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235919_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235919_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235923_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235923_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235931_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235931_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235932_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235932_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235935_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235935_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235940_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235940_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235941_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235941_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235944_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235944_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235947_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235947_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235950_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235950_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235953_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235953_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235956_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235956_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235957_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235957_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235958_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235958_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235961_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235961_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235962_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235962_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 235963_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235963_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235967_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235967_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 235968_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235968_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235971_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235971_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 235972_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235972_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
**** FOUND 23:48:26.80 +54:40:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235974_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235974_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235975_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235975_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235978_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235978_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235979_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235979_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 235984_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235984_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235985_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235985_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235987_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235987_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
**** FOUND 00:08:23.72 +54:42:13.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 235989_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235989_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235992_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235992_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 235993_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235993_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 235994_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 235994_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 235995_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 235995_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236000_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236000_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236002_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236002_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236003_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236003_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236005_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236005_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236009_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236009_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236010_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236010_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236011_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236011_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236012_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236012_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236015_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236015_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 236016_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236016_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236017_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236017_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 236020_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236020_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 236024_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236024_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236025_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236025_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236030_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236030_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 236031_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236031_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236036_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236036_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 236037_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236037_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 236038_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236038_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
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Considering the candidate 236039_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236039_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 236044_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236044_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236045_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236045_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
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Considering the candidate 236047_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236047_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236048_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236048_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236050_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236050_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 236053_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236053_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236055_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236055_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236059_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236059_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236062_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236062_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
**** FOUND 23:56:17.25 +53:11:16.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 236064_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236064_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236065_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236065_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236069_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236069_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236072_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236072_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236081_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236081_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236083_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236083_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236087_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236087_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236091_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236091_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236102_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236102_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236111_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236111_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236112_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236112_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236122_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236122_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236126_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236126_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236128_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236128_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236134_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236134_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236135_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236135_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236141_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236141_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 236147_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236147_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236148_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236148_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 236160_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236160_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236162_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236162_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 236171_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 236171_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236177_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 236177_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46841_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 46841_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219159_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 219159_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191364_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 191364_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179100_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 179100_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
Preparing report for the candidate 25587_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197606_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 197606_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
**** FOUND 23:44:31.88 +56:34:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121532_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090
The candidate 121532_fd_Cas-04-Q2b1x1_2026-07-26_02-55-18_20.00sec_4.90C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 14s
make_report_in_HTML.sh TOTAL: 382s
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 ####
23:44:32.67 +56:34:54.3
00:15:48.73 +57:32:19.4
23:59:52.81 +56:58:28.5
23:27:27.27 +53:55:25.9
00:02:37.40 +55:49:29.5
00:13:11.54 +50:29:26.2
23:28:47.68 +55:42:05.1
23:47:00.89 +55:10:15.3
00:02:53.27 +56:47:56.8
23:35:05.74 +56:37:22.4
00:29:49.87 +57:44:24.4
23:56:52.73 +55:03:44.2
23:44:40.09 +53:04:18.5
23:18:39.20 +55:18:48.8
23:48:20.18 +55:11:05.3
00:11:00.58 +52:48:13.1
23:41:09.88 +57:06:07.9
23:45:45.38 +57:15:51.9
23:58:32.13 +54:07:42.3
00:15:25.71 +57:02:54.6
23:50:14.74 +56:24:08.4
23:41:22.47 +52:21:55.0
23:39:35.07 +55:18:05.3
23:38:03.17 +51:03:31.7
23:22:35.16 +54:22:00.3
23:23:41.19 +53:38:23.8
00:20:49.80 +52:35:26.1
23:16:52.09 +55:47:52.0
00:08:31.06 +56:46:19.6
23:19:36.82 +50:24:58.0
23:52:23.28 +51:58:06.5
23:37:44.85 +55:12:16.6
23:16:05.34 +55:19:44.4
23:16:22.00 +52:30:46.5
23:25:38.82 +57:34:19.1
23:19:22.56 +56:55:30.8
23:22:52.86 +52:08:27.7
00:11:44.19 +54:49:05.1
23:24:46.67 +54:41:49.8
00:25:44.00 +54:04:10.8
23:56:38.30 +56:24:23.5
23:50:35.75 +57:09:06.4
23:26:57.46 +54:34:29.6
00:25:08.26 +53:39:22.1
23:12:31.37 +56:31:47.0
23:20:45.99 +53:19:15.9
23:56:26.14 +56:13:16.2
23:37:15.03 +56:33:09.8
23:30:30.10 +54:53:43.2
23:31:57.48 +54:10:54.8
23:19:01.09 +54:18:02.6
23:56:58.11 +56:44:18.6
23:58:37.14 +53:54:47.1
23:45:57.02 +56:53:10.3
23:39:40.85 +57:15:46.7
23:28:30.79 +57:13:04.9
23:13:55.36 +55:22:07.2
23:19:18.68 +53:23:10.0
23:10:18.23 +56:52:14.2
23:11:54.60 +56:27:28.4
23:15:03.46 +56:00:09.2
23:21:30.45 +55:24:07.9
23:51:58.61 +53:09:19.2
23:14:33.63 +54:33:11.9
23:11:29.55 +56:00:28.5
23:16:16.91 +52:28:06.7
23:19:14.05 +56:28:30.4
23:22:04.37 +54:51:00.3
23:32:48.98 +53:52:50.1
23:27:48.73 +49:42:25.7
23:36:47.40 +50:45:10.4
23:21:13.25 +55:40:59.4
23:54:34.65 +57:28:04.2
00:22:57.69 +55:45:15.2
23:20:48.61 +53:19:00.9
23:43:55.17 +56:19:46.5
23:47:12.74 +57:25:28.7
23:22:45.78 +57:23:00.7
23:26:38.33 +53:47:40.3
23:23:26.68 +54:23:40.1
23:22:02.31 +55:43:41.1
23:32:49.01 +54:46:38.0
23:57:57.64 +50:30:08.3
23:57:54.05 +56:28:12.2
23:25:19.53 +55:06:28.9
23:30:23.41 +57:57:12.0
23:59:03.31 +53:35:20.6
00:27:08.86 +50:01:08.3
23:10:52.33 +57:01:38.7
00:13:35.65 +56:24:23.9
23:18:19.32 +53:13:24.1
00:12:55.37 +50:00:03.0
23:58:50.05 +54:41:49.5
00:07:09.81 +57:23:10.8
23:57:56.35 +50:30:59.5
00:20:02.82 +50:08:55.9
23:40:52.98 +57:50:35.7
23:56:31.15 +53:44:48.2
23:49:45.14 +56:38:12.3
00:24:49.00 +53:02:22.8
00:12:13.11 +50:41:18.4
23:24:03.95 +54:35:38.9
23:52:05.29 +50:10:17.3
23:29:40.53 +51:43:30.4
23:18:33.45 +49:57:07.7
23:43:23.69 +51:59:26.5
23:57:51.72 +56:29:02.3
23:12:11.66 +55:19:43.6
23:31:54.22 +55:26:00.4
00:07:56.66 +53:41:08.0
23:21:31.14 +55:55:32.2
00:13:58.31 +55:15:52.0
00:12:33.36 +57:13:41.7
23:12:32.05 +57:05:41.1
23:38:06.06 +50:59:35.0
23:32:47.26 +54:06:00.7
23:46:59.80 +57:24:39.0
23:45:14.10 +49:49:19.5
23:34:22.58 +51:39:22.8
23:30:03.04 +54:39:53.7
23:32:41.94 +58:04:45.8
00:20:13.49 +57:49:39.8
23:15:13.26 +52:54:41.3
23:58:56.41 +53:17:11.7
23:34:19.66 +54:04:14.6
23:49:55.13 +52:10:38.2
23:29:37.56 +50:43:08.5
23:36:04.26 +51:21:42.2
23:23:44.71 +53:48:00.6
00:03:25.85 +55:39:18.2
23:23:26.73 +57:10:13.4
00:19:39.43 +50:48:15.0
00:00:20.87 +56:49:48.3
00:08:13.12 +54:03:49.3
23:44:18.13 +57:20:24.7
00:02:25.22 +54:32:44.9
23:56:15.70 +56:09:37.5
23:20:45.16 +55:33:00.2
23:21:19.87 +55:56:11.3
23:47:39.62 +56:51:37.1
23:26:29.66 +55:06:24.3
23:58:56.00 +56:57:59.6
00:12:01.35 +53:36:40.1
23:50:58.54 +54:43:02.9
00:06:11.22 +51:25:18.4
23:28:42.42 +53:51:09.6
00:25:00.05 +52:51:11.0
00:00:52.63 +53:17:23.0
00:12:49.78 +55:50:22.8
23:42:23.25 +51:48:08.2
23:25:08.93 +54:30:24.1
00:09:58.09 +50:49:56.8
23:55:51.58 +54:53:32.4
23:43:20.49 +55:42:18.9
00:07:38.40 +57:11:00.6
23:26:45.28 +53:47:42.1
23:43:03.76 +52:46:21.9
00:14:46.44 +53:48:10.2
00:09:11.07 +57:36:12.5
23:15:23.66 +53:33:30.5
00:13:29.83 +56:53:48.5
23:48:00.94 +51:54:05.2
23:52:42.84 +55:29:51.2
23:34:08.47 +51:33:33.8
23:21:38.29 +50:06:23.1
########### 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 ####
23:44:32.67 +56:34:54.3
00:02:37.40 +55:49:29.5
00:13:11.54 +50:29:26.2
23:28:47.68 +55:42:05.1
23:47:00.89 +55:10:15.3
00:02:53.27 +56:47:56.8
23:35:05.74 +56:37:22.4
00:29:49.87 +57:44:24.4
23:56:52.73 +55:03:44.2
23:44:40.09 +53:04:18.5
23:18:39.20 +55:18:48.8
23:48:20.18 +55:11:05.3
00:11:00.58 +52:48:13.1
23:41:09.88 +57:06:07.9
23:45:45.38 +57:15:51.9
23:58:32.13 +54:07:42.3
00:15:25.71 +57:02:54.6
23:50:14.74 +56:24:08.4
23:41:22.47 +52:21:55.0
23:39:35.07 +55:18:05.3
23:38:03.17 +51:03:31.7
23:22:35.16 +54:22:00.3
23:23:41.19 +53:38:23.8
00:20:49.80 +52:35:26.1
23:16:52.09 +55:47:52.0
00:08:31.06 +56:46:19.6
23:19:36.82 +50:24:58.0
23:52:23.28 +51:58:06.5
23:37:44.85 +55:12:16.6
23:16:05.34 +55:19:44.4
23:16:22.00 +52:30:46.5
23:25:38.82 +57:34:19.1
23:19:22.56 +56:55:30.8
23:22:52.86 +52:08:27.7
00:11:44.19 +54:49:05.1
23:24:46.67 +54:41:49.8
00:25:44.00 +54:04:10.8
23:56:38.30 +56:24:23.5
23:50:35.75 +57:09:06.4
23:26:57.46 +54:34:29.6
00:25:08.26 +53:39:22.1
23:12:31.37 +56:31:47.0
23:20:45.99 +53:19:15.9
23:56:26.14 +56:13:16.2
23:37:15.03 +56:33:09.8
23:30:30.10 +54:53:43.2
23:31:57.48 +54:10:54.8
23:19:01.09 +54:18:02.6
23:56:58.11 +56:44:18.6
23:58:37.14 +53:54:47.1
23:45:57.02 +56:53:10.3
23:39:40.85 +57:15:46.7
23:28:30.79 +57:13:04.9
23:13:55.36 +55:22:07.2
23:19:18.68 +53:23:10.0
23:10:18.23 +56:52:14.2
23:11:54.60 +56:27:28.4
23:15:03.46 +56:00:09.2
23:21:30.45 +55:24:07.9
23:51:58.61 +53:09:19.2
23:14:33.63 +54:33:11.9
23:11:29.55 +56:00:28.5
23:16:16.91 +52:28:06.7
23:19:14.05 +56:28:30.4
23:22:04.37 +54:51:00.3
23:32:48.98 +53:52:50.1
23:27:48.73 +49:42:25.7
23:36:47.40 +50:45:10.4
23:21:13.25 +55:40:59.4
23:54:34.65 +57:28:04.2
00:22:57.69 +55:45:15.2
23:20:48.61 +53:19:00.9
23:43:55.17 +56:19:46.5
23:47:12.74 +57:25:28.7
23:22:45.78 +57:23:00.7
23:26:38.33 +53:47:40.3
23:23:26.68 +54:23:40.1
23:22:02.31 +55:43:41.1
23:32:49.01 +54:46:38.0
23:57:57.64 +50:30:08.3
23:57:54.05 +56:28:12.2
23:25:19.53 +55:06:28.9
23:30:23.41 +57:57:12.0
23:59:03.31 +53:35:20.6
00:27:08.86 +50:01:08.3
23:10:52.33 +57:01:38.7
00:13:35.65 +56:24:23.9
23:18:19.32 +53:13:24.1
00:12:55.37 +50:00:03.0
23:58:50.05 +54:41:49.5
00:07:09.81 +57:23:10.8
23:57:56.35 +50:30:59.5
00:20:02.82 +50:08:55.9
23:40:52.98 +57:50:35.7
23:56:31.15 +53:44:48.2
23:49:45.14 +56:38:12.3
00:24:49.00 +53:02:22.8
00:12:13.11 +50:41:18.4
23:24:03.95 +54:35:38.9
23:52:05.29 +50:10:17.3
23:29:40.53 +51:43:30.4
23:18:33.45 +49:57:07.7
23:43:23.69 +51:59:26.5
23:57:51.72 +56:29:02.3
23:12:11.66 +55:19:43.6
23:31:54.22 +55:26:00.4
00:07:56.66 +53:41:08.0
23:21:31.14 +55:55:32.2
00:13:58.31 +55:15:52.0
00:12:33.36 +57:13:41.7
23:12:32.05 +57:05:41.1
23:38:06.06 +50:59:35.0
23:32:47.26 +54:06:00.7
23:46:59.80 +57:24:39.0
23:45:14.10 +49:49:19.5
23:34:22.58 +51:39:22.8
23:30:03.04 +54:39:53.7
23:32:41.94 +58:04:45.8
00:20:13.49 +57:49:39.8
23:15:13.26 +52:54:41.3
23:58:56.41 +53:17:11.7
23:34:19.66 +54:04:14.6
23:49:55.13 +52:10:38.2
23:29:37.56 +50:43:08.5
23:36:04.26 +51:21:42.2
23:23:44.71 +53:48:00.6
00:03:25.85 +55:39:18.2
23:23:26.73 +57:10:13.4
00:19:39.43 +50:48:15.0
00:00:20.87 +56:49:48.3
00:08:13.12 +54:03:49.3
23:44:18.13 +57:20:24.7
00:02:25.22 +54:32:44.9
23:56:15.70 +56:09:37.5
23:20:45.16 +55:33:00.2
23:21:19.87 +55:56:11.3
23:47:39.62 +56:51:37.1
23:26:29.66 +55:06:24.3
23:58:56.00 +56:57:59.6
00:12:01.35 +53:36:40.1
23:50:58.54 +54:43:02.9
00:06:11.22 +51:25:18.4
23:28:42.42 +53:51:09.6
00:25:00.05 +52:51:11.0
00:00:52.63 +53:17:23.0
00:12:49.78 +55:50:22.8
23:42:23.25 +51:48:08.2
23:25:08.93 +54:30:24.1
00:09:58.09 +50:49:56.8
23:55:51.58 +54:53:32.4
23:43:20.49 +55:42:18.9
00:07:38.40 +57:11:00.6
23:26:45.28 +53:47:42.1
23:43:03.76 +52:46:21.9
00:14:46.44 +53:48:10.2
00:09:11.07 +57:36:12.5
23:15:23.66 +53:33:30.5
00:13:29.83 +56:53:48.5
23:48:00.94 +51:54:05.2
23:52:42.84 +55:29:51.2
23:34:08.47 +51:33:33.8
23:27:27.27 +53:55:25.9
23:59:52.81 +56:58:28.5
00:15:48.73 +57:32:19.4
23:21:38.29 +50:06:23.1
###################################################################################
23:44:32.67 +56:34:54.3 -- not an asteroid (will add it to exclusion list)
00:02:37.40 +55:49:29.5 -- not an asteroid (will add it to exclusion list)
00:13:11.54 +50:29:26.2 -- not an asteroid (will add it to exclusion list)
23:28:47.68 +55:42:05.1 -- not an asteroid (will add it to exclusion list)
23:47:00.89 +55:10:15.3 -- not an asteroid (will add it to exclusion list)
00:02:53.27 +56:47:56.8 -- not an asteroid (will add it to exclusion list)
23:35:05.74 +56:37:22.4 -- not an asteroid (will add it to exclusion list)
00:29:49.87 +57:44:24.4 -- not an asteroid (will add it to exclusion list)
23:56:52.73 +55:03:44.2 -- not an asteroid (will add it to exclusion list)
23:44:40.09 +53:04:18.5 -- not an asteroid (will add it to exclusion list)
23:18:39.20 +55:18:48.8 -- not an asteroid (will add it to exclusion list)
23:48:20.18 +55:11:05.3 -- not an asteroid (will add it to exclusion list)
00:11:00.58 +52:48:13.1 -- not an asteroid (will add it to exclusion list)
23:41:09.88 +57:06:07.9 -- not an asteroid (will add it to exclusion list)
23:45:45.38 +57:15:51.9 -- not an asteroid (will add it to exclusion list)
23:58:32.13 +54:07:42.3 -- not an asteroid (will add it to exclusion list)
00:15:25.71 +57:02:54.6 -- not an asteroid (will add it to exclusion list)
23:50:14.74 +56:24:08.4 -- not an asteroid (will add it to exclusion list)
23:41:22.47 +52:21:55.0 -- not an asteroid (will add it to exclusion list)
23:39:35.07 +55:18:05.3 -- not an asteroid (will add it to exclusion list)
23:38:03.17 +51:03:31.7 -- not an asteroid (will add it to exclusion list)
23:22:35.16 +54:22:00.3 -- not an asteroid (will add it to exclusion list)
23:23:41.19 +53:38:23.8 -- not an asteroid (will add it to exclusion list)
00:20:49.80 +52:35:26.1 -- not an asteroid (will add it to exclusion list)
23:16:52.09 +55:47:52.0 -- not an asteroid (will add it to exclusion list)
00:08:31.06 +56:46:19.6 -- not an asteroid (will add it to exclusion list)
23:19:36.82 +50:24:58.0 -- not an asteroid (will add it to exclusion list)
23:52:23.28 +51:58:06.5 -- not an asteroid (will add it to exclusion list)
23:37:44.85 +55:12:16.6 -- not an asteroid (will add it to exclusion list)
23:16:05.34 +55:19:44.4 -- not an asteroid (will add it to exclusion list)
23:16:22.00 +52:30:46.5 -- not an asteroid (will add it to exclusion list)
23:25:38.82 +57:34:19.1 -- not an asteroid (will add it to exclusion list)
23:19:22.56 +56:55:30.8 -- not an asteroid (will add it to exclusion list)
23:22:52.86 +52:08:27.7 -- not an asteroid (will add it to exclusion list)
00:11:44.19 +54:49:05.1 -- not an asteroid (will add it to exclusion list)
23:24:46.67 +54:41:49.8 -- not an asteroid (will add it to exclusion list)
00:25:44.00 +54:04:10.8 -- not an asteroid (will add it to exclusion list)
23:56:38.30 +56:24:23.5 -- not an asteroid (will add it to exclusion list)
23:50:35.75 +57:09:06.4 -- not an asteroid (will add it to exclusion list)
23:26:57.46 +54:34:29.6 -- not an asteroid (will add it to exclusion list)
00:25:08.26 +53:39:22.1 -- not an asteroid (will add it to exclusion list)
23:12:31.37 +56:31:47.0 -- not an asteroid (will add it to exclusion list)
23:20:45.99 +53:19:15.9 -- not an asteroid (will add it to exclusion list)
23:56:26.14 +56:13:16.2 -- not an asteroid (will add it to exclusion list)
23:37:15.03 +56:33:09.8 -- not an asteroid (will add it to exclusion list)
23:30:30.10 +54:53:43.2 -- not an asteroid (will add it to exclusion list)
23:31:57.48 +54:10:54.8 -- not an asteroid (will add it to exclusion list)
23:19:01.09 +54:18:02.6 -- not an asteroid (will add it to exclusion list)
23:56:58.11 +56:44:18.6 -- not an asteroid (will add it to exclusion list)
23:58:37.14 +53:54:47.1 -- not an asteroid (will add it to exclusion list)
23:45:57.02 +56:53:10.3 -- not an asteroid (will add it to exclusion list)
23:39:40.85 +57:15:46.7 -- not an asteroid (will add it to exclusion list)
23:28:30.79 +57:13:04.9 -- not an asteroid (will add it to exclusion list)
23:13:55.36 +55:22:07.2 -- not an asteroid (will add it to exclusion list)
23:19:18.68 +53:23:10.0 -- not an asteroid (will add it to exclusion list)
23:10:18.23 +56:52:14.2 -- not an asteroid (will add it to exclusion list)
23:11:54.60 +56:27:28.4 -- not an asteroid (will add it to exclusion list)
23:15:03.46 +56:00:09.2 -- not an asteroid (will add it to exclusion list)
23:21:30.45 +55:24:07.9 -- not an asteroid (will add it to exclusion list)
23:51:58.61 +53:09:19.2 -- not an asteroid (will add it to exclusion list)
23:14:33.63 +54:33:11.9 -- not an asteroid (will add it to exclusion list)
23:11:29.55 +56:00:28.5 -- not an asteroid (will add it to exclusion list)
23:16:16.91 +52:28:06.7 -- not an asteroid (will add it to exclusion list)
23:19:14.05 +56:28:30.4 -- not an asteroid (will add it to exclusion list)
23:22:04.37 +54:51:00.3 -- not an asteroid (will add it to exclusion list)
23:32:48.98 +53:52:50.1 -- not an asteroid (will add it to exclusion list)
23:27:48.73 +49:42:25.7 -- not an asteroid (will add it to exclusion list)
23:36:47.40 +50:45:10.4 -- not an asteroid (will add it to exclusion list)
23:21:13.25 +55:40:59.4 -- not an asteroid (will add it to exclusion list)
23:54:34.65 +57:28:04.2 -- not an asteroid (will add it to exclusion list)
00:22:57.69 +55:45:15.2 -- not an asteroid (will add it to exclusion list)
23:20:48.61 +53:19:00.9 -- not an asteroid (will add it to exclusion list)
23:43:55.17 +56:19:46.5 -- not an asteroid (will add it to exclusion list)
23:47:12.74 +57:25:28.7 -- not an asteroid (will add it to exclusion list)
23:22:45.78 +57:23:00.7 -- not an asteroid (will add it to exclusion list)
23:26:38.33 +53:47:40.3 -- not an asteroid (will add it to exclusion list)
23:23:26.68 +54:23:40.1 -- not an asteroid (will add it to exclusion list)
23:22:02.31 +55:43:41.1 -- not an asteroid (will add it to exclusion list)
23:32:49.01 +54:46:38.0 -- not an asteroid (will add it to exclusion list)
23:57:57.64 +50:30:08.3 -- not an asteroid (will add it to exclusion list)
23:57:54.05 +56:28:12.2 -- not an asteroid (will add it to exclusion list)
23:25:19.53 +55:06:28.9 -- not an asteroid (will add it to exclusion list)
23:30:23.41 +57:57:12.0 -- not an asteroid (will add it to exclusion list)
23:59:03.31 +53:35:20.6 -- not an asteroid (will add it to exclusion list)
00:27:08.86 +50:01:08.3 -- not an asteroid (will add it to exclusion list)
23:10:52.33 +57:01:38.7 -- not an asteroid (will add it to exclusion list)
00:13:35.65 +56:24:23.9 -- not an asteroid (will add it to exclusion list)
23:18:19.32 +53:13:24.1 -- not an asteroid (will add it to exclusion list)
00:12:55.37 +50:00:03.0 -- not an asteroid (will add it to exclusion list)
23:58:50.05 +54:41:49.5 -- not an asteroid (will add it to exclusion list)
00:07:09.81 +57:23:10.8 -- not an asteroid (will add it to exclusion list)
23:57:56.35 +50:30:59.5 -- not an asteroid (will add it to exclusion list)
00:20:02.82 +50:08:55.9 -- not an asteroid (will add it to exclusion list)
23:40:52.98 +57:50:35.7 -- not an asteroid (will add it to exclusion list)
23:56:31.15 +53:44:48.2 -- not an asteroid (will add it to exclusion list)
23:49:45.14 +56:38:12.3 -- not an asteroid (will add it to exclusion list)
00:24:49.00 +53:02:22.8 -- not an asteroid (will add it to exclusion list)
00:12:13.11 +50:41:18.4 -- not an asteroid (will add it to exclusion list)
23:24:03.95 +54:35:38.9 -- not an asteroid (will add it to exclusion list)
23:52:05.29 +50:10:17.3 -- not an asteroid (will add it to exclusion list)
23:29:40.53 +51:43:30.4 -- not an asteroid (will add it to exclusion list)
23:18:33.45 +49:57:07.7 -- not an asteroid (will add it to exclusion list)
23:43:23.69 +51:59:26.5 -- not an asteroid (will add it to exclusion list)
23:57:51.72 +56:29:02.3 -- not an asteroid (will add it to exclusion list)
23:12:11.66 +55:19:43.6 -- not an asteroid (will add it to exclusion list)
23:31:54.22 +55:26:00.4 -- not an asteroid (will add it to exclusion list)
00:07:56.66 +53:41:08.0 -- not an asteroid (will add it to exclusion list)
23:21:31.14 +55:55:32.2 -- not an asteroid (will add it to exclusion list)
00:13:58.31 +55:15:52.0 -- not an asteroid (will add it to exclusion list)
00:12:33.36 +57:13:41.7 -- not an asteroid (will add it to exclusion list)
23:12:32.05 +57:05:41.1 -- not an asteroid (will add it to exclusion list)
23:38:06.06 +50:59:35.0 -- not an asteroid (will add it to exclusion list)
23:32:47.26 +54:06:00.7 -- not an asteroid (will add it to exclusion list)
23:46:59.80 +57:24:39.0 -- not an asteroid (will add it to exclusion list)
23:45:14.10 +49:49:19.5 -- not an asteroid (will add it to exclusion list)
23:34:22.58 +51:39:22.8 -- not an asteroid (will add it to exclusion list)
23:30:03.04 +54:39:53.7 -- not an asteroid (will add it to exclusion list)
23:32:41.94 +58:04:45.8 -- not an asteroid (will add it to exclusion list)
00:20:13.49 +57:49:39.8 -- not an asteroid (will add it to exclusion list)
23:15:13.26 +52:54:41.3 -- not an asteroid (will add it to exclusion list)
23:58:56.41 +53:17:11.7 -- not an asteroid (will add it to exclusion list)
23:34:19.66 +54:04:14.6 -- not an asteroid (will add it to exclusion list)
23:49:55.13 +52:10:38.2 -- not an asteroid (will add it to exclusion list)
23:29:37.56 +50:43:08.5 -- not an asteroid (will add it to exclusion list)
23:36:04.26 +51:21:42.2 -- not an asteroid (will add it to exclusion list)
23:23:44.71 +53:48:00.6 -- not an asteroid (will add it to exclusion list)
00:03:25.85 +55:39:18.2 -- not an asteroid (will add it to exclusion list)
23:23:26.73 +57:10:13.4 -- not an asteroid (will add it to exclusion list)
00:19:39.43 +50:48:15.0 -- not an asteroid (will add it to exclusion list)
00:00:20.87 +56:49:48.3 -- not an asteroid (will add it to exclusion list)
00:08:13.12 +54:03:49.3 -- not an asteroid (will add it to exclusion list)
23:44:18.13 +57:20:24.7 -- not an asteroid (will add it to exclusion list)
00:02:25.22 +54:32:44.9 -- not an asteroid (will add it to exclusion list)
23:56:15.70 +56:09:37.5 -- not an asteroid (will add it to exclusion list)
23:20:45.16 +55:33:00.2 -- not an asteroid (will add it to exclusion list)
23:21:19.87 +55:56:11.3 -- not an asteroid (will add it to exclusion list)
23:47:39.62 +56:51:37.1 -- not an asteroid (will add it to exclusion list)
23:26:29.66 +55:06:24.3 -- not an asteroid (will add it to exclusion list)
23:58:56.00 +56:57:59.6 -- not an asteroid (will add it to exclusion list)
00:12:01.35 +53:36:40.1 -- not an asteroid (will add it to exclusion list)
23:50:58.54 +54:43:02.9 -- not an asteroid (will add it to exclusion list)
00:06:11.22 +51:25:18.4 -- not an asteroid (will add it to exclusion list)
23:28:42.42 +53:51:09.6 -- not an asteroid (will add it to exclusion list)
00:25:00.05 +52:51:11.0 -- not an asteroid (will add it to exclusion list)
00:00:52.63 +53:17:23.0 -- not an asteroid (will add it to exclusion list)
00:12:49.78 +55:50:22.8 -- not an asteroid (will add it to exclusion list)
23:42:23.25 +51:48:08.2 -- not an asteroid (will add it to exclusion list)
23:25:08.93 +54:30:24.1 -- not an asteroid (will add it to exclusion list)
00:09:58.09 +50:49:56.8 -- not an asteroid (will add it to exclusion list)
23:55:51.58 +54:53:32.4 -- not an asteroid (will add it to exclusion list)
23:43:20.49 +55:42:18.9 -- not an asteroid (will add it to exclusion list)
00:07:38.40 +57:11:00.6 -- not an asteroid (will add it to exclusion list)
23:26:45.28 +53:47:42.1 -- not an asteroid (will add it to exclusion list)
23:43:03.76 +52:46:21.9 -- not an asteroid (will add it to exclusion list)
00:14:46.44 +53:48:10.2 -- not an asteroid (will add it to exclusion list)
00:09:11.07 +57:36:12.5 -- not an asteroid (will add it to exclusion list)
23:15:23.66 +53:33:30.5 -- not an asteroid (will add it to exclusion list)
00:13:29.83 +56:53:48.5 -- not an asteroid (will add it to exclusion list)
23:48:00.94 +51:54:05.2 -- not an asteroid (will add it to exclusion list)
23:52:42.84 +55:29:51.2 -- not an asteroid (will add it to exclusion list)
23:34:08.47 +51:33:33.8 -- not an asteroid (will add it to exclusion list)
23:27:27.27 +53:55:25.9 -- not an asteroid (will add it to exclusion list)
23:59:52.81 +56:58:28.5 -- not an asteroid (will add it to exclusion list)
00:15:48.73 +57:32:19.4 -- not an asteroid (will add it to exclusion list)
23:21:38.29 +50:06:23.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:20.87 +56:49:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:00:52.63 +53:17:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:25.22 +54:32:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:37.40 +55:49:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:53.27 +56:47:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:25.85 +55:39:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:11.22 +51:25:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:09.81 +57:23:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:38.40 +57:11:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:56.66 +53:41:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:13.12 +54:03:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:31.06 +56:46:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:11.07 +57:36:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:58.09 +50:49:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:00.58 +52:48:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:44.19 +54:49:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:01.35 +53:36:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:13.11 +50:41:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:33.36 +57:13:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:49.78 +55:50:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:55.37 +50:00:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:11.54 +50:29:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:29.83 +56:53:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:35.65 +56:24:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:58.31 +55:15:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:46.44 +53:48:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:25.71 +57:02:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:48.73 +57:32:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:39.43 +50:48:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:02.82 +50:08:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:13.49 +57:49:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:49.80 +52:35:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:57.69 +55:45:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:49.00 +53:02:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:00.05 +52:51:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:08.26 +53:39:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:44.00 +54:04:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:08.86 +50:01:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:49.87 +57:44:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:18.23 +56:52:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:52.33 +57:01:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:29.55 +56:00:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:54.60 +56:27:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:11.66 +55:19:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:31.37 +56:31:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:32.05 +57:05:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:55.36 +55:22:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:33.63 +54:33:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:03.46 +56:00:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:13.26 +52:54:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:23.66 +53:33:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:05.34 +55:19:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:16.91 +52:28:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:22.00 +52:30:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:52.09 +55:47:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:19.32 +53:13:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:33.45 +49:57:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:39.20 +55:18:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:01.09 +54:18:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:14.05 +56:28:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:18.68 +53:23:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:22.56 +56:55:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:36.82 +50:24:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:45.16 +55:33:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:45.99 +53:19:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:48.61 +53:19:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:13.25 +55:40:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:19.87 +55:56:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:30.45 +55:24:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:31.14 +55:55:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:38.29 +50:06:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:02.31 +55:43:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:04.37 +54:51:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:35.16 +54:22:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:45.78 +57:23:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:52.86 +52:08:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:26.68 +54:23:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:26.73 +57:10:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:41.19 +53:38:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:44.71 +53:48:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:03.95 +54:35:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:46.67 +54:41:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:08.93 +54:30:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:19.53 +55:06:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:38.82 +57:34:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:29.66 +55:06:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:38.33 +53:47:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:45.28 +53:47:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:57.46 +54:34:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:27.27 +53:55:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:48.73 +49:42:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:30.79 +57:13:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:42.42 +53:51:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:47.68 +55:42:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:37.56 +50:43:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:40.53 +51:43:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:03.04 +54:39:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:23.41 +57:57:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:30.10 +54:53:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:54.22 +55:26:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:57.48 +54:10:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:41.94 +58:04:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:47.26 +54:06:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:48.98 +53:52:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:49.01 +54:46:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:08.47 +51:33:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:19.66 +54:04:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:22.58 +51:39:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:05.74 +56:37:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:04.26 +51:21:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:47.40 +50:45:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:15.03 +56:33:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:44.85 +55:12:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:03.17 +51:03:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:06.06 +50:59:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:35.07 +55:18:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:40.85 +57:15:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:52.98 +57:50:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:09.88 +57:06:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:22.47 +52:21:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:23.25 +51:48:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:03.76 +52:46:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:20.49 +55:42:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:23.69 +51:59:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:55.17 +56:19:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:18.13 +57:20:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:32.67 +56:34:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:40.09 +53:04:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:14.10 +49:49:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:45.38 +57:15:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:57.02 +56:53:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:59.80 +57:24:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:00.89 +55:10:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:12.74 +57:25:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:39.62 +56:51:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:00.94 +51:54:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:20.18 +55:11:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:45.14 +56:38:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:55.13 +52:10:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:14.74 +56:24:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:35.75 +57:09:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:58.54 +54:43:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:58.61 +53:09:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:05.29 +50:10:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:23.28 +51:58:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:42.84 +55:29:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:34.65 +57:28:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:51.58 +54:53:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:15.70 +56:09:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:26.14 +56:13:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:31.15 +53:44:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:38.30 +56:24:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:52.73 +55:03:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:58.11 +56:44:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:51.72 +56:29:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:54.05 +56:28:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:56.35 +50:30:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:57.64 +50:30:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:32.13 +54:07:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:37.14 +53:54:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:50.05 +54:41:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:56.00 +56:57:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:56.41 +53:17:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:03.31 +53:35:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:52.81 +56:58:28.5 -- 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)
00:00:20.87 +56:49:48.3 -- not a known variable star
00:00:52.63 +53:17:23.0 -- not a known variable star
00:02:25.22 +54:32:44.9 -- not a known variable star
00:02:37.40 +55:49:29.5 -- not a known variable star
00:02:53.27 +56:47:56.8 -- not a known variable star
00:03:25.85 +55:39:18.2 -- a known variable star
00:06:11.22 +51:25:18.4 -- not a known variable star
00:07:09.81 +57:23:10.8 -- not a known variable star
00:07:38.40 +57:11:00.6 -- not a known variable star
00:07:56.66 +53:41:08.0 -- a known variable star
00:08:13.12 +54:03:49.3 -- a known variable star
00:08:31.06 +56:46:19.6 -- not a known variable star
00:09:11.07 +57:36:12.5 -- not a known variable star
00:09:58.09 +50:49:56.8 -- not a known variable star
00:11:00.58 +52:48:13.1 -- a known variable star
00:11:44.19 +54:49:05.1 -- not a known variable star
00:12:01.35 +53:36:40.1 -- not a known variable star
00:12:13.11 +50:41:18.4 -- not a known variable star
00:12:33.36 +57:13:41.7 -- not a known variable star
00:12:49.78 +55:50:22.8 -- not a known variable star
00:12:55.37 +50:00:03.0 -- not a known variable star
00:13:11.54 +50:29:26.2 -- not a known variable star
00:13:29.83 +56:53:48.5 -- not a known variable star
00:13:35.65 +56:24:23.9 -- not a known variable star
00:13:58.31 +55:15:52.0 -- not a known variable star
00:14:46.44 +53:48:10.2 -- not a known variable star
00:15:25.71 +57:02:54.6 -- not a known variable star
00:15:48.73 +57:32:19.4 -- not a known variable star
00:19:39.43 +50:48:15.0 -- not a known variable star
00:20:02.82 +50:08:55.9 -- not a known variable star
00:20:13.49 +57:49:39.8 -- not a known variable star
00:20:49.80 +52:35:26.1 -- not a known variable star
00:22:57.69 +55:45:15.2 -- not a known variable star
00:24:49.00 +53:02:22.8 -- not a known variable star
00:25:00.05 +52:51:11.0 -- not a known variable star
00:25:08.26 +53:39:22.1 -- not a known variable star
00:25:44.00 +54:04:10.8 -- not a known variable star
00:27:08.86 +50:01:08.3 -- not a known variable star
00:29:49.87 +57:44:24.4 -- not a known variable star
23:10:18.23 +56:52:14.2 -- not a known variable star
23:10:52.33 +57:01:38.7 -- not a known variable star
23:11:29.55 +56:00:28.5 -- not a known variable star
23:11:54.60 +56:27:28.4 -- a known variable star
23:12:11.66 +55:19:43.6 -- not a known variable star
23:12:31.37 +56:31:47.0 -- a known variable star
23:12:32.05 +57:05:41.1 -- not a known variable star
23:13:55.36 +55:22:07.2 -- not a known variable star
23:14:33.63 +54:33:11.9 -- a known variable star
23:15:03.46 +56:00:09.2 -- not a known variable star
23:15:13.26 +52:54:41.3 -- not a known variable star
23:15:23.66 +53:33:30.5 -- not a known variable star
23:16:05.34 +55:19:44.4 -- a known variable star
23:16:16.91 +52:28:06.7 -- not a known variable star
23:16:22.00 +52:30:46.5 -- not a known variable star
23:16:52.09 +55:47:52.0 -- not a known variable star
23:18:19.32 +53:13:24.1 -- a known variable star
23:18:33.45 +49:57:07.7 -- not a known variable star
23:18:39.20 +55:18:48.8 -- not a known variable star
23:19:01.09 +54:18:02.6 -- a known variable star
23:19:14.05 +56:28:30.4 -- not a known variable star
23:19:18.68 +53:23:10.0 -- not a known variable star
23:19:22.56 +56:55:30.8 -- not a known variable star
23:19:36.82 +50:24:58.0 -- not a known variable star
23:20:45.16 +55:33:00.2 -- a known variable star
23:20:45.99 +53:19:15.9 -- not a known variable star
23:20:48.61 +53:19:00.9 -- not a known variable star
23:21:13.25 +55:40:59.4 -- not a known variable star
23:21:19.87 +55:56:11.3 -- not a known variable star
23:21:30.45 +55:24:07.9 -- not a known variable star
23:21:31.14 +55:55:32.2 -- not a known variable star
23:21:38.29 +50:06:23.1 -- not a known variable star
23:22:02.31 +55:43:41.1 -- not a known variable star
23:22:04.37 +54:51:00.3 -- not a known variable star
23:22:35.16 +54:22:00.3 -- not a known variable star
23:22:45.78 +57:23:00.7 -- not a known variable star
23:22:52.86 +52:08:27.7 -- not a known variable star
23:23:26.68 +54:23:40.1 -- not a known variable star
23:23:26.73 +57:10:13.4 -- a known variable star
23:23:41.19 +53:38:23.8 -- not a known variable star
23:23:44.71 +53:48:00.6 -- not a known variable star
23:24:03.95 +54:35:38.9 -- not a known variable star
23:24:46.67 +54:41:49.8 -- not a known variable star
23:25:08.93 +54:30:24.1 -- not a known variable star
23:25:19.53 +55:06:28.9 -- not a known variable star
23:25:38.82 +57:34:19.1 -- a known variable star
23:26:29.66 +55:06:24.3 -- not a known variable star
23:26:38.33 +53:47:40.3 -- not a known variable star
23:26:45.28 +53:47:42.1 -- not a known variable star
23:26:57.46 +54:34:29.6 -- not a known variable star
23:27:27.27 +53:55:25.9 -- not a known variable star
23:27:48.73 +49:42:25.7 -- not a known variable star
23:28:30.79 +57:13:04.9 -- a known variable star
23:28:42.42 +53:51:09.6 -- not a known variable star
23:28:47.68 +55:42:05.1 -- not a known variable star
23:29:37.56 +50:43:08.5 -- not a known variable star
23:29:40.53 +51:43:30.4 -- not a known variable star
23:30:03.04 +54:39:53.7 -- not a known variable star
23:30:23.41 +57:57:12.0 -- not a known variable star
23:30:30.10 +54:53:43.2 -- not a known variable star
23:31:54.22 +55:26:00.4 -- not a known variable star
23:31:57.48 +54:10:54.8 -- not a known variable star
23:32:41.94 +58:04:45.8 -- not a known variable star
23:32:47.26 +54:06:00.7 -- not a known variable star
23:32:48.98 +53:52:50.1 -- not a known variable star
23:32:49.01 +54:46:38.0 -- not a known variable star
23:34:08.47 +51:33:33.8 -- not a known variable star
23:34:19.66 +54:04:14.6 -- not a known variable star
23:34:22.58 +51:39:22.8 -- not a known variable star
23:35:05.74 +56:37:22.4 -- a known variable star
23:36:04.26 +51:21:42.2 -- not a known variable star
23:36:47.40 +50:45:10.4 -- not a known variable star
23:37:15.03 +56:33:09.8 -- not a known variable star
23:37:44.85 +55:12:16.6 -- not a known variable star
23:38:03.17 +51:03:31.7 -- not a known variable star
23:38:06.06 +50:59:35.0 -- not a known variable star
23:39:35.07 +55:18:05.3 -- not a known variable star
23:39:40.85 +57:15:46.7 -- not a known variable star
23:40:52.98 +57:50:35.7 -- not a known variable star
23:41:09.88 +57:06:07.9 -- not a known variable star
23:41:22.47 +52:21:55.0 -- not a known variable star
23:42:23.25 +51:48:08.2 -- not a known variable star
23:43:03.76 +52:46:21.9 -- not a known variable star
23:43:20.49 +55:42:18.9 -- not a known variable star
23:43:23.69 +51:59:26.5 -- not a known variable star
23:43:55.17 +56:19:46.5 -- a known variable star
23:44:18.13 +57:20:24.7 -- not a known variable star
23:44:32.67 +56:34:54.3 -- a known variable star
23:44:40.09 +53:04:18.5 -- not a known variable star
23:45:14.10 +49:49:19.5 -- not a known variable star
23:45:45.38 +57:15:51.9 -- a known variable star
23:45:57.02 +56:53:10.3 -- not a known variable star
23:46:59.80 +57:24:39.0 -- not a known variable star
23:47:00.89 +55:10:15.3 -- not a known variable star
23:47:12.74 +57:25:28.7 -- a known variable star
23:47:39.62 +56:51:37.1 -- not a known variable star
23:48:00.94 +51:54:05.2 -- not a known variable star
23:48:20.18 +55:11:05.3 -- not a known variable star
23:49:45.14 +56:38:12.3 -- not a known variable star
23:49:55.13 +52:10:38.2 -- not a known variable star
23:50:14.74 +56:24:08.4 -- not a known variable star
23:50:35.75 +57:09:06.4 -- not a known variable star
23:50:58.54 +54:43:02.9 -- a known variable star
23:51:58.61 +53:09:19.2 -- not a known variable star
23:52:05.29 +50:10:17.3 -- not a known variable star
23:52:23.28 +51:58:06.5 -- not a known variable star
23:52:42.84 +55:29:51.2 -- not a known variable star
23:54:34.65 +57:28:04.2 -- not a known variable star
23:55:51.58 +54:53:32.4 -- not a known variable star
23:56:15.70 +56:09:37.5 -- a known variable star
23:56:26.14 +56:13:16.2 -- not a known variable star
23:56:31.15 +53:44:48.2 -- not a known variable star
23:56:38.30 +56:24:23.5 -- not a known variable star
23:56:52.73 +55:03:44.2 -- not a known variable star
23:56:58.11 +56:44:18.6 -- not a known variable star
23:57:51.72 +56:29:02.3 -- not a known variable star
23:57:54.05 +56:28:12.2 -- not a known variable star
23:57:56.35 +50:30:59.5 -- not a known variable star
23:57:57.64 +50:30:08.3 -- not a known variable star
23:58:32.13 +54:07:42.3 -- not a known variable star
23:58:37.14 +53:54:47.1 -- not a known variable star
23:58:50.05 +54:41:49.5 -- a known variable star
23:58:56.00 +56:57:59.6 -- not a known variable star
23:58:56.41 +53:17:11.7 -- not a known variable star
23:59:03.31 +53:35:20.6 -- not a known variable star
23:59:52.81 +56:58:28.5 -- a known variable star
Found 142 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
165 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 165 (excluding asteroids and hot pixels, 142 new), not updating the exclusion list!
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Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461247.82942575 -observatory V36
07:08:32.78 +18:55:13.4 Mercury (1.4mag)
11:15:32.51 +05:15:06.0 Venus (-4.2mag)
05:11:28.58 +22:59:01.6 Mars (1.3mag)
08:31:14.75 +19:23:17.0 Jupiter (-1.8mag)
00:56:48.76 +03:21:40.3 Saturn (0.7mag)
04:09:59.93 +20:52:25.8 Uranus (5.8mag)
00:16:42.21 +00:17:42.8 Neptune (7.7mag)
20:29:23.53 -23:24:57.4 Pluto (14.4mag)
17:42:32.12 -28:41:12.1 Moon (-11.8mag)
-rw-r--r-- 1 apache apache 362 Jul 26 10:08 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461247.82942575:
08:31:21.83 +19:22:49.6 Io (6.0mag)
08:31:15.04 +19:23:15.9 Europa (6.3mag)
08:31:22.59 +19:22:42.6 Ganymede (5.5mag)
08:31:44.29 +19:21:19.2 Callisto (6.7mag)
08:29:07.85 +19:15:09.9 Himalia (15.7mag)
08:31:14.70 +19:23:18.3 Thebe (16.6mag)
08:28:31.77 +19:16:15.1 Elara (17.7mag)
08:35:11.32 +19:09:04.3 Pasiphae (17.9mag)
08:35:15.42 +19:30:57.9 Carme (19.0mag)
-rw-r--r-- 1 apache apache 365 Jul 26 10:11 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461247.82942575:
18:18:25.44 -28:32:57.1 JWST
16:30:12.51 +46:47:27.2 Chandra
04:20:16.70 +54:20:23.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 26 10:09 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461247.82942575 -observatory V36
02:58:01.18 +16:11:20.3 17.8mag P/1996 R2 (Lagerkvist)
18:07:12.00 -34:38:06.5 13.9mag P/2010 H2 (Vales)
06:41:29.53 -68:28:59.8 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:06:06.01 +32:44:03.3 17.7mag C/2017 K2 (PANSTARRS)
03:01:02.94 +29:44:19.8 16.2mag P/2021 N1 (ZTF)
22:48:47.53 +32:02:16.5 17.3mag C/2022 E2 (ATLAS)
06:30:08.18 +26:44:38.5 16.7mag C/2022 N2 (PANSTARRS)
10:09:44.17 +29:03:21.5 16.9mag C/2022 QE78 (ATLAS)
09:20:13.70 +05:13:37.0 17.9mag C/2022 R6 (PANSTARRS)
15:11:06.35 -11:49:31.9 17.8mag P/2023 B1 (PANSTARRS)
21:28:22.17 +67:07:07.9 17.9mag C/2023 H5 (Lemmon)
16:03:29.84 -11:42:08.2 14.1mag C/2023 R1 (PANSTARRS)
08:29:27.47 +66:38:14.9 18.0mag C/2024 A1 (ATLAS)
07:53:01.59 +30:46:03.0 15.0mag C/2024 E1 (Wierzchos)
15:09:57.74 +15:35:36.8 17.6mag C/2024 G6 (ATLAS)
19:20:07.81 +41:56:44.2 13.7mag C/2024 J3 (ATLAS)
21:28:49.79 +48:06:18.0 17.7mag C/2024 R4 (PANSTARRS)
05:04:16.20 -13:12:56.9 15.6mag C/2024 T5 (ATLAS)
06:47:12.56 +26:23:06.7 17.9mag C/2025 J1 (Borisov)
07:24:27.91 -14:30:26.3 17.2mag C/2025 R3 (PANSTARRS)
10:15:37.29 +21:39:48.7 17.5mag C/2025 V2 (Rankin)
12:51:07.53 +03:08:43.7 17.0mag C/2025 Y1 (ATLAS)
16:14:52.77 +78:49:05.3 17.1mag C/2026 A2 (Bok)
03:00:34.09 +45:50:55.5 16.9mag C/2026 B2 (Sun-Gao)
11:36:36.69 +07:01:00.6 17.1mag A/2026 E1
21:42:30.65 -21:36:34.0 6.9mag 10P/Tempel
11:21:33.83 -02:39:17.7 16.2mag 29P/Schwassmann-Wachmann
04:22:32.83 +31:12:57.2 17.9mag 47P/Ashbrook-Jackson
10:41:15.44 +08:51:29.1 17.1mag 63P/Wild
00:53:24.16 -05:06:46.6 15.5mag 65P/Gunn
05:05:39.65 +20:43:12.3 13.7mag 78P/Gehrels
02:45:53.88 +12:32:56.7 16.5mag 88P/Howell
07:21:34.22 +29:13:23.6 15.9mag 93P/Lovas
03:31:19.27 +11:56:26.9 18.0mag 112P/Urata-Niijima
05:13:37.11 +31:13:02.1 16.5mag 114P/Wiseman-Skiff
08:47:35.83 +28:40:24.2 15.1mag 123P/West-Hartley
11:18:25.28 -05:14:09.2 17.0mag 124P/Mrkos
05:17:01.07 +21:08:07.3 16.2mag 128P/Shoemaker-Holt
06:05:49.35 +19:24:47.6 17.8mag 131P/Mueller
08:07:55.12 +13:22:09.4 17.5mag 141P-D/Machholz
03:21:21.04 -19:51:26.9 16.9mag 161P/Hartley-IRAS
06:30:39.83 +36:40:49.6 15.6mag 162P/SidingSpring
17:55:41.74 +27:46:29.7 13.3mag 169P/NEAT
02:17:21.99 +09:00:50.8 17.6mag 220P/McNaught
16:36:41.13 -09:12:30.3 17.4mag 235P/LINEAR
20:32:04.24 -52:15:30.2 17.8mag 259P/Garradd
02:44:40.44 +19:29:53.9 15.5mag 260P/McNaught
06:26:04.20 +37:42:11.8 17.3mag 295P/LINEAR
15:07:22.81 +04:31:07.5 17.7mag 391P/Kowalski
08:49:05.80 +18:59:16.8 17.9mag 450P/LONEOS
08:16:28.62 +37:51:40.5 18.0mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Jul 26 10:08 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
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
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -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
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
-rw-r--r-- 1 apache apache 5.6K Jul 26 10:08 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:47.45 +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
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
-rw-r--r-- 1 apache apache 189K Jul 26 10:08 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
23:00:56.681 -02:58:01.46 AT 2026uav 2026-06-27.40 22.3003
21:41:28.556 -10:15:02.03 AT 2026uau 2026-06-27.33 22.5499
23:36:00.567 +03:08:40.99 AT 2026uat 2026-06-27.40 22.3861
22:51:17.819 -02:44:30.07 AT 2026uas 2026-06-27.43 23.6131
22:43:31.162 -13:04:19.53 AT 2026uar 2026-06-27.41 23.404
22:56:11.772 -15:33:00.49 AT 2026uaq 2026-06-27.41 22.9473
00:34:21.041 -43:24:58.27 AT 2026uap 2026-06-26.42 23.5619
18:13:13.910 +08:19:45.95 AT 2026uao 2026-07-12.25 19.6718
15:59:20.050 +31:57:53.76 AT 2026uan 2026-07-03.75 20.59
16:18:19.991 +31:46:16.25 AT 2026uam 2026-07-03.75 21.58
15:46:15.870 +52:34:46.97 AT 2026ual 2026-07-03.73 21.47
15:47:43.770 +56:00:26.98 AT 2026uak 2026-07-03.72 21.4
16:16:42.449 +22:13:18.43 AT 2026uaj 2026-07-03.68 20.61
23:55:42.693 +34:28:37.99 AT 2026uai 2026-07-02.77 20.43
14:33:38.730 +31:20:49.35 AT 2026uah 2026-06-30.67 21.31
16:20:08.450 +15:55:00.65 AT 2026uag 2026-06-24.78 21.81
23:49:07.700 +34:00:30.50 AT 2026uaf 2026-06-11.84 20.33
13:48:41.440 +00:58:56.34 AT 2026uae 2026-07-09.63 22.3
13:45:12.450 -01:04:07.83 AT 2026uad 2026-07-09.63 22.39
13:52:49.020 +01:35:09.64 AT 2026uac 2026-07-08.63 21.91
-rw-r--r-- 1 apache apache 88K Jul 26 10:08 tns_transients_list.txt
