This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.25 23:38:14.48 +50:25:54.0
111.18523 -10.76314 galactic And Second-epoch detections are separated by 8.8" and 6.6 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 | 23:38:14.48 +50:25:54.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:14.48 +50:25:54.0: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:14.48 +50:25:54.0: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 38 14.48 +50 25 54.0 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.17 00:19:20.29 +50:14:26.1
117.68863 -12.30408 galactic Cas Second-epoch detections are separated by 6.1" and 6.7 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 | 00:19:20.29 +50:14:26.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:19:20.29 +50:14:26.1: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:19:20.29 +50:14:26.1: 14.85 +/- 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 08 28.2058* 00 19 20.29 +50 14 26.1 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,2461280.7058,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 11.98 23:20:05.34 +55:44:17.8
110.26457 -4.87057 galactic Cas Second-epoch detections are separated by 3.2" and 6.4 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 | 23:20:05.34 +55:44:17.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:05.34 +55:44:17.8: 15.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:05.34 +55:44:17.8: 14.78 +/- 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 08 28.2058* 23 20 05.34 +55 44 17.8 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.12 23:35:14.99 +52:50:25.3
111.44042 -8.32311 galactic Cas Second-epoch detections are separated by 2.2" and 6.5 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 | 23:35:14.99 +52:50:25.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:14.99 +52:50:25.3: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:14.99 +52:50:25.3: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 35 14.99 +52 50 25.3 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.12,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 11.64 23:45:24.96 +54:18:51.5
113.31312 -7.31981 galactic Cas Second-epoch detections are separated by 6.0" and 6.5 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 | 23:45:24.96 +54:18:51.5 (user input) | T | P | (position from user input) J-Ks=1.138+/- (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:24.96 +54:18:51.5: 15.55 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:24.96 +54:18:51.5: 14.95 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.55 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 45 24.96 +54 18 51.5 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 10.48 23:21:42.49 +50:06:38.8
108.53276 -10.23555 galactic And Second-epoch detections are separated by 3.3" and 6.6 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 J350.4335+50.1053 | 23:21:42.49 +50:06:38.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:42.49 +50:06:38.8: 15.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:42.49 +50:06:38.8: 14.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 21 42.49 +50 06 38.8 10.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.4335+50.1053,2461280.7058,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.4335+50.1053 20260828.2058 10.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 11.29 23:54:34.26 +51:57:43.2
114.09451 -9.93130 galactic Cas Second-epoch detections are separated by 1.5" and 6.7 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 J358.6345+51.9707 | 23:54:34.26 +51:57:43.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:54:34.26 +51:57:43.2: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:54:34.26 +51:57:43.2: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 54 34.26 +51 57 43.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.6345+51.9707,2461280.7058,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.6345+51.9707 20260828.2058 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 11.47 23:34:54.38 +52:08:13.6
111.18044 -8.97980 galactic Cas Second-epoch detections are separated by 2.5" and 6.6 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 | 23:34:54.38 +52:08:13.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:54.38 +52:08:13.6: 13.67 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:54.38 +52:08:13.6: 13.90 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 08 28.2058* 23 34 54.38 +52 08 13.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,11.47,0.05,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 20260828.2058 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 11.63 00:00:07.97 +51:20:34.4
114.81845 -10.71883 galactic Cas Second-epoch detections are separated by 6.4" and 6.6 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 | 00:00:07.97 +51:20:34.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:00:07.97 +51:20:34.4: 14.49 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:00:07.97 +51:20:34.4: 14.92 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.49 +/- 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 08 28.2058* 00 00 07.97 +51 20 34.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 11.98 23:32:44.57 +53:36:12.5
111.30826 -7.48288 galactic Cas Second-epoch detections are separated by 3.9" and 6.5 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 J353.1680+53.6064 | 23:32:44.57 +53:36:12.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:44.57 +53:36:12.5: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:44.57 +53:36:12.5: 14.83 +/- 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 08 28.2058* 23 32 44.57 +53 36 12.5 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.1680+53.6064,2461280.7058,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.1680+53.6064 20260828.2058 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.18 00:25:49.42 +50:28:02.5
118.76681 -12.19713 galactic Cas Second-epoch detections are separated by 0.9" and 6.7 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 | 00:25:49.42 +50:28:02.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:25:49.42 +50:28:02.5: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:25:49.42 +50:28:02.5: 14.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 25 49.42 +50 28 02.5 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.12 23:35:43.98 +55:35:51.8
112.31914 -5.70633 galactic Cas Second-epoch detections are separated by 3.0" and 6.4 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 | 23:35:43.98 +55:35:51.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:43.98 +55:35:51.8: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:43.98 +55:35:51.8: 14.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 35 43.98 +55 35 51.8 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.12,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 12.19 23:28:15.89 +50:18:04.2
109.60265 -10.40561 galactic And Second-epoch detections are separated by 0.2" and 6.6 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 | 23:28:15.89 +50:18:04.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:15.89 +50:18:04.2: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:15.89 +50:18:04.2: 14.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 28 15.89 +50 18 04.2 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.17 23:22:07.42 +49:54:19.3
108.52454 -10.45139 galactic And Second-epoch detections are separated by 6.2" and 6.6 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 | 23:22:07.42 +49:54:19.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:07.42 +49:54:19.3: 15.11 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:07.42 +49:54:19.3: 14.73 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.11 +/- 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 08 28.2058* 23 22 07.42 +49 54 19.3 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.15 23:38:40.09 +56:54:44.7
113.08693 -4.56189 galactic Cas Second-epoch detections are separated by 2.9" and 6.4 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 J354.6470+56.9166 | 23:38:35.73 +56:54:39.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.755+/- (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:40.09 +56:54:44.7: 14.74 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:40.09 +56:54:44.7: 14.67 +/- 0.32 detection
Forced photometry reference-image weighted average: 14.72 +/- 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 08 28.2058* 23 38 40.09 +56 54 44.7 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.6470+56.9166,2461280.7058,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.6470+56.9166 20260828.2058 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.20 23:33:21.87 +54:04:28.5
111.53934 -7.06120 galactic Cas Second-epoch detections are separated by 2.0" and 6.5 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 | 23:33:21.87 +54:04:28.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:21.87 +54:04:28.5: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:21.87 +54:04:28.5: 14.78 +/- 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 08 28.2058* 23 33 21.87 +54 04 28.5 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.26 00:19:20.06 +55:37:10.4
118.37621 -6.96796 galactic Cas Second-epoch detections are separated by 6.6" and 6.6 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 421440749646517504 | 00:19:23.94 +55:37:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:19:20.06 +55:37:10.4: 15.10 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:19:20.06 +55:37:10.4: 14.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.10 +/- 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 08 28.2058* 00 19 20.06 +55 37 10.4 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
Gaia DR3 421440749646517504,2461280.7058,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 421440749646517504 20260828.2058 12.26CV 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 08 28.2058 2461280.7058 12.30 23:39:28.46 +51:28:27.3
111.67310 -9.81749 galactic Cas Second-epoch detections are separated by 4.4" and 6.6 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 | 23:39:28.46 +51:28:27.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:28.46 +51:28:27.3: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:28.46 +51:28:27.3: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 39 28.46 +51 28 27.3 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.29 23:33:12.21 +50:10:29.9
110.32575 -10.77209 galactic And Second-epoch detections are separated by 2.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.3199+50.1781 | 23:33:12.21 +50:10:29.9 (user input) | SINE (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:12.21 +50:10:29.9: 15.05 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:12.21 +50:10:29.9: 14.47 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.80 +/- 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 08 28.2058* 23 33 12.21 +50 10 29.9 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.3199+50.1781,2461280.7058,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J353.3199+50.1781 20260828.2058 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.32 23:25:03.71 +57:01:59.5
111.35260 -3.88395 galactic Cas Second-epoch detections are separated by 8.8" and 6.6 pix
The object was found in VSX20" Gaia DR3 1997332592068479616
Type: ROT
# Max. Min./Amp. JD0 Period
15.950 G 15.980 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:25:03.71 +57:01:59.5: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:25:03.71 +57:01:59.5: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 25 03.71 +57 01 59.5 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
Gaia DR3 1997332592068479616,2461280.7058,14.32,0.05,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
Gaia DR3 1997332592068479616 20260828.2058 14.32CV 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 08 28.2058 2461280.7058 14.38 23:33:53.29 +55:45:09.2
112.11498 -5.48200 galactic Cas Second-epoch detections are separated by 4.8" and 6.7 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 | 23:33:53.29 +55:45:09.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:53.29 +55:45:09.2: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:53.29 +55:45:09.2: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 33 53.29 +55 45 09.2 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,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.33 23:18:03.58 +55:43:10.1
109.98942 -4.78812 galactic Cas Second-epoch detections are separated by 1.5" and 5.9 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 | 23:18:03.58 +55:43:10.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:03.58 +55:43:10.1: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:03.58 +55:43:10.1: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 03.58 +55 43 10.1 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,2461280.7058,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.37 23:31:39.33 +56:24:27.2
112.01450 -4.76366 galactic Cas Second-epoch detections are separated by 4.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.8988+56.3983 | 23:31:39.33 +56:24:27.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:39.33 +56:24:27.2: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:39.33 +56:24:27.2: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 39.33 +56 24 27.2 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 J352.8988+56.3983,2461280.7058,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.8988+56.3983 20260828.2058 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.29 23:33:16.96 +55:43:28.3
112.02487 -5.48337 galactic Cas Second-epoch detections are separated by 3.0" and 6.5 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 | 23:33:16.96 +55:43:28.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:16.96 +55:43:28.3: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:16.96 +55:43:28.3: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 33 16.96 +55 43 28.3 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.28 23:25:14.02 +55:36:09.2
110.90402 -5.24312 galactic Cas Second-epoch detections are separated by 7.6" and 6.2 pix
The object was found in VSX16" Gaia DR3 1996960888417419136
Type: ROT
# Max. Min./Amp. JD0 Period
15.450 G 15.490 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:25:14.02 +55:36:09.2: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:25:14.02 +55:36:09.2: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 25 14.02 +55 36 09.2 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
Gaia DR3 1996960888417419136,2461280.7058,14.28,0.05,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
Gaia DR3 1996960888417419136 20260828.2058 14.28CV 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 08 28.2058 2461280.7058 14.40 00:04:10.84 +53:29:33.7
115.85322 -8.72830 galactic Cas Second-epoch detections are separated by 7.0" and 6.4 pix
The object was found in VSX19" Gaia DR3 396210050163206016
Type: ROT
# Max. Min./Amp. JD0 Period
14.600 G 14.640 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:04:10.84 +53:29:33.7: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:04:10.84 +53:29:33.7: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 04 10.84 +53 29 33.7 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 396210050163206016,2461280.7058,14.40,0.05,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 396210050163206016 20260828.2058 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 08 28.2058 2461280.7058 14.29 23:11:16.06 +56:36:21.6
109.43213 -3.61729 galactic Cas Second-epoch detections are separated by 2.6" and 6.1 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 | 23:11:16.06 +56:36:21.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:11:16.06 +56:36:21.6: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:11:16.06 +56:36:21.6: 14.72 +/- 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 08 28.2058* 23 11 16.06 +56 36 21.6 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,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.48 23:25:35.82 +57:55:06.6
111.71089 -3.07090 galactic Cas Second-epoch detections are separated by 6.8" and 6.4 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 | 23:25:35.82 +57:55:06.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:25:35.82 +57:55:06.6: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:25:35.82 +57:55:06.6: 14.92 +/- 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 08 28.2058* 23 25 35.82 +57 55 06.6 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
target,2461280.7058,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.35 23:34:32.46 +54:30:26.4
111.83404 -6.69906 galactic Cas Second-epoch detections are separated by 5.4" and 6.4 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 | 23:34:32.46 +54:30:26.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:32.46 +54:30:26.4: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:32.46 +54:30:26.4: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 32.46 +54 30 26.4 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,2461280.7058,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.40 23:37:31.07 +54:37:57.2
112.28633 -6.70413 galactic Cas Second-epoch detections are separated by 1.8" and 6.6 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 | 23:37:31.07 +54:37:57.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:31.07 +54:37:57.2: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:31.07 +54:37:57.2: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 37 31.07 +54 37 57.2 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,2461280.7058,14.40,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.44 23:23:31.78 +55:24:15.3
110.60941 -5.35026 galactic Cas Second-epoch detections are separated by 8.1" and 6.8 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 | 23:23:31.78 +55:24:15.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:31.78 +55:24:15.3: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:31.78 +55:24:15.3: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 31.78 +55 24 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
target,2461280.7058,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.44CV 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 08 28.2058 2461280.7058 14.32 23:18:53.90 +53:45:26.0
109.40717 -6.66680 galactic Cas Second-epoch detections are separated by 5.8" and 6.5 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 | 23:18:53.90 +53:45:26.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:53.90 +53:45:26.0: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:53.90 +53:45:26.0: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 53.90 +53 45 26.0 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,2461280.7058,14.32,0.05,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
target 20260828.2058 14.32CV 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 08 28.2058 2461280.7058 14.45 23:20:39.97 +55:09:31.8
110.14049 -5.44257 galactic Cas Second-epoch detections are separated by 8.2" and 6.7 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 | 23:20:39.97 +55:09:31.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:39.97 +55:09:31.8: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:39.97 +55:09:31.8: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 20 39.97 +55 09 31.8 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
target,2461280.7058,14.45,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.44 00:23:24.29 +54:04:50.0
118.78089 -8.56510 galactic Cas Second-epoch detections are separated by 8.1" and 6.5 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 | 00:23:24.29 +54:04:50.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:23:24.29 +54:04:50.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:23:24.29 +54:04:50.0: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 23 24.29 +54 04 50.0 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,2461280.7058,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.44CV 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 08 28.2058 2461280.7058 14.38 23:42:03.14 +51:28:48.3
112.06655 -9.92194 galactic Cas Second-epoch detections are separated by 5.5" and 6.2 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 | 23:42:03.14 +51:28:48.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:03.14 +51:28:48.3: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:03.14 +51:28:48.3: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 42 03.14 +51 28 48.3 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
target,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.35 23:10:28.92 +57:11:08.3
109.55258 -3.04020 galactic Cas Second-epoch detections are separated by 7.5" and 6.7 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 | 23:10:28.92 +57:11:08.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:10:28.92 +57:11:08.3: 15.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:10:28.92 +57:11:08.3: 14.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 10 28.92 +57 11 08.3 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.56 23:10:29.21 +57:13:04.4
109.56546 -3.01062 galactic Cas Second-epoch detections are separated by 7.7" and 6.0 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 | 23:10:29.21 +57:13:04.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:10:29.21 +57:13:04.4: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:10:29.21 +57:13:04.4: 14.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 10 29.21 +57 13 04.4 14.6 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,2461280.7058,14.56,0.05,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 20260828.2058 14.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.38 23:26:30.09 +51:45:22.5
109.81443 -8.93914 galactic Cas Second-epoch detections are separated by 8.9" and 6.5 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 | 23:26:30.09 +51:45:22.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:30.09 +51:45:22.5: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:30.09 +51:45:22.5: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 26 30.09 +51 45 22.5 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,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.37 23:28:37.29 +56:49:15.5
111.74505 -4.24120 galactic Cas Second-epoch detections are separated by 7.1" and 6.4 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 | 23:28:37.29 +56:49:15.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:37.29 +56:49:15.5: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:37.29 +56:49:15.5: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 28 37.29 +56 49 15.5 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,2461280.7058,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.34 23:47:45.19 +49:57:10.9
112.55060 -11.63068 galactic Cas Second-epoch detections are separated by 6.8" and 6.4 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 | 23:47:45.19 +49:57:10.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:47:45.19 +49:57:10.9: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:47:45.19 +49:57:10.9: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 47 45.19 +49 57 10.9 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.32 23:48:36.95 +50:34:52.5
112.84533 -11.05608 galactic Cas Second-epoch detections are separated by 3.9" and 6.5 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 | 23:48:36.95 +50:34:52.5 (user input) | T | P | (position from user input) SpType: A9V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:36.95 +50:34:52.5: 15.23 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:36.95 +50:34:52.5: 15.05 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.23 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 48 36.95 +50 34 52.5 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,2461280.7058,14.32,0.05,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
target 20260828.2058 14.32CV 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 08 28.2058 2461280.7058 14.48 00:09:23.43 +51:02:03.8
116.21347 -11.28804 galactic Cas Second-epoch detections are separated by 6.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:09:23.43 +51:02:03.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:23.43 +51:02:03.8: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:23.43 +51:02:03.8: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 09 23.43 +51 02 03.8 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
target,2461280.7058,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.31 23:30:35.12 +53:14:45.6
110.88914 -7.72474 galactic Cas Second-epoch detections are separated by 7.2" and 6.4 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 | 23:30:35.12 +53:14:45.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:35.12 +53:14:45.6: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:35.12 +53:14:45.6: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 35.12 +53 14 45.6 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,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.34 23:11:28.21 +56:37:54.0
109.46767 -3.60402 galactic Cas Second-epoch detections are separated by 3.0" and 6.4 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 | 23:11:28.21 +56:37:54.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:11:28.21 +56:37:54.0: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:11:28.21 +56:37:54.0: 14.83 +/- 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 08 28.2058* 23 11 28.21 +56 37 54.0 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,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.29 23:28:24.32 +51:59:26.8
110.17254 -8.81201 galactic Cas Second-epoch detections are separated by 5.4" and 6.3 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 | 23:28:24.32 +51:59:26.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:24.32 +51:59:26.8: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:24.32 +51:59:26.8: 14.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 28 24.32 +51 59 26.8 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,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.33 23:36:27.75 +57:32:22.4
112.97760 -3.87595 galactic Cas Second-epoch detections are separated by 8.9" and 6.8 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 | 23:36:27.75 +57:32:22.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:27.75 +57:32:22.4: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:27.75 +57:32:22.4: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 36 27.75 +57 32 22.4 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,2461280.7058,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.34 23:19:26.47 +50:59:21.6
108.50117 -9.28657 galactic And Second-epoch detections are separated by 5.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:19:26.47 +50:59:21.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:26.47 +50:59:21.6: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:26.47 +50:59:21.6: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 26.47 +50 59 21.6 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.41 00:10:51.20 +52:25:07.5
116.66958 -9.95883 galactic Cas Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J002.7064+52.4082 | 00:10:51.20 +52:25:07.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:10:51.20 +52:25:07.5: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:10:51.20 +52:25:07.5: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 10 51.20 +52 25 07.5 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 J002.7064+52.4082,2461280.7058,14.41,0.05,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
ATO J002.7064+52.4082 20260828.2058 14.41CV 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 08 28.2058 2461280.7058 14.29 23:37:04.13 +54:30:54.1
112.18981 -6.79825 galactic Cas Second-epoch detections are separated by 5.2" and 6.5 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 J354.2619+54.5153 | 23:37:04.13 +54:30:54.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:04.13 +54:30:54.1: 15.20 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:04.13 +54:30:54.1: 14.99 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.20 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 37 04.13 +54 30 54.1 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 J354.2619+54.5153,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.2619+54.5153 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.41 00:13:26.58 +53:19:41.1
117.20307 -9.12051 galactic Cas Second-epoch detections are separated by 6.1" and 6.8 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 | 00:13:26.58 +53:19:41.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:13:26.58 +53:19:41.1: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:13:26.58 +53:19:41.1: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 13 26.58 +53 19 41.1 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,2461280.7058,14.41,0.05,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 20260828.2058 14.41CV 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 08 28.2058 2461280.7058 14.26 23:24:25.61 +53:57:00.3
110.24493 -6.76450 galactic Cas Second-epoch detections are separated by 5.4" and 6.6 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 | 23:24:25.61 +53:57:00.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:25.61 +53:57:00.3: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:25.61 +53:57:00.3: 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 08 28.2058* 23 24 25.61 +53 57 00.3 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.26,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.38 00:12:38.00 +53:52:11.1
117.16523 -8.56695 galactic Cas Second-epoch detections are separated by 3.7" and 6.7 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 | 00:12:38.00 +53:52:11.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:12:38.00 +53:52:11.1: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:12:38.00 +53:52:11.1: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 12 38.00 +53 52 11.1 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,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.32 23:15:04.32 +55:33:55.7
109.53914 -4.78041 galactic Cas Second-epoch detections are separated by 3.1" and 6.6 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 | 23:15:04.32 +55:33:55.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:04.32 +55:33:55.7: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:04.32 +55:33:55.7: 14.81 +/- 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 08 28.2058* 23 15 04.32 +55 33 55.7 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,2461280.7058,14.32,0.05,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
target 20260828.2058 14.32CV 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 08 28.2058 2461280.7058 14.38 23:17:29.14 +51:35:32.9
108.42899 -8.61414 galactic And Second-epoch detections are separated by 6.9" and 6.5 pix
The object was found in VSX22" Gaia DR3 1991974362666372096
Type: VAR
# Max. Min./Amp. JD0 Period
16.790 G 17.070 G 0.080158100000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:29.14 +51:35:32.9: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:29.14 +51:35:32.9: 14.80 +/- 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 08 28.2058* 23 17 29.14 +51 35 32.9 14.4 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
Gaia DR3 1991974362666372096,2461280.7058,14.38,0.05,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 1991974362666372096 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.27 23:31:42.78 +55:31:56.5
111.75438 -5.59967 galactic Cas Second-epoch detections are separated by 5.3" and 6.3 pix
The object was found in VSX22" Gaia DR3 1997642963584321920
Type: RS
# Max. Min./Amp. JD0 Period
16.320 G 16.390 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:42.78 +55:31:56.5: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:42.78 +55:31:56.5: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 42.78 +55 31 56.5 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
Gaia DR3 1997642963584321920,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997642963584321920 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.20 23:18:24.24 +53:43:23.0
109.32617 -6.67297 galactic Cas Second-epoch detections are separated by 5.1" and 6.3 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 | 23:18:24.24 +53:43:23.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:24.24 +53:43:23.0: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:24.24 +53:43:23.0: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 24.24 +53 43 23.0 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.20,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.39 23:53:22.44 +53:30:17.8
114.26521 -8.38692 galactic Cas Second-epoch detections are separated by 8.9" and 6.3 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 J358.3470+53.5147 | 23:53:22.44 +53:30:17.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:53:22.44 +53:30:17.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:53:22.44 +53:30:17.8: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 53 22.44 +53 30 17.8 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
ATO J358.3470+53.5147,2461280.7058,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.3470+53.5147 20260828.2058 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.29 00:12:29.83 +53:38:35.5
117.11028 -8.78781 galactic Cas Second-epoch detections are separated by 1.9" and 6.5 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 | 00:12:29.83 +53:38:35.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:12:29.83 +53:38:35.5: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:12:29.83 +53:38:35.5: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 12 29.83 +53 38 35.5 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,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.34 00:10:19.86 +50:21:11.1
116.24944 -11.98454 galactic Cas Second-epoch detections are separated by 7.1" and 6.6 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 | 00:10:19.86 +50:21:11.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:10:19.86 +50:21:11.1: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:10:19.86 +50:21:11.1: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 10 19.86 +50 21 11.1 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,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.38 00:00:01.36 +53:01:37.5
115.14492 -9.06554 galactic Cas Second-epoch detections are separated by 5.0" and 6.6 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 1945197598964125696 | 23:59:57.91 +53:01:13.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:00:01.36 +53:01:37.5: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:00:01.36 +53:01:37.5: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 00 01.36 +53 01 37.5 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 1945197598964125696,2461280.7058,14.38,0.05,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 1945197598964125696 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.31 00:12:07.85 +52:25:18.0
116.86537 -9.98647 galactic Cas Second-epoch detections are separated by 6.7" and 6.7 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 | 00:12:07.85 +52:25:18.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:12:07.85 +52:25:18.0: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:12:07.85 +52:25:18.0: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 12 07.85 +52 25 18.0 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,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.27 23:51:27.72 +54:14:05.2
114.15685 -7.61195 galactic Cas Second-epoch detections are separated by 5.7" and 6.5 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 J357.8662+54.2451 | 23:51:27.72 +54:14:05.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:51:27.72 +54:14:05.2: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:51:27.72 +54:14:05.2: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 51 27.72 +54 14 05.2 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 J357.8662+54.2451,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.8662+54.2451 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.47 23:24:52.09 +54:41:49.4
110.55493 -6.08097 galactic Cas Second-epoch detections are separated by 4.1" and 6.5 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 | 23:24:52.09 +54:41:49.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:52.09 +54:41:49.4: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:52.09 +54:41:49.4: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 24 52.09 +54 41 49.4 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
target,2461280.7058,14.47,0.05,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 20260828.2058 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.28 00:16:21.72 +53:48:42.7
117.70724 -8.70369 galactic Cas Second-epoch detections are separated by 6.8" and 6.8 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 | 00:16:21.72 +53:48:42.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:16:21.72 +53:48:42.7: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:16:21.72 +53:48:42.7: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 16 21.72 +53 48 42.7 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,2461280.7058,14.28,0.05,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 20260828.2058 14.28CV 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 08 28.2058 2461280.7058 14.28 00:07:27.60 +51:29:05.2
115.98782 -10.79305 galactic Cas Second-epoch detections are separated by 1.7" and 6.6 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 | 00:07:27.60 +51:29:05.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:27.60 +51:29:05.2: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:27.60 +51:29:05.2: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 07 27.60 +51 29 05.2 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,2461280.7058,14.28,0.05,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 20260828.2058 14.28CV 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 08 28.2058 2461280.7058 14.31 00:11:38.66 +54:02:13.9
117.04587 -8.37915 galactic Cas Second-epoch detections are separated by 4.3" and 6.3 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 | 00:11:38.66 +54:02:13.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:11:38.66 +54:02:13.9: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:11:38.66 +54:02:13.9: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 11 38.66 +54 02 13.9 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.22 23:28:01.21 +55:38:38.0
111.29125 -5.33116 galactic Cas Second-epoch detections are separated by 3.0" and 6.5 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 | 23:28:01.21 +55:38:38.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:01.21 +55:38:38.0: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:01.21 +55:38:38.0: 14.85 +/- 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 08 28.2058* 23 28 01.21 +55 38 38.0 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.16 23:11:20.95 +56:24:15.5
109.36629 -3.80831 galactic Cas Second-epoch detections are separated by 4.3" and 6.4 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 | 23:11:20.95 +56:24:15.5 (user input) | T | P | (position from user input) J-Ks=-0.289+/- (O)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:11:20.95 +56:24:15.5: 15.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:11:20.95 +56:24:15.5: 14.80 +/- 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 08 28.2058* 23 11 20.95 +56 24 15.5 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.16,0.05,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 20260828.2058 14.16CV 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 08 28.2058 2461280.7058 14.24 23:23:47.98 +53:18:18.4
109.93987 -7.34154 galactic Cas Second-epoch detections are separated by 7.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:23:47.98 +53:18:18.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:47.98 +53:18:18.4: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:47.98 +53:18:18.4: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 47.98 +53 18 18.4 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.27 00:07:09.76 +50:30:14.6
115.76718 -11.75074 galactic Cas Second-epoch detections are separated by 1.2" and 6.5 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 | 00:07:09.76 +50:30:14.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:09.76 +50:30:14.6: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:09.76 +50:30:14.6: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 07 09.76 +50 30 14.6 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,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.36 23:38:01.96 +57:01:56.2
113.03719 -4.42258 galactic Cas Second-epoch detections are separated by 5.3" and 6.6 pix
The object was found in VSX15" Gaia DR3 1998627782406015744
Type: RS
# Max. Min./Amp. JD0 Period
17.090 G 17.190 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:01.96 +57:01:56.2: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:01.96 +57:01:56.2: 14.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 38 01.96 +57 01 56.2 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 1998627782406015744,2461280.7058,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998627782406015744 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.37 23:09:04.86 +57:24:42.0
109.46407 -2.75899 galactic Cas Second-epoch detections are separated by 5.2" and 6.7 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 | 23:09:04.86 +57:24:42.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:09:04.86 +57:24:42.0: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:09:04.86 +57:24:42.0: 14.75 +/- 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 08 28.2058* 23 09 04.86 +57 24 42.0 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,2461280.7058,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.19 23:23:36.32 +52:43:39.9
109.71673 -7.87565 galactic And Second-epoch detections are separated by 7.9" and 6.5 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 | 23:23:36.32 +52:43:39.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:36.32 +52:43:39.9: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:36.32 +52:43:39.9: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 36.32 +52 43 39.9 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.19,0.05,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 20260828.2058 14.19CV 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 08 28.2058 2461280.7058 14.20 23:21:26.05 +51:16:44.1
108.90031 -9.12417 galactic And Second-epoch detections are separated by 7.7" and 6.5 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 1991518370278012544 | 23:21:27.38 +51:17:26.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:26.05 +51:16:44.1: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:26.05 +51:16:44.1: 14.78 +/- 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 08 28.2058* 23 21 26.05 +51 16 44.1 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991518370278012544,2461280.7058,14.20,0.05,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
Gaia DR3 1991518370278012544 20260828.2058 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 08 28.2058 2461280.7058 14.22 23:35:59.42 +51:23:05.6
111.11909 -9.74811 galactic Cas Second-epoch detections are separated by 6.8" and 6.6 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 | 23:35:59.42 +51:23:05.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:59.42 +51:23:05.6: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:59.42 +51:23:05.6: 15.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 35 59.42 +51 23 05.6 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.20 23:29:05.04 +55:58:56.1
111.54104 -5.05741 galactic Cas Second-epoch detections are separated by 7.5" and 6.2 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 | 23:29:05.04 +55:58:56.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:05.04 +55:58:56.1: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:29:05.04 +55:58:56.1: 14.92 +/- 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 08 28.2058* 23 29 05.04 +55 58 56.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.20,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.19 00:13:29.41 +53:19:49.2
117.21046 -9.11933 galactic Cas Second-epoch detections are separated by 3.1" and 6.8 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 | 00:13:29.41 +53:19:49.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:13:29.41 +53:19:49.2: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:13:29.41 +53:19:49.2: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 13 29.41 +53 19 49.2 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.19,0.05,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 20260828.2058 14.19CV 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 08 28.2058 2461280.7058 14.30 23:15:34.34 +55:01:27.8
109.40812 -5.31032 galactic Cas Second-epoch detections are separated by 7.9" and 6.3 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 | 23:15:34.34 +55:01:27.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:34.34 +55:01:27.8: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:34.34 +55:01:27.8: 14.76 +/- 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 08 28.2058* 23 15 34.34 +55 01 27.8 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,2461280.7058,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.39 23:52:55.59 +53:55:19.6
114.29539 -7.96559 galactic Cas Second-epoch detections are separated by 4.6" and 6.7 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 | 23:52:55.59 +53:55:19.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:52:55.59 +53:55:19.6: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:52:55.59 +53:55:19.6: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 52 55.59 +53 55 19.6 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,2461280.7058,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.32 23:43:57.22 +51:35:21.9
112.38541 -9.89512 galactic Cas Second-epoch detections are separated by 5.0" and 6.4 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 | 23:43:57.22 +51:35:21.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:43:57.22 +51:35:21.9: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:43:57.22 +51:35:21.9: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 43 57.22 +51 35 21.9 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.32,0.05,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
target 20260828.2058 14.32CV 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 08 28.2058 2461280.7058 14.27 23:46:45.03 +50:07:53.8
112.43733 -11.41740 galactic Cas Second-epoch detections are separated by 7.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:46:45.03 +50:07:53.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:46:45.03 +50:07:53.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:46:45.03 +50:07:53.8: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 46 45.03 +50 07 53.8 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,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.30 23:32:52.30 +53:44:57.6
111.37101 -7.34958 galactic Cas Second-epoch detections are separated by 5.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.2058+53.7612 | 23:32:51.39 +53:45:34.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:52.30 +53:44:57.6: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:52.30 +53:44:57.6: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 32 52.30 +53 44 57.6 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 J353.2058+53.7612,2461280.7058,14.30,0.05,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 J353.2058+53.7612 20260828.2058 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.29 00:25:07.42 +56:25:13.5
119.27705 -6.26448 galactic Cas Second-epoch detections are separated by 5.8" and 6.1 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 | 00:25:07.42 +56:25:13.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:25:07.42 +56:25:13.5: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:25:07.42 +56:25:13.5: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 25 07.42 +56 25 13.5 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,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.36 23:41:50.24 +55:02:54.1
113.00351 -6.47609 galactic Cas Second-epoch detections are separated by 6.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J355.4521+55.0501 | 23:41:50.24 +55:02:54.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:41:50.24 +55:02:54.1: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:41:50.24 +55:02:54.1: 15.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 41 50.24 +55 02 54.1 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
ATO J355.4521+55.0501,2461280.7058,14.36,0.05,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 J355.4521+55.0501 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.30 23:42:42.37 +53:38:55.8
112.75039 -7.85871 galactic Cas Second-epoch detections are separated by 2.3" and 6.4 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 | 23:42:42.37 +53:38:55.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:42.37 +53:38:55.8: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:42.37 +53:38:55.8: 15.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 42 42.37 +53 38 55.8 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,2461280.7058,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.36 23:34:22.88 +52:49:51.6
111.31098 -8.29335 galactic Cas Second-epoch detections are separated by 7.4" and 6.4 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 | 23:34:22.88 +52:49:51.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:22.88 +52:49:51.6: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:22.88 +52:49:51.6: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 22.88 +52 49 51.6 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,2461280.7058,14.36,0.05,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 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.36 23:46:00.08 +52:44:54.5
112.99588 -8.85628 galactic Cas Second-epoch detections are separated by 6.1" and 6.7 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 | 23:46:00.08 +52:44:54.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:46:00.08 +52:44:54.5: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:46:00.08 +52:44:54.5: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 46 00.08 +52 44 54.5 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,2461280.7058,14.36,0.05,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 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.27 23:26:47.97 +57:24:35.9
111.69824 -3.60410 galactic Cas Second-epoch detections are separated by 3.7" and 5.9 pix
The object was found in VSX 9" ZTF J232648.96+572431.3
Type: EA
# Max. Min./Amp. JD0 Period
17.638 r Y 0.637 r 2458376.87550 0.498432800000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:47.97 +57:24:35.9: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:47.97 +57:24:35.9: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 26 47.97 +57 24 35.9 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J232648.96+572431.3,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J232648.96+572431.3 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.41 23:16:13.35 +55:12:31.4
109.56213 -5.17212 galactic Cas Second-epoch detections are separated by 7.2" and 6.3 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 | 23:16:13.35 +55:12:31.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:16:13.35 +55:12:31.4: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:16:13.35 +55:12:31.4: 14.92 +/- 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 08 28.2058* 23 16 13.35 +55 12 31.4 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,2461280.7058,14.41,0.05,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 20260828.2058 14.41CV 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 08 28.2058 2461280.7058 14.31 23:54:00.82 +50:12:59.3
113.61041 -11.61307 galactic Cas Second-epoch detections are separated by 8.4" and 6.6 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 | 23:54:00.82 +50:12:59.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:54:00.82 +50:12:59.3: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:54:00.82 +50:12:59.3: 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 08 28.2058* 23 54 00.82 +50 12 59.3 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:29:29.10 +51:00:39.4
110.01859 -9.79446 galactic Cas Second-epoch detections are separated by 7.5" and 6.3 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 | 23:29:29.10 +51:00:39.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:29.10 +51:00:39.4: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:29:29.10 +51:00:39.4: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 29 29.10 +51 00 39.4 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,2461280.7058,14.26,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.16 23:29:57.38 +55:09:17.0
111.39865 -5.88198 galactic Cas Second-epoch detections are separated by 5.1" and 6.7 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 | 23:29:57.38 +55:09:17.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:57.38 +55:09:17.0: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:29:57.38 +55:09:17.0: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 29 57.38 +55 09 17.0 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.16,0.05,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 20260828.2058 14.16CV 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 08 28.2058 2461280.7058 14.21 23:34:23.08 +50:30:41.4
110.61166 -10.50788 galactic And Second-epoch detections are separated by 7.6" and 6.4 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 | 23:34:23.08 +50:30:41.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:23.08 +50:30:41.4: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:23.08 +50:30:41.4: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 23.08 +50 30 41.4 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.21 23:27:52.16 +57:08:13.7
111.74803 -3.90886 galactic Cas Second-epoch detections are separated by 8.1" and 6.3 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 | 23:27:52.16 +57:08:13.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:52.16 +57:08:13.7: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:52.16 +57:08:13.7: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 27 52.16 +57 08 13.7 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.19 23:39:10.80 +52:38:27.8
111.95899 -8.68441 galactic Cas Second-epoch detections are separated by 6.5" and 6.4 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 J354.8063+52.6438 | 23:39:10.80 +52:38:27.8 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:10.80 +52:38:27.8: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:10.80 +52:38:27.8: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 39 10.80 +52 38 27.8 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 J354.8063+52.6438,2461280.7058,14.19,0.05,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 J354.8063+52.6438 20260828.2058 14.19CV 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 08 28.2058 2461280.7058 14.20 00:08:58.01 +52:27:28.7
116.38809 -9.87332 galactic Cas Second-epoch detections are separated by 1.8" and 6.6 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 | 00:08:58.01 +52:27:28.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:08:58.01 +52:27:28.7: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:08:58.01 +52:27:28.7: 15.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 08 58.01 +52 27 28.7 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.20,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.39 00:03:29.46 +53:34:39.7
115.76733 -8.62575 galactic Cas Second-epoch detections are separated by 8.9" and 6.7 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 J000.8553+53.5845 | 00:03:29.46 +53:34:39.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:03:29.46 +53:34:39.7: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:03:29.46 +53:34:39.7: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 03 29.46 +53 34 39.7 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 J000.8553+53.5845,2461280.7058,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J000.8553+53.5845 20260828.2058 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.02 23:09:15.63 +57:16:03.9
109.43104 -2.90115 galactic Cas Second-epoch detections are separated by 7.1" and 6.2 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 | 23:09:15.63 +57:16:03.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:09:15.63 +57:16:03.9: 15.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:09:15.63 +57:16:03.9: 14.73 +/- 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 08 28.2058* 23 09 15.63 +57 16 03.9 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
target,2461280.7058,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.02CV 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 08 28.2058 2461280.7058 14.15 23:26:02.96 +53:45:44.1
110.41018 -7.02063 galactic Cas Second-epoch detections are separated by 8.9" and 6.5 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 | 23:26:02.96 +53:45:44.1 (user input) | T | P | (position from user input) J-Ks=1.016+/-0.234 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:02.96 +53:45:44.1: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:02.96 +53:45:44.1: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 26 02.96 +53 45 44.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.07 23:19:34.37 +50:14:46.9
108.25536 -9.98922 galactic And Second-epoch detections are separated by 1.7" and 6.5 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 | 23:19:34.37 +50:14:46.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:34.37 +50:14:46.9: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:34.37 +50:14:46.9: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 34.37 +50 14 46.9 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.07,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.29 23:17:51.12 +53:37:04.6
109.21165 -6.74223 galactic Cas Second-epoch detections are separated by 8.0" and 6.3 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 J349.4769+53.6220 | 23:17:51.12 +53:37:04.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:51.12 +53:37:04.6: 15.46 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:51.12 +53:37:04.6: 14.86 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.46 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 17 51.12 +53 37 04.6 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 J349.4769+53.6220,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.4769+53.6220 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.22 23:29:02.05 +50:39:49.2
109.83825 -10.10125 galactic And Second-epoch detections are separated by 5.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:29:02.05 +50:39:49.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:02.05 +50:39:49.2: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:29:02.05 +50:39:49.2: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 29 02.05 +50 39 49.2 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.19 23:24:52.23 +53:53:18.9
110.28648 -6.84417 galactic Cas Second-epoch detections are separated by 3.0" and 6.6 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 | 23:24:52.23 +53:53:18.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:52.23 +53:53:18.9: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:52.23 +53:53:18.9: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 24 52.23 +53 53 18.9 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.19,0.05,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 20260828.2058 14.19CV 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 08 28.2058 2461280.7058 14.17 23:24:18.43 +51:34:22.7
109.42799 -8.99972 galactic And Second-epoch detections are separated by 1.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:18.43 +51:34:22.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:18.43 +51:34:22.7: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:18.43 +51:34:22.7: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 24 18.43 +51 34 22.7 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:23:04.40 +52:25:37.5
109.53755 -8.13149 galactic And Second-epoch detections are separated by 7.2" and 6.3 pix
The object was found in VSX25" Gaia DR3 1992400285983099008
Type:
# Max. Min./Amp. JD0 Period
15.510 G 15.540 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:04.40 +52:25:37.5: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:04.40 +52:25:37.5: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 04.40 +52 25 37.5 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992400285983099008,2461280.7058,14.26,0.05,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
Gaia DR3 1992400285983099008 20260828.2058 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 08 28.2058 2461280.7058 14.34 00:08:29.28 +51:35:14.5
116.16598 -10.71927 galactic Cas Second-epoch detections are separated by 6.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:08:29.28 +51:35:14.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:08:29.28 +51:35:14.5: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:08:29.28 +51:35:14.5: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 08 29.28 +51 35 14.5 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,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.28 00:04:32.67 +51:18:17.9
115.49954 -10.88880 galactic Cas Second-epoch detections are separated by 6.6" and 6.7 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 J001.1258+51.3056 | 00:04:32.67 +51:18:17.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:04:32.67 +51:18:17.9: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:04:32.67 +51:18:17.9: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 04 32.67 +51 18 17.9 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J001.1258+51.3056,2461280.7058,14.28,0.05,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 J001.1258+51.3056 20260828.2058 14.28CV 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 08 28.2058 2461280.7058 14.36 23:18:26.78 +53:20:30.8
109.19623 -7.03170 galactic Cas Second-epoch detections are separated by 7.5" and 6.2 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 | 23:18:26.78 +53:20:30.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:26.78 +53:20:30.8: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:26.78 +53:20:30.8: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 26.78 +53 20 30.8 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
target,2461280.7058,14.36,0.05,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 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.15 23:15:46.07 +57:41:56.2
110.40443 -2.82707 galactic Cas Second-epoch detections are separated by 6.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:15:46.07 +57:41:56.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:46.07 +57:41:56.2: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:46.07 +57:41:56.2: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 15 46.07 +57 41 56.2 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.13 23:16:41.88 +57:37:13.2
110.49234 -2.94516 galactic Cas Second-epoch detections are separated by 5.9" and 6.5 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 | 23:16:41.88 +57:37:13.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:16:41.88 +57:37:13.2: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:16:41.88 +57:37:13.2: 14.80 +/- 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 08 28.2058* 23 16 41.88 +57 37 13.2 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,2461280.7058,14.13,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.29 23:15:56.98 +56:35:14.2
110.02533 -3.87263 galactic Cas Second-epoch detections are separated by 8.8" and 6.2 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 | 23:15:56.98 +56:35:14.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:56.98 +56:35:14.2: 15.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:56.98 +56:35:14.2: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 15 56.98 +56 35 14.2 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,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.13 23:17:31.57 +57:13:09.0
110.45339 -3.35971 galactic Cas Second-epoch detections are separated by 4.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:17:31.57 +57:13:09.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:31.57 +57:13:09.0: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:31.57 +57:13:09.0: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 17 31.57 +57 13 09.0 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.13,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.18 23:32:54.99 +53:38:40.9
111.34557 -7.45135 galactic Cas Second-epoch detections are separated by 5.5" and 6.7 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 | 23:32:54.99 +53:38:40.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:54.99 +53:38:40.9: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:54.99 +53:38:40.9: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 32 54.99 +53 38 40.9 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.10 23:22:19.10 +54:46:28.8
110.23233 -5.88467 galactic Cas Second-epoch detections are separated by 8.9" and 6.5 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 | 23:22:19.10 +54:46:28.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:19.10 +54:46:28.8: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:19.10 +54:46:28.8: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 22 19.10 +54 46 28.8 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,2461280.7058,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.14 23:36:05.96 +54:46:13.3
112.12846 -6.51337 galactic Cas Second-epoch detections are separated by 0.6" and 6.5 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 | 23:36:05.96 +54:46:13.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:05.96 +54:46:13.3: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:05.96 +54:46:13.3: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 36 05.96 +54 46 13.3 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,2461280.7058,14.14,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.20 23:31:17.80 +54:01:18.7
111.23182 -7.01934 galactic Cas Second-epoch detections are separated by 1.3" and 6.1 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 J352.8312+54.0204 | 23:31:17.80 +54:01:18.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:17.80 +54:01:18.7: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:17.80 +54:01:18.7: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 17.80 +54 01 18.7 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 J352.8312+54.0204,2461280.7058,14.20,0.05,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 J352.8312+54.0204 20260828.2058 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 08 28.2058 2461280.7058 14.28 23:23:47.22 +52:32:55.6
109.68228 -8.05349 galactic And Second-epoch detections are separated by 5.4" and 6.5 pix
The object was found in VSX21" Gaia DR3 1992402824304726528
Type: S
# Max. Min./Amp. JD0 Period
17.320 G 18.260 G
ATTENTION: measured mag 14.28 is 3.0 mag brighter than the VSX record maximum brightness 17.32 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:47.22 +52:32:55.6: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:47.22 +52:32:55.6: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 47.22 +52 32 55.6 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992402824304726528,2461280.7058,14.28,0.05,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
Gaia DR3 1992402824304726528 20260828.2058 14.28CV 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 08 28.2058 2461280.7058 14.21 00:05:44.31 +50:40:09.1
115.56991 -11.54816 galactic Cas Second-epoch detections are separated by 5.3" and 6.7 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 395477603620972544 | 00:05:40.10 +50:40:13.4 (Gaia DR3) | ROT (local) | 8.231500000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:44.31 +50:40:09.1: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:44.31 +50:40:09.1: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 05 44.31 +50 40 09.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395477603620972544,2461280.7058,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 395477603620972544 20260828.2058 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.09 23:18:06.71 +50:59:08.4
108.30168 -9.21579 galactic And Second-epoch detections are separated by 2.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:18:06.71 +50:59:08.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:06.71 +50:59:08.4: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:06.71 +50:59:08.4: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 06.71 +50 59 08.4 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.09,0.05,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 20260828.2058 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.23 23:52:25.64 +52:52:42.7
113.98140 -8.96466 galactic Cas Second-epoch detections are separated by 7.9" and 6.2 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 | 23:52:25.64 +52:52:42.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:52:25.64 +52:52:42.7: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:52:25.64 +52:52:42.7: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 52 25.64 +52 52 42.7 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.17 23:18:48.13 +50:21:35.5
108.17930 -9.83951 galactic And Second-epoch detections are separated by 4.2" and 6.8 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 | 23:18:48.13 +50:21:35.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:48.13 +50:21:35.5: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:48.13 +50:21:35.5: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 48.13 +50 21 35.5 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.23 23:38:11.37 +52:05:02.3
111.65351 -9.17649 galactic Cas Second-epoch detections are separated by 8.6" and 6.5 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 J354.5500+52.0712 | 23:38:11.37 +52:05:02.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:11.37 +52:05:02.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:11.37 +52:05:02.3: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 38 11.37 +52 05 02.3 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.5500+52.0712,2461280.7058,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.5500+52.0712 20260828.2058 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.14 23:25:37.16 +51:45:06.5
109.68240 -8.89857 galactic And Second-epoch detections are separated by 7.5" and 6.3 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 | 23:25:37.16 +51:45:06.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:25:37.16 +51:45:06.5: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:25:37.16 +51:45:06.5: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 25 37.16 +51 45 06.5 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.14,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.16 23:17:39.13 +56:25:45.6
110.18847 -4.10419 galactic Cas Second-epoch detections are separated by 7.9" and 6.6 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 | 23:17:39.13 +56:25:45.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:39.13 +56:25:45.6: 15.07 +/- 0.26 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:39.13 +56:25:45.6: 14.89 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.07 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 17 39.13 +56 25 45.6 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.16,0.05,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 20260828.2058 14.16CV 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 08 28.2058 2461280.7058 14.18 23:26:19.28 +53:47:48.6
110.45981 -7.00103 galactic Cas Second-epoch detections are separated by 4.9" and 6.4 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 J351.5988+53.7960 | 23:26:19.28 +53:47:48.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:19.28 +53:47:48.6: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:19.28 +53:47:48.6: 14.73 +/- 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 08 28.2058* 23 26 19.28 +53 47 48.6 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 J351.5988+53.7960,2461280.7058,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.5988+53.7960 20260828.2058 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.23 23:19:52.88 +49:51:22.2
108.16280 -10.37185 galactic And Second-epoch detections are separated by 7.4" and 6.4 pix
The object was found in VSX 4" Gaia DR3 1991159482809413504
Type: E
# Max. Min./Amp. JD0 Period
19.220 G 20.150 G 0.427519000000
ATTENTION: measured mag 14.23 is 5.0 mag brighter than the VSX record maximum brightness 19.22 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:52.88 +49:51:22.2: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:52.88 +49:51:22.2: 14.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 52.88 +49 51 22.2 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991159482809413504,2461280.7058,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991159482809413504 20260828.2058 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:45:01.22 +55:19:04.4
113.51577 -6.33495 galactic Cas Second-epoch detections are separated by 4.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.2373+55.3196 | 23:45:01.22 +55:19:04.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:01.22 +55:19:04.4: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:01.22 +55:19:04.4: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 45 01.22 +55 19 04.4 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 J356.2373+55.3196,2461280.7058,14.26,0.05,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
ATO J356.2373+55.3196 20260828.2058 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 08 28.2058 2461280.7058 14.06 00:10:41.39 +53:58:59.5
116.89730 -8.41043 galactic Cas Second-epoch detections are separated by 8.0" and 6.5 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 | 00:10:41.39 +53:58:59.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:10:41.39 +53:58:59.5: 15.59 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:10:41.39 +53:58:59.5: 15.08 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.59 +/- 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 08 28.2058* 00 10 41.39 +53 58 59.5 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,2461280.7058,14.06,0.05,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 20260828.2058 14.06CV 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 08 28.2058 2461280.7058 14.16 23:56:48.43 +50:59:50.3
114.22621 -10.94868 galactic Cas Second-epoch detections are separated by 7.5" and 6.6 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 | 23:56:48.43 +50:59:50.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:56:48.43 +50:59:50.3: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:56:48.43 +50:59:50.3: 15.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 56 48.43 +50 59 50.3 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.16,0.05,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 20260828.2058 14.16CV 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 08 28.2058 2461280.7058 14.13 23:21:29.67 +54:16:21.5
109.94724 -6.31589 galactic Cas Second-epoch detections are separated by 2.7" and 6.3 pix
The object was found in VSX11" ZTF J232129.53+541632.4
Type: EW
# Max. Min./Amp. JD0 Period
17.382 r Y 0.094 r 2458324.97230 0.389571200000
ATTENTION: measured mag 14.13 is 3.2 mag brighter than the VSX record maximum brightness 17.29 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:29.67 +54:16:21.5: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:29.67 +54:16:21.5: 14.92 +/- 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 08 28.2058* 23 21 29.67 +54 16 21.5 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
ZTF J232129.53+541632.4,2461280.7058,14.13,0.05,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
ZTF J232129.53+541632.4 20260828.2058 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 08 28.2058 2461280.7058 14.22 23:28:38.20 +51:01:20.5
109.89390 -9.74126 galactic Cas Second-epoch detections are separated by 8.1" and 6.7 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 | 23:28:38.20 +51:01:20.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:38.20 +51:01:20.5: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:38.20 +51:01:20.5: 14.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 28 38.20 +51 01 20.5 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.13 23:30:52.31 +54:23:23.5
111.28641 -6.65009 galactic Cas Second-epoch detections are separated by 2.6" and 6.4 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 J352.6976+54.3862 | 23:30:52.31 +54:23:23.5 (user input) | DBF (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:52.31 +54:23:23.5: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:52.31 +54:23:23.5: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 52.31 +54 23 23.5 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 J352.6976+54.3862,2461280.7058,14.13,0.05,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
ATO J352.6976+54.3862 20260828.2058 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 08 28.2058 2461280.7058 14.05 23:37:39.47 +51:21:05.3
111.36215 -9.85528 galactic Cas Second-epoch detections are separated by 7.7" and 6.7 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 J354.4306+51.3499 | 23:37:39.47 +51:21:05.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.736+/-0.139 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:39.47 +51:21:05.3: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:39.47 +51:21:05.3: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 37 39.47 +51 21 05.3 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.4306+51.3499,2461280.7058,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.4306+51.3499 20260828.2058 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.24 00:08:10.60 +52:36:10.1
116.29256 -9.71036 galactic Cas Second-epoch detections are separated by 7.8" and 6.7 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 | 00:08:10.60 +52:36:10.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:08:10.60 +52:36:10.1: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:08:10.60 +52:36:10.1: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 08 10.60 +52 36 10.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.15 23:30:21.39 +50:22:09.6
109.94648 -10.44690 galactic And Second-epoch detections are separated by 3.4" and 6.6 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 | 23:30:21.39 +50:22:09.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:21.39 +50:22:09.6: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:21.39 +50:22:09.6: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 21.39 +50 22 09.6 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.20 00:20:28.23 +54:57:49.1
118.45664 -7.63880 galactic Cas Second-epoch detections are separated by 7.9" and 6.2 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 | 00:20:28.23 +54:57:49.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:20:28.23 +54:57:49.1: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:20:28.23 +54:57:49.1: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 20 28.23 +54 57 49.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.20,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.10 23:43:35.35 +55:18:49.6
113.31682 -6.28628 galactic Cas Second-epoch detections are separated by 2.5" and 6.2 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 | 23:43:35.35 +55:18:49.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:43:35.35 +55:18:49.6: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:43:35.35 +55:18:49.6: 15.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 43 35.35 +55 18 49.6 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,2461280.7058,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.15 23:53:59.45 +50:05:18.9
113.57734 -11.73685 galactic Cas Second-epoch detections are separated by 7.3" and 6.6 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 | 23:53:59.45 +50:05:18.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:53:59.45 +50:05:18.9: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:53:59.45 +50:05:18.9: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 53 59.45 +50 05 18.9 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.15 23:40:12.92 +55:26:29.3
112.88672 -6.03507 galactic Cas Second-epoch detections are separated by 7.7" and 6.6 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 | 23:40:12.92 +55:26:29.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:40:12.92 +55:26:29.3: 15.58 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:40:12.92 +55:26:29.3: 14.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.58 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 40 12.92 +55 26 29.3 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.20 00:07:29.15 +51:05:33.0
115.92280 -11.18012 galactic Cas Second-epoch detections are separated by 1.0" and 6.7 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 | 00:07:29.15 +51:05:33.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:29.15 +51:05:33.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:29.15 +51:05:33.0: 15.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 07 29.15 +51 05 33.0 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.20,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.19 23:39:36.07 +51:31:08.8
111.70503 -9.77991 galactic Cas Second-epoch detections are separated by 6.3" and 6.3 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 | 23:39:36.07 +51:31:08.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:36.07 +51:31:08.8: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:36.07 +51:31:08.8: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 39 36.07 +51 31 08.8 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
target,2461280.7058,14.19,0.05,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 20260828.2058 14.19CV 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 08 28.2058 2461280.7058 14.09 23:18:04.96 +55:30:11.1
109.91561 -4.99165 galactic Cas Second-epoch detections are separated by 7.2" and 6.3 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 | 23:18:04.96 +55:30:11.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:04.96 +55:30:11.1: 15.04 +/- 0.27 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:04.96 +55:30:11.1: 14.85 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.04 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 04.96 +55 30 11.1 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,2461280.7058,14.09,0.05,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 20260828.2058 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.00 23:17:32.53 +56:09:21.0
110.07673 -4.35443 galactic Cas Second-epoch detections are separated by 3.5" and 6.4 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 1997177079892670336 | 23:17:30.28 +56:08:42.4 (Gaia DR3) | E (local) | 6.931300000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.433+/-0.054 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:32.53 +56:09:21.0: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:32.53 +56:09:21.0: 14.85 +/- 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 08 28.2058* 23 17 32.53 +56 09 21.0 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
Gaia DR3 1997177079892670336,2461280.7058,14.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1997177079892670336 20260828.2058 14.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.06 23:57:13.66 +51:50:40.9
114.47491 -10.13468 galactic Cas Second-epoch detections are separated by 8.7" and 6.5 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 | 23:57:13.66 +51:50:40.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:13.66 +51:50:40.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:13.66 +51:50:40.9: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 57 13.66 +51 50 40.9 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.06,0.05,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 20260828.2058 14.06CV 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 08 28.2058 2461280.7058 14.09 23:23:07.34 +49:28:50.7
108.53108 -10.90563 galactic And Second-epoch detections are separated by 5.8" and 6.7 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 1943050905592679424 | 23:23:08.57 +49:28:11.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:07.34 +49:28:50.7: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:07.34 +49:28:50.7: 14.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 07.34 +49 28 50.7 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943050905592679424,2461280.7058,14.09,0.05,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
Gaia DR3 1943050905592679424 20260828.2058 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.14 00:06:07.57 +50:16:46.8
115.56055 -11.94243 galactic Cas Second-epoch detections are separated by 5.6" and 6.6 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 | 00:06:07.57 +50:16:46.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:06:07.57 +50:16:46.8: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:06:07.57 +50:16:46.8: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 06 07.57 +50 16 46.8 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,2461280.7058,14.14,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.11 23:23:13.80 +51:43:35.2
109.32095 -8.79900 galactic And Second-epoch detections are separated by 3.5" and 6.8 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 J350.7977+51.7176 | 23:23:13.80 +51:43:35.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:13.80 +51:43:35.2: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:13.80 +51:43:35.2: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 13.80 +51 43 35.2 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.7977+51.7176,2461280.7058,14.11,0.05,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 J350.7977+51.7176 20260828.2058 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.08 23:30:43.51 +55:32:50.3
111.62535 -5.54260 galactic Cas Second-epoch detections are separated by 1.7" and 6.5 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 | 23:30:43.51 +55:32:50.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:43.51 +55:32:50.3: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:43.51 +55:32:50.3: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 43.51 +55 32 50.3 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,2461280.7058,14.08,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.03 23:24:54.00 +51:36:31.5
109.52796 -8.99668 galactic And Second-epoch detections are separated by 7.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:54.00 +51:36:31.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:54.00 +51:36:31.5: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:54.00 +51:36:31.5: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 24 54.00 +51 36 31.5 14.0 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,2461280.7058,14.03,0.05,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 20260828.2058 14.03CV 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 08 28.2058 2461280.7058 14.10 23:14:42.54 +55:59:12.5
109.64579 -4.36952 galactic Cas Second-epoch detections are separated by 4.1" and 6.0 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 | 23:14:42.54 +55:59:12.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:14:42.54 +55:59:12.5: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:42.54 +55:59:12.5: 14.75 +/- 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 08 28.2058* 23 14 42.54 +55 59 12.5 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,2461280.7058,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.14 23:59:31.46 +54:09:40.4
115.30235 -7.93971 galactic Cas Second-epoch detections are separated by 8.0" and 6.4 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 J359.8907+54.1501 | 23:59:31.46 +54:09:40.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:59:31.46 +54:09:40.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:59:31.46 +54:09:40.4: 15.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 59 31.46 +54 09 40.4 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
ATO J359.8907+54.1501,2461280.7058,14.14,0.05,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
ATO J359.8907+54.1501 20260828.2058 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 08 28.2058 2461280.7058 14.03 23:17:49.47 +51:39:33.9
108.50289 -8.57047 galactic And Second-epoch detections are separated by 8.9" and 6.4 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 J349.4612+51.6677 | 23:17:49.47 +51:39:33.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:49.47 +51:39:33.9: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:49.47 +51:39:33.9: 14.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 17 49.47 +51 39 33.9 14.0 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
ATO J349.4612+51.6677,2461280.7058,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.4612+51.6677 20260828.2058 14.03CV 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 08 28.2058 2461280.7058 14.09 23:35:50.44 +54:56:06.3
112.14061 -6.34493 galactic Cas Second-epoch detections are separated by 4.3" and 6.4 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 | 23:35:50.44 +54:56:06.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:50.44 +54:56:06.3: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:50.44 +54:56:06.3: 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 08 28.2058* 23 35 50.44 +54 56 06.3 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,2461280.7058,14.09,0.05,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 20260828.2058 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.16 00:07:34.46 +51:47:00.5
116.05802 -10.50189 galactic Cas Second-epoch detections are separated by 3.6" and 6.6 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 | 00:07:34.46 +51:47:00.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:34.46 +51:47:00.5: 15.09 +/- 0.21 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:34.46 +51:47:00.5: 14.96 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.05 +/- 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 08 28.2058* 00 07 34.46 +51 47 00.5 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.16,0.05,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 20260828.2058 14.16CV 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 08 28.2058 2461280.7058 14.29 23:35:16.90 +50:04:40.1
110.61971 -10.96455 galactic And Second-epoch detections are separated by 7.3" and 6.8 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 | 23:35:16.90 +50:04:40.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:16.90 +50:04:40.1: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:16.90 +50:04:40.1: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 35 16.90 +50 04 40.1 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.18 23:39:11.14 +57:04:18.8
113.19927 -4.42827 galactic Cas Second-epoch detections are separated by 7.2" and 5.5 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 | 23:39:11.14 +57:04:18.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:11.14 +57:04:18.8: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:11.14 +57:04:18.8: 14.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 39 11.14 +57 04 18.8 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
target,2461280.7058,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.02 23:30:06.64 +55:31:12.4
111.53383 -5.54155 galactic Cas Second-epoch detections are separated by 5.1" and 6.5 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 J352.5270+55.5075 | 23:30:06.64 +55:31:12.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:06.64 +55:31:12.4: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:06.64 +55:31:12.4: 14.92 +/- 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 08 28.2058* 23 30 06.64 +55 31 12.4 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 J352.5270+55.5075,2461280.7058,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.5270+55.5075 20260828.2058 14.02CV 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 08 28.2058 2461280.7058 14.03 00:16:59.35 +52:47:31.5
117.66053 -9.72672 galactic Cas Second-epoch detections are separated by 0.8" and 6.6 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 419200460341859712 | 00:16:55.06 +52:47:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:16:59.35 +52:47:31.5: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:16:59.35 +52:47:31.5: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 16 59.35 +52 47 31.5 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
Gaia DR3 419200460341859712,2461280.7058,14.03,0.05,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 419200460341859712 20260828.2058 14.03CV 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 08 28.2058 2461280.7058 14.10 23:23:12.70 +56:57:56.7
111.09197 -3.86403 galactic Cas Second-epoch detections are separated by 2.2" and 6.5 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 | 23:23:12.70 +56:57:56.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:12.70 +56:57:56.7: 15.29 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:12.70 +56:57:56.7: 14.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.29 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 12.70 +56 57 56.7 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,2461280.7058,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.07 23:45:23.37 +50:21:07.2
112.28018 -11.14875 galactic Cas Second-epoch detections are separated by 7.7" and 6.6 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 | 23:45:23.37 +50:21:07.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:23.37 +50:21:07.2: 15.55 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:23.37 +50:21:07.2: 15.04 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.55 +/- 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 08 28.2058* 23 45 23.37 +50 21 07.2 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,2461280.7058,14.07,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.09 00:19:26.40 +49:42:31.1
117.63600 -12.83380 galactic Cas Second-epoch detections are separated by 7.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:19:26.40 +49:42:31.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:19:26.40 +49:42:31.1: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:19:26.40 +49:42:31.1: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 19 26.40 +49 42 31.1 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,2461280.7058,14.09,0.05,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 20260828.2058 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.08 00:06:29.74 +51:42:56.0
115.87878 -10.53967 galactic Cas Second-epoch detections are separated by 4.2" and 6.3 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 | 00:06:29.74 +51:42:56.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:06:29.74 +51:42:56.0: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:06:29.74 +51:42:56.0: 15.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 06 29.74 +51 42 56.0 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.08,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.95 23:27:25.43 +56:44:45.4
111.56520 -4.26023 galactic Cas Second-epoch detections are separated by 6.7" and 6.4 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 | 23:27:25.43 +56:44:45.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:25.43 +56:44:45.4: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:25.43 +56:44:45.4: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 27 25.43 +56 44 45.4 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,2461280.7058,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.02 23:38:26.80 +56:58:36.3
113.07585 -4.49168 galactic Cas Second-epoch detections are separated by 2.6" and 6.3 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 | 23:38:26.80 +56:58:36.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:26.80 +56:58:36.3: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:26.80 +56:58:36.3: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 38 26.80 +56 58 36.3 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,2461280.7058,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.02CV 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 08 28.2058 2461280.7058 13.98 23:27:41.36 +54:21:24.4
110.83305 -6.53582 galactic Cas Second-epoch detections are separated by 6.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:27:41.36 +54:21:24.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:41.36 +54:21:24.4: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:41.36 +54:21:24.4: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 27 41.36 +54 21 24.4 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,2461280.7058,13.98,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.01 23:23:09.84 +53:47:00.6
110.01213 -6.85922 galactic Cas Second-epoch detections are separated by 4.9" and 6.7 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 | 23:23:09.84 +53:47:00.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:09.84 +53:47:00.6: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:09.84 +53:47:00.6: 14.92 +/- 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 08 28.2058* 23 23 09.84 +53 47 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
target,2461280.7058,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.93 23:13:46.60 +54:38:25.2
109.02511 -5.57295 galactic Cas Second-epoch detections are separated by 7.6" and 6.5 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 | 23:13:46.60 +54:38:25.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:13:46.60 +54:38:25.2: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:13:46.60 +54:38:25.2: 14.85 +/- 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 08 28.2058* 23 13 46.60 +54 38 25.2 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
target,2461280.7058,13.93,0.05,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 20260828.2058 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.02 23:11:38.67 +56:35:48.7
109.47681 -3.64530 galactic Cas Second-epoch detections are separated by 3.6" and 6.6 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 | 23:11:38.67 +56:35:48.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:11:38.67 +56:35:48.7: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:11:38.67 +56:35:48.7: 14.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 11 38.67 +56 35 48.7 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,2461280.7058,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.02CV 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 08 28.2058 2461280.7058 14.03 23:31:16.51 +51:15:13.0
110.36623 -9.65180 galactic Cas Second-epoch detections are separated by 4.1" and 6.5 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 | 23:31:16.51 +51:15:13.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:16.51 +51:15:13.0: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:16.51 +51:15:13.0: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 16.51 +51 15 13.0 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,2461280.7058,14.03,0.05,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 20260828.2058 14.03CV 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 08 28.2058 2461280.7058 13.96 00:16:18.85 +56:42:06.0
118.09926 -5.84015 galactic Cas Second-epoch detections are separated by 3.7" and 6.6 pix
The object was found in VSX14" Gaia DR3 421604508158822528
Type: ROT
# Max. Min./Amp. JD0 Period
15.280 G 15.310 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:16:18.85 +56:42:06.0: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:16:18.85 +56:42:06.0: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 16 18.85 +56 42 06.0 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
Gaia DR3 421604508158822528,2461280.7058,13.96,0.05,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
Gaia DR3 421604508158822528 20260828.2058 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 08 28.2058 2461280.7058 13.93 23:12:08.53 +57:31:17.6
109.88705 -2.81350 galactic Cas Second-epoch detections are separated by 4.7" and 6.7 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 | 23:12:08.53 +57:31:17.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:08.53 +57:31:17.6: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:08.53 +57:31:17.6: 14.78 +/- 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 08 28.2058* 23 12 08.53 +57 31 17.6 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,2461280.7058,13.93,0.05,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 20260828.2058 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.99 23:34:14.03 +52:18:18.2
111.13128 -8.78886 galactic Cas Second-epoch detections are separated by 3.9" and 6.2 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 | 23:34:14.03 +52:18:18.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:14.03 +52:18:18.2: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:14.03 +52:18:18.2: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 14.03 +52 18 18.2 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
target,2461280.7058,13.99,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.86 23:17:18.12 +56:04:16.7
110.01518 -4.42150 galactic Cas Second-epoch detections are separated by 3.8" and 6.5 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 | 23:17:18.12 +56:04:16.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:18.12 +56:04:16.7: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:18.12 +56:04:16.7: 14.85 +/- 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 08 28.2058* 23 17 18.12 +56 04 16.7 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.04 23:59:22.19 +50:46:57.6
114.58318 -11.24311 galactic Cas Second-epoch detections are separated by 4.0" and 6.2 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 | 23:59:22.19 +50:46:57.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:59:22.19 +50:46:57.6: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:59:22.19 +50:46:57.6: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 59 22.19 +50 46 57.6 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,2461280.7058,14.04,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.04 00:00:44.99 +52:08:03.4
115.07420 -9.96244 galactic Cas Second-epoch detections are separated by 5.6" and 6.6 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 | 00:00:44.99 +52:08:03.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:00:44.99 +52:08:03.4: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:00:44.99 +52:08:03.4: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 00 44.99 +52 08 03.4 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,2461280.7058,14.04,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.07 23:26:05.54 +54:30:20.9
110.66030 -6.31978 galactic Cas Second-epoch detections are separated by 7.7" and 6.6 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 J351.5402+54.4996 | 23:26:05.54 +54:30:20.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:05.54 +54:30:20.9: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:05.54 +54:30:20.9: 14.70 +/- 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 08 28.2058* 23 26 05.54 +54 30 20.9 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 J351.5402+54.4996,2461280.7058,14.07,0.05,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
ATO J351.5402+54.4996 20260828.2058 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 08 28.2058 2461280.7058 13.96 23:33:46.42 +50:32:46.8
110.52807 -10.44554 galactic And Second-epoch detections are separated by 7.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.4341+50.5555 | 23:33:46.42 +50:32:46.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:46.42 +50:32:46.8: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:46.42 +50:32:46.8: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 33 46.42 +50 32 46.8 14.0 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
ATO J353.4341+50.5555,2461280.7058,13.96,0.05,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
ATO J353.4341+50.5555 20260828.2058 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 08 28.2058 2461280.7058 14.05 23:30:40.30 +54:19:13.7
111.23690 -6.70708 galactic Cas Second-epoch detections are separated by 2.3" and 6.8 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 | 23:30:40.30 +54:19:13.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:40.30 +54:19:13.7: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:40.30 +54:19:13.7: 14.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 40.30 +54 19 13.7 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,2461280.7058,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.05 23:42:33.85 +53:51:34.2
112.78644 -7.65003 galactic Cas Second-epoch detections are separated by 2.0" and 6.6 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 | 23:42:33.85 +53:51:34.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:33.85 +53:51:34.2: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:33.85 +53:51:34.2: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 42 33.85 +53 51 34.2 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,2461280.7058,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.05 23:49:27.48 +51:58:31.5
113.32014 -9.73587 galactic Cas Second-epoch detections are separated by 5.4" and 6.5 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 | 23:49:27.48 +51:58:31.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:49:27.48 +51:58:31.5: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:49:27.48 +51:58:31.5: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 49 27.48 +51 58 31.5 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,2461280.7058,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.90 23:58:27.86 +52:16:14.1
114.75416 -9.75804 galactic Cas Second-epoch detections are separated by 5.1" and 6.7 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 | 23:58:27.86 +52:16:14.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:27.86 +52:16:14.1: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:27.86 +52:16:14.1: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 58 27.86 +52 16 14.1 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,2461280.7058,13.90,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 13.98 23:23:34.50 +52:08:32.1
109.51345 -8.42551 galactic And Second-epoch detections are separated by 6.8" and 6.7 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 1992342492902853888 | 23:23:32.97 +52:09:08.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:34.50 +52:08:32.1: 15.46 +/- 0.36 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:34.50 +52:08:32.1: 14.92 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.46 +/- 0.36
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 34.50 +52 08 32.1 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1992342492902853888,2461280.7058,13.98,0.05,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
Gaia DR3 1992342492902853888 20260828.2058 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 08 28.2058 2461280.7058 14.10 23:52:37.11 +53:51:53.0
114.23759 -8.01115 galactic Cas Second-epoch detections are separated by 3.6" and 6.4 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 | 23:52:37.11 +53:51:53.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:52:37.11 +53:51:53.0: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:52:37.11 +53:51:53.0: 15.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 52 37.11 +53 51 53.0 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.97 00:10:19.20 +51:21:32.1
116.41402 -10.99172 galactic Cas Second-epoch detections are separated by 2.3" and 6.5 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 | 00:10:19.20 +51:21:32.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:10:19.20 +51:21:32.1: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:10:19.20 +51:21:32.1: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 10 19.20 +51 21 32.1 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.97,0.05,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 20260828.2058 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.95 23:36:52.38 +55:44:54.7
112.51744 -5.60820 galactic Cas Second-epoch detections are separated by 6.4" and 6.4 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 | 23:36:52.38 +55:44:54.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:52.38 +55:44:54.7: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:52.38 +55:44:54.7: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 36 52.38 +55 44 54.7 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.98 23:16:05.69 +53:59:27.5
109.10267 -6.30095 galactic Cas Second-epoch detections are separated by 6.6" and 6.3 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 J349.0200+53.9930 | 23:16:05.69 +53:59:27.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:16:05.69 +53:59:27.5: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:16:05.69 +53:59:27.5: 14.74 +/- 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 08 28.2058* 23 16 05.69 +53 59 27.5 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 J349.0200+53.9930,2461280.7058,13.98,0.05,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 J349.0200+53.9930 20260828.2058 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 08 28.2058 2461280.7058 13.94 00:17:09.91 +50:18:49.9
117.34630 -12.18582 galactic Cas Second-epoch detections are separated by 5.5" and 6.5 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 | 00:17:09.91 +50:18:49.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:17:09.91 +50:18:49.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:17:09.91 +50:18:49.9: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 17 09.91 +50 18 49.9 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.94,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.94 00:08:05.50 +51:46:22.3
116.13636 -10.52604 galactic Cas Second-epoch detections are separated by 3.2" and 6.6 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 | 00:08:05.50 +51:46:22.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:08:05.50 +51:46:22.3: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:08:05.50 +51:46:22.3: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 08 05.50 +51 46 22.3 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,2461280.7058,13.94,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.93 23:27:04.72 +55:04:53.5
110.98306 -5.82112 galactic Cas Second-epoch detections are separated by 7.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J351.7789+55.0697 | 23:27:04.72 +55:04:53.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:04.72 +55:04:53.5: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:04.72 +55:04:53.5: 14.77 +/- 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 08 28.2058* 23 27 04.72 +55 04 53.5 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 J351.7789+55.0697,2461280.7058,13.93,0.05,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 J351.7789+55.0697 20260828.2058 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.05 00:06:32.90 +54:39:32.0
116.40993 -7.64342 galactic Cas Second-epoch detections are separated by 8.5" and 6.6 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 | 00:06:32.90 +54:39:32.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:06:32.90 +54:39:32.0: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:06:32.90 +54:39:32.0: 15.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 06 32.90 +54 39 32.0 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.97 23:14:26.97 +57:33:59.7
110.19167 -2.88622 galactic Cas Second-epoch detections are separated by 7.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2009549368842708992 | 23:14:24.05 +57:33:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:14:26.97 +57:33:59.7: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:26.97 +57:33:59.7: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 14 26.97 +57 33 59.7 14.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2009549368842708992,2461280.7058,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009549368842708992 20260828.2058 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.95 23:22:41.71 +50:08:48.8
108.69633 -10.25594 galactic And Second-epoch detections are separated by 3.4" and 6.5 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 | 23:22:41.71 +50:08:48.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:41.71 +50:08:48.8: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:41.71 +50:08:48.8: 14.92 +/- 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 08 28.2058* 23 22 41.71 +50 08 48.8 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.84 23:17:19.53 +55:48:30.3
109.92426 -4.66829 galactic Cas Second-epoch detections are separated by 2.1" and 6.0 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 | 23:17:19.53 +55:48:30.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:19.53 +55:48:30.3: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:19.53 +55:48:30.3: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 17 19.53 +55 48 30.3 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,2461280.7058,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.93 23:24:52.56 +55:09:33.4
110.70931 -5.64500 galactic Cas Second-epoch detections are separated by 6.3" and 6.8 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 | 23:24:52.56 +55:09:33.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:52.56 +55:09:33.4: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:52.56 +55:09:33.4: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 24 52.56 +55 09 33.4 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,2461280.7058,13.93,0.05,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 20260828.2058 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.81 23:18:52.99 +54:59:05.7
109.83932 -5.51676 galactic Cas Second-epoch detections are separated by 4.1" and 6.5 pix
The object was found in VSX24" Gaia DR3 1996825236170302720
Type: ROT
# Max. Min./Amp. JD0 Period
14.230 G 14.260 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:52.99 +54:59:05.7: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:52.99 +54:59:05.7: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 52.99 +54 59 05.7 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
Gaia DR3 1996825236170302720,2461280.7058,13.81,0.05,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
Gaia DR3 1996825236170302720 20260828.2058 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 08 28.2058 2461280.7058 13.86 23:31:49.97 +56:40:30.7
112.11956 -4.51614 galactic Cas Second-epoch detections are separated by 2.5" and 6.6 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 | 23:31:49.97 +56:40:30.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:49.97 +56:40:30.7: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:49.97 +56:40:30.7: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 49.97 +56 40 30.7 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.80 23:14:33.20 +57:06:08.3
110.03462 -3.32344 galactic Cas Second-epoch detections are separated by 8.2" and 6.4 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 | 23:14:33.20 +57:06:08.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:14:33.20 +57:06:08.3: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:33.20 +57:06:08.3: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 14 33.20 +57 06 08.3 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,2461280.7058,13.80,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.87 23:24:02.23 +55:45:42.7
110.79706 -5.03705 galactic Cas Second-epoch detections are separated by 2.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:02.23 +55:45:42.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:02.23 +55:45:42.7: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:02.23 +55:45:42.7: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 24 02.23 +55 45 42.7 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.79 00:07:46.77 +54:40:41.9
116.59021 -7.65498 galactic Cas Second-epoch detections are separated by 6.8" and 6.6 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 J001.9389+54.6881 | 00:07:45.35 +54:41:17.2 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:46.77 +54:40:41.9: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:46.77 +54:40:41.9: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 07 46.77 +54 40 41.9 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
ATO J001.9389+54.6881,2461280.7058,13.79,0.05,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 J001.9389+54.6881 20260828.2058 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.88 23:22:30.34 +55:44:27.1
110.58621 -4.98459 galactic Cas Second-epoch detections are separated by 5.2" and 6.3 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 | 23:22:30.34 +55:44:27.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:30.34 +55:44:27.1: 15.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:30.34 +55:44:27.1: 14.69 +/- 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 08 28.2058* 23 22 30.34 +55 44 27.1 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,2461280.7058,13.88,0.05,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 20260828.2058 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.80 23:21:36.05 +52:40:17.3
109.40910 -7.82546 galactic And Second-epoch detections are separated by 6.6" and 6.5 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 | 23:21:36.05 +52:40:17.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:36.05 +52:40:17.3: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:36.05 +52:40:17.3: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 21 36.05 +52 40 17.3 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,2461280.7058,13.80,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.88 23:38:06.02 +51:03:58.2
111.34700 -10.14851 galactic Cas Second-epoch detections are separated by 6.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:38:06.02 +51:03:58.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:06.02 +51:03:58.2: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:06.02 +51:03:58.2: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 38 06.02 +51 03 58.2 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
target,2461280.7058,13.88,0.05,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 20260828.2058 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.97 23:46:39.65 +50:07:15.9
112.42043 -11.42395 galactic Cas Second-epoch detections are separated by 4.4" and 6.8 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 | 23:46:39.65 +50:07:15.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:46:39.65 +50:07:15.9: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:46:39.65 +50:07:15.9: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 46 39.65 +50 07 15.9 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
target,2461280.7058,13.97,0.05,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 20260828.2058 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.79 23:30:38.22 +55:00:24.1
111.44558 -6.05292 galactic Cas Second-epoch detections are separated by 4.2" and 6.4 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 1997424916685930880 | 23:30:38.78 +55:00:57.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:38.22 +55:00:24.1: 14.82 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:38.22 +55:00:24.1: 14.82 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.82 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 38.22 +55 00 24.1 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997424916685930880,2461280.7058,13.79,0.05,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 1997424916685930880 20260828.2058 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.85 23:24:06.72 +51:31:34.1
109.38317 -9.03370 galactic And Second-epoch detections are separated by 2.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:06.72 +51:31:34.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:06.72 +51:31:34.1: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:06.72 +51:31:34.1: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 24 06.72 +51 31 34.1 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,2461280.7058,13.85,0.05,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 20260828.2058 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.88 23:14:16.98 +56:27:23.4
109.76305 -3.91078 galactic Cas Second-epoch detections are separated by 8.0" and 6.3 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 | 23:14:16.98 +56:27:23.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:14:16.98 +56:27:23.4: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:16.98 +56:27:23.4: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 14 16.98 +56 27 23.4 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,2461280.7058,13.88,0.05,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 20260828.2058 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.84 00:02:47.38 +51:31:20.4
115.26744 -10.62400 galactic Cas Second-epoch detections are separated by 4.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:02:47.38 +51:31:20.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:02:47.38 +51:31:20.4: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:02:47.38 +51:31:20.4: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 02 47.38 +51 31 20.4 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,2461280.7058,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.90 23:21:31.13 +51:34:43.0
109.01743 -8.84739 galactic And Second-epoch detections are separated by 6.7" and 6.8 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 | 23:21:31.13 +51:34:43.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:31.13 +51:34:43.0: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:31.13 +51:34:43.0: 14.92 +/- 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 08 28.2058* 23 21 31.13 +51 34 43.0 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.90,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 13.79 00:24:08.31 +50:22:15.3
118.48331 -12.26488 galactic Cas Second-epoch detections are separated by 6.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:24:08.31 +50:22:15.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:24:08.31 +50:22:15.3: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:24:08.31 +50:22:15.3: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 24 08.31 +50 22 15.3 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,2461280.7058,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.79 23:15:46.19 +55:44:39.1
109.69630 -4.64965 galactic Cas Second-epoch detections are separated by 2.5" and 6.4 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 1997144708719631872 | 23:15:47.61 +55:45:05.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:46.19 +55:44:39.1: 14.99 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:46.19 +55:44:39.1: 14.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.99 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 15 46.19 +55 44 39.1 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1997144708719631872,2461280.7058,13.79,0.05,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 1997144708719631872 20260828.2058 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.79 23:15:30.94 +55:29:10.7
109.56893 -4.87699 galactic Cas Second-epoch detections are separated by 7.4" and 6.3 pix
The object was found in VSX10" Gaia DR3 1997079601312812032
Type: S
# Max. Min./Amp. JD0 Period
15.090 G 15.880 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:30.94 +55:29:10.7: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:30.94 +55:29:10.7: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 15 30.94 +55 29 10.7 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
Gaia DR3 1997079601312812032,2461280.7058,13.79,0.05,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 1997079601312812032 20260828.2058 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.77 23:19:52.02 +49:24:30.4
108.00019 -10.79007 galactic And Second-epoch detections are separated by 7.5" and 6.6 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 | 23:19:52.02 +49:24:30.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:52.02 +49:24:30.4: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:52.02 +49:24:30.4: 14.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 52.02 +49 24 30.4 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.77,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.79 23:25:50.46 +54:19:34.7
110.56659 -6.47752 galactic Cas Second-epoch detections are separated by 2.2" and 6.6 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 | 23:25:50.46 +54:19:34.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:25:50.46 +54:19:34.7: 14.77 +/- 0.18 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:25:50.46 +54:19:34.7: 14.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.77 +/- 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 08 28.2058* 23 25 50.46 +54 19 34.7 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,2461280.7058,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.94 23:30:41.60 +51:38:08.5
110.39903 -9.26045 galactic Cas Second-epoch detections are separated by 5.8" and 6.4 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 | 23:30:41.60 +51:38:08.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:41.60 +51:38:08.5: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:41.60 +51:38:08.5: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 41.60 +51 38 08.5 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,2461280.7058,13.94,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.71 23:54:20.86 +51:29:40.6
113.95462 -10.37928 galactic Cas Second-epoch detections are separated by 6.8" and 6.6 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 | 23:54:20.86 +51:29:40.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:54:20.86 +51:29:40.6: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:54:20.86 +51:29:40.6: 15.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 54 20.86 +51 29 40.6 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.71,0.05,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 20260828.2058 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.73 23:41:48.03 +51:06:34.3
111.92642 -10.26810 galactic Cas Second-epoch detections are separated by 6.4" and 6.6 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 | 23:41:48.03 +51:06:34.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:41:48.03 +51:06:34.3: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:41:48.03 +51:06:34.3: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 41 48.03 +51 06 34.3 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
target,2461280.7058,13.73,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.84 23:22:50.20 +51:55:38.5
109.33196 -8.58938 galactic And Second-epoch detections are separated by 7.1" and 6.5 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 | 23:22:50.20 +51:55:38.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:50.20 +51:55:38.5: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:50.20 +51:55:38.5: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 22 50.20 +51 55 38.5 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,2461280.7058,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.84 23:23:17.36 +55:37:43.3
110.65270 -5.12739 galactic Cas Second-epoch detections are separated by 5.0" and 6.6 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 | 23:23:17.36 +55:37:43.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:17.36 +55:37:43.3: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:17.36 +55:37:43.3: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 17.36 +55 37 43.3 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,2461280.7058,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.69 23:45:28.49 +54:37:56.6
113.40311 -7.01439 galactic Cas Second-epoch detections are separated by 7.7" and 6.5 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 | 23:45:28.49 +54:37:56.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:28.49 +54:37:56.6: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:28.49 +54:37:56.6: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 45 28.49 +54 37 56.6 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,2461280.7058,13.69,0.05,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 20260828.2058 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.87 23:55:31.73 +51:24:35.3
114.11807 -10.50263 galactic Cas Second-epoch detections are separated by 7.1" and 6.6 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 J358.8978+51.4028 | 23:55:31.73 +51:24:35.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:55:31.73 +51:24:35.3: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:55:31.73 +51:24:35.3: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 55 31.73 +51 24 35.3 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 J358.8978+51.4028,2461280.7058,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.8978+51.4028 20260828.2058 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.73 23:20:42.25 +52:15:34.7
109.13619 -8.16490 galactic And Second-epoch detections are separated by 5.8" and 6.6 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 | 23:20:42.25 +52:15:34.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:42.25 +52:15:34.7: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:42.25 +52:15:34.7: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 20 42.25 +52 15 34.7 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
target,2461280.7058,13.73,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.76 23:36:30.79 +50:26:34.8
110.92032 -10.67314 galactic And Second-epoch detections are separated by 5.5" and 6.4 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 | 23:36:30.79 +50:26:34.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:30.79 +50:26:34.8: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:30.79 +50:26:34.8: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 36 30.79 +50 26 34.8 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,2461280.7058,13.76,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 13.71 23:27:27.22 +52:12:45.3
110.10451 -8.55504 galactic Cas Second-epoch detections are separated by 8.7" and 6.5 pix
The object was found in VSX11" Gaia DR3 1991676463734530560
Type: ROT
# Max. Min./Amp. JD0 Period
16.270 G 16.320 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:27.22 +52:12:45.3: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:27.22 +52:12:45.3: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 27 27.22 +52 12 45.3 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 1991676463734530560,2461280.7058,13.71,0.05,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
Gaia DR3 1991676463734530560 20260828.2058 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.58 23:10:36.58 +56:49:29.7
109.43145 -3.38049 galactic Cas Second-epoch detections are separated by 5.8" and 6.5 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 | 23:10:36.58 +56:49:29.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:10:36.58 +56:49:29.7: 15.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:10:36.58 +56:49:29.7: 14.81 +/- 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 08 28.2058* 23 10 36.58 +56 49 29.7 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
target,2461280.7058,13.58,0.05,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 20260828.2058 13.58CV 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 08 28.2058 2461280.7058 13.62 23:43:54.73 +53:29:50.5
112.88453 -8.05196 galactic Cas Second-epoch detections are separated by 2.5" and 6.4 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 J355.9857+53.5040 | 23:43:54.73 +53:29:50.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:43:54.73 +53:29:50.5: 14.89 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:43:54.73 +53:29:50.5: 14.43 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 43 54.73 +53 29 50.5 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
ATO J355.9857+53.5040,2461280.7058,13.62,0.05,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 J355.9857+53.5040 20260828.2058 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 08 28.2058 2461280.7058 13.64 23:19:05.21 +50:33:42.9
108.29499 -9.66665 galactic And Second-epoch detections are separated by 2.4" and 6.2 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 | 23:19:05.21 +50:33:42.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:05.21 +50:33:42.9: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:05.21 +50:33:42.9: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 05.21 +50 33 42.9 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.64,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.57 23:37:43.66 +50:45:05.0
111.19852 -10.43345 galactic Cas Second-epoch detections are separated by 3.4" and 6.6 pix
The object was found in VSX21" Gaia DR3 1944539060221592192
Type: ROT
# Max. Min./Amp. JD0 Period
15.630 G 15.670 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:43.66 +50:45:05.0: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:43.66 +50:45:05.0: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 37 43.66 +50 45 05.0 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
Gaia DR3 1944539060221592192,2461280.7058,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944539060221592192 20260828.2058 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.60 00:05:32.75 +50:54:18.9
115.58276 -11.31048 galactic Cas Second-epoch detections are separated by 0.1" and 6.5 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 | 00:05:32.75 +50:54:18.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:32.75 +50:54:18.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:32.75 +50:54:18.9: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 05 32.75 +50 54 18.9 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,2461280.7058,13.60,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 13.35 23:30:32.15 +54:54:01.6
111.39865 -6.14948 galactic Cas Second-epoch detections are separated by 6.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.6420+54.9068 | 23:30:32.15 +54:54:01.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:32.15 +54:54:01.6: 15.21 +/- 0.26 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:32.15 +54:54:01.6: 14.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.21 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 32.15 +54 54 01.6 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 J352.6420+54.9068,2461280.7058,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.6420+54.9068 20260828.2058 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.47 23:20:38.47 +54:42:03.0
109.97828 -5.87120 galactic Cas Second-epoch detections are separated by 3.6" and 6.4 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 | 23:20:38.47 +54:42:03.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:38.47 +54:42:03.0: 14.96 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:38.47 +54:42:03.0: 14.87 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.96 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 20 38.47 +54 42 03.0 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,2461280.7058,13.47,0.05,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 20260828.2058 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.36 23:18:17.24 +54:09:17.2
109.46378 -6.26311 galactic Cas Second-epoch detections are separated by 7.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:18:17.24 +54:09:17.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:17.24 +54:09:17.2: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:17.24 +54:09:17.2: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 17.24 +54 09 17.2 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,2461280.7058,13.36,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.35 00:20:40.54 +52:18:07.6
118.16119 -10.28446 galactic Cas Second-epoch detections are separated by 2.2" and 6.7 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 419126415109275136 | 00:20:37.58 +52:18:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:20:40.54 +52:18:07.6: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:20:40.54 +52:18:07.6: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 20 40.54 +52 18 07.6 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
Gaia DR3 419126415109275136,2461280.7058,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 419126415109275136 20260828.2058 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.28 23:15:06.10 +56:02:21.3
109.71623 -4.34072 galactic Cas Second-epoch detections are separated by 4.1" and 6.6 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 | 23:15:06.10 +56:02:21.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:06.10 +56:02:21.3: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:06.10 +56:02:21.3: 14.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 15 06.10 +56 02 21.3 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,2461280.7058,13.28,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.17 23:38:16.32 +56:01:28.1
112.78494 -5.39910 galactic Cas Second-epoch detections are separated by 8.8" and 6.6 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 | 23:38:16.32 +56:01:28.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:16.32 +56:01:28.1: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:16.32 +56:01:28.1: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 38 16.32 +56 01 28.1 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.11 23:12:55.82 +55:28:00.1
109.21983 -4.76057 galactic Cas Second-epoch detections are separated by 8.0" and 6.5 pix
The object was found in VSX17" ZTF J231256.89+552746.2
Type: BY
# Max. Min./Amp. JD0 Period
17.664 r Y 0.059 r 2458312.92640 0.895689800000
ATTENTION: measured mag 13.11 is 4.5 mag brighter than the VSX record maximum brightness 17.61 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:55.82 +55:28:00.1: 14.30 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:55.82 +55:28:00.1: 14.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.30 +/- 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 08 28.2058* 23 12 55.82 +55 28 00.1 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
ZTF J231256.89+552746.2,2461280.7058,13.11,0.05,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
ZTF J231256.89+552746.2 20260828.2058 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 08 28.2058 2461280.7058 12.83 23:32:12.56 +57:11:42.1
112.32664 -4.03633 galactic Cas Second-epoch detections are separated by 5.9" and 6.6 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 | 23:32:12.56 +57:11:42.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:12.56 +57:11:42.1: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:12.56 +57:11:42.1: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 32 12.56 +57 11 42.1 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.87 23:21:10.38 +55:54:00.5
110.46399 -4.77111 galactic Cas Second-epoch detections are separated by 4.0" and 6.5 pix
The object was found in VSX12" ZTF J232111.75+555357.2
Type: EW
# Max. Min./Amp. JD0 Period
17.487 r Y 0.217 r 2458273.92520 0.421857800000
ATTENTION: measured mag 12.87 is 4.4 mag brighter than the VSX record maximum brightness 17.27 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:10.38 +55:54:00.5: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:10.38 +55:54:00.5: 14.83 +/- 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 08 28.2058* 23 21 10.38 +55 54 00.5 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J232111.75+555357.2,2461280.7058,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J232111.75+555357.2 20260828.2058 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.86 23:12:00.73 +56:27:20.8
109.47080 -3.79509 galactic Cas Second-epoch detections are separated by 3.9" and 6.6 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 | 23:12:00.73 +56:27:20.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:00.73 +56:27:20.8: 15.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:00.73 +56:27:20.8: 14.70 +/- 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 08 28.2058* 23 12 00.73 +56 27 20.8 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.86,0.05,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 20260828.2058 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.70 00:07:16.31 +51:00:11.3
115.87323 -11.26230 galactic Cas Second-epoch detections are separated by 2.5" and 6.5 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 | 00:07:16.31 +51:00:11.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:16.31 +51:00:11.3: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:16.31 +51:00:11.3: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 07 16.31 +51 00 11.3 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
target,2461280.7058,12.70,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 12.36 23:35:42.50 +52:19:08.8
111.35338 -8.84191 galactic Cas Second-epoch detections are separated by 1.5" and 6.5 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 | 23:35:42.50 +52:19:08.8 (user input) | T | P | (position from user input) J-Ks=0.628+/-0.077 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:42.50 +52:19:08.8: 14.60 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:42.50 +52:19:08.8: 14.99 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.60 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 35 42.50 +52 19 08.8 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.36,0.05,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 20260828.2058 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.39 23:30:13.36 +55:17:29.0
111.47765 -5.76390 galactic Cas Second-epoch detections are separated by 3.7" and 6.4 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 | 23:30:13.36 +55:17:29.0 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.042 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:13.36 +55:17:29.0: 15.10 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:13.36 +55:17:29.0: 14.71 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.10 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 13.36 +55 17 29.0 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.63 23:41:59.95 +54:41:41.0
112.93080 -6.82306 galactic Cas Second-epoch detections are separated by 3.2" and 6.7 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 | 23:41:59.95 +54:41:41.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:41:59.95 +54:41:41.0: 14.53 +/- 0.15 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:41:59.95 +54:41:41.0: 14.67 +/- 0.29 detection
Forced photometry reference-image weighted average: 14.56 +/- 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 08 28.2058* 23 41 59.95 +54 41 41.0 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,2461280.7058,12.63,0.05,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 20260828.2058 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 12.63 23:12:59.24 +56:18:47.6
109.54297 -3.97772 galactic Cas Second-epoch detections are separated by 4.0" and 6.4 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 J348.2419+56.3061 | 23:12:59.24 +56:18:47.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:59.24 +56:18:47.6: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:59.24 +56:18:47.6: 14.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 12 59.24 +56 18 47.6 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.2419+56.3061,2461280.7058,12.63,0.05,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
ATO J348.2419+56.3061 20260828.2058 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.00 23:32:51.32 +54:47:13.9
111.68373 -6.35925 galactic Cas Second-epoch detections are separated by 5.2" and 6.5 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 | 23:32:51.32 +54:47:13.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:51.32 +54:47:13.9: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:51.32 +54:47:13.9: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 32 51.32 +54 47 13.9 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
target,2461280.7058,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.49 23:23:37.36 +52:10:37.1
109.53222 -8.39527 galactic And Second-epoch detections are separated by 7.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.9019+52.1860 | 23:23:37.36 +52:10:37.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:37.36 +52:10:37.1: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:37.36 +52:10:37.1: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 37.36 +52 10 37.1 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.9019+52.1860,2461280.7058,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.9019+52.1860 20260828.2058 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.48 00:24:44.88 +53:56:10.0
118.96368 -8.72987 galactic Cas Second-epoch detections are separated by 8.2" and 6.3 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 | 00:24:44.88 +53:56:10.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:24:44.88 +53:56:10.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:24:44.88 +53:56:10.0: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 24 44.88 +53 56 10.0 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,2461280.7058,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.54 00:11:25.51 +51:27:46.6
116.60421 -10.91653 galactic Cas Second-epoch detections are separated by 5.0" and 6.4 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 | 00:11:25.51 +51:27:46.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:11:25.51 +51:27:46.6: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:11:25.51 +51:27:46.6: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 11 25.51 +51 27 46.6 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
target,2461280.7058,13.54,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.51 23:17:13.51 +56:09:04.4
110.03372 -4.34302 galactic Cas Second-epoch detections are separated by 2.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1997188727843968896 | 23:17:14.58 +56:08:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:13.51 +56:09:04.4: 15.12 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:13.51 +56:09:04.4: 14.77 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.12 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 17 13.51 +56 09 04.4 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
Gaia DR3 1997188727843968896,2461280.7058,13.51,0.05,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
Gaia DR3 1997188727843968896 20260828.2058 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.53 23:42:01.24 +52:33:44.2
112.35690 -8.87833 galactic Cas Second-epoch detections are separated by 4.1" and 6.2 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 | 23:42:01.24 +52:33:44.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:01.24 +52:33:44.2: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:01.24 +52:33:44.2: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 42 01.24 +52 33 44.2 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
target,2461280.7058,13.53,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.60 23:10:20.45 +56:50:57.4
109.40666 -3.34398 galactic Cas Second-epoch detections are separated by 6.3" and 6.4 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 | 23:10:20.45 +56:50:57.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:10:20.45 +56:50:57.4: 15.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:10:20.45 +56:50:57.4: 14.61 +/- 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 08 28.2058* 23 10 20.45 +56 50 57.4 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
target,2461280.7058,13.60,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 13.66 23:24:13.25 +57:04:21.3
111.25743 -3.80905 galactic Cas Second-epoch detections are separated by 1.2" and 6.2 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 | 23:24:13.25 +57:04:21.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:13.25 +57:04:21.3: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:13.25 +57:04:21.3: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 24 13.25 +57 04 21.3 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
target,2461280.7058,13.66,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.72 23:13:11.90 +55:44:22.2
109.35680 -4.52137 galactic Cas Second-epoch detections are separated by 7.8" and 6.4 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 J348.3153+55.7412 | 23:13:11.90 +55:44:22.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:13:11.90 +55:44:22.2: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:13:11.90 +55:44:22.2: 14.75 +/- 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 08 28.2058* 23 13 11.90 +55 44 22.2 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 J348.3153+55.7412,2461280.7058,13.72,0.05,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
ATO J348.3153+55.7412 20260828.2058 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.66 23:13:46.75 +55:05:40.2
109.19399 -5.15105 galactic Cas Second-epoch detections are separated by 4.4" and 6.5 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 | 23:13:46.75 +55:05:40.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:13:46.75 +55:05:40.2: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:13:46.75 +55:05:40.2: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 13 46.75 +55 05 40.2 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
target,2461280.7058,13.66,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.79 23:57:03.64 +52:12:14.7
114.52680 -9.77802 galactic Cas Second-epoch detections are separated by 5.4" and 6.4 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 | 23:57:03.64 +52:12:14.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:03.64 +52:12:14.7: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:03.64 +52:12:14.7: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 57 03.64 +52 12 14.7 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,2461280.7058,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.62 23:43:56.31 +50:48:29.6
112.17465 -10.64829 galactic Cas Second-epoch detections are separated by 6.0" and 6.8 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 | 23:43:56.31 +50:48:29.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:43:56.31 +50:48:29.6: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:43:56.31 +50:48:29.6: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 43 56.31 +50 48 29.6 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,2461280.7058,13.62,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.73 23:13:43.46 +55:17:10.3
109.25778 -4.97003 galactic Cas Second-epoch detections are separated by 3.7" and 6.6 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 | 23:13:43.46 +55:17:10.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:13:43.46 +55:17:10.3: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:13:43.46 +55:17:10.3: 14.77 +/- 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 08 28.2058* 23 13 43.46 +55 17 10.3 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
target,2461280.7058,13.73,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.82 23:36:56.18 +53:26:38.5
111.86181 -7.81883 galactic Cas Second-epoch detections are separated by 4.5" and 6.5 pix
The object was found in VSX21" Gaia DR3 1993262715411148672
Type: S
# Max. Min./Amp. JD0 Period
16.690 G 17.460 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:56.18 +53:26:38.5: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:56.18 +53:26:38.5: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 36 56.18 +53 26 38.5 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1993262715411148672,2461280.7058,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993262715411148672 20260828.2058 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.82 23:35:07.39 +50:23:49.7
110.69125 -10.65201 galactic And Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J353.7750+50.4068 | 23:35:07.39 +50:23:49.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:07.39 +50:23:49.7: 14.96 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:07.39 +50:23:49.7: 14.99 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.96 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 35 07.39 +50 23 49.7 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
ATO J353.7750+50.4068,2461280.7058,13.82,0.05,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
ATO J353.7750+50.4068 20260828.2058 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.84 23:18:28.53 +51:19:29.9
108.47805 -8.91907 galactic And Second-epoch detections are separated by 3.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:18:28.53 +51:19:29.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:28.53 +51:19:29.9: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:28.53 +51:19:29.9: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 28.53 +51 19 29.9 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.89 00:14:23.52 +53:09:22.5
117.31976 -9.31134 galactic Cas Second-epoch detections are separated by 3.1" and 6.7 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 | 00:14:23.52 +53:09:22.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:14:23.52 +53:09:22.5: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:14:23.52 +53:09:22.5: 15.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 14 23.52 +53 09 22.5 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,2461280.7058,13.89,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.88 23:46:19.77 +51:19:58.5
112.68137 -10.23836 galactic Cas Second-epoch detections are separated by 8.0" and 6.5 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 | 23:46:19.77 +51:19:58.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:46:19.77 +51:19:58.5: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:46:19.77 +51:19:58.5: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 46 19.77 +51 19 58.5 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,2461280.7058,13.88,0.05,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 20260828.2058 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.92 23:17:55.99 +56:24:54.8
110.21988 -4.13116 galactic Cas Second-epoch detections are separated by 3.6" and 6.0 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 | 23:17:55.99 +56:24:54.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:55.99 +56:24:54.8: 15.27 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:55.99 +56:24:54.8: 14.88 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 17 55.99 +56 24 54.8 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.92,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 13.87 23:37:56.65 +56:26:03.7
112.85673 -4.99293 galactic Cas Second-epoch detections are separated by 6.1" and 6.4 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 | 23:37:56.65 +56:26:03.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:56.65 +56:26:03.7: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:56.65 +56:26:03.7: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 37 56.65 +56 26 03.7 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.84 23:15:11.52 +57:21:43.1
110.21004 -3.11315 galactic Cas Second-epoch detections are separated by 3.7" and 6.1 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 | 23:15:11.52 +57:21:43.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:11.52 +57:21:43.1: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:11.52 +57:21:43.1: 14.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 15 11.52 +57 21 43.1 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.90 00:09:56.98 +50:50:46.1
116.27050 -11.48822 galactic Cas Second-epoch detections are separated by 5.0" and 6.5 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 | 00:09:56.98 +50:50:46.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:56.98 +50:50:46.1: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:56.98 +50:50:46.1: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 09 56.98 +50 50 46.1 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,2461280.7058,13.90,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.04 23:14:18.44 +57:19:41.7
110.08644 -3.10099 galactic Cas Second-epoch detections are separated by 7.6" and 6.5 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 | 23:14:18.44 +57:19:41.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:14:18.44 +57:19:41.7: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:18.44 +57:19:41.7: 14.79 +/- 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 08 28.2058* 23 14 18.44 +57 19 41.7 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,2461280.7058,14.04,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.94 00:22:11.58 +52:16:55.0
118.39294 -10.33188 galactic Cas Second-epoch detections are separated by 8.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:22:11.58 +52:16:55.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:22:11.58 +52:16:55.0: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:22:11.58 +52:16:55.0: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 22 11.58 +52 16 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
target,2461280.7058,13.94,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.05 23:26:02.05 +54:34:25.4
110.67454 -6.25282 galactic Cas Second-epoch detections are separated by 5.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J351.4987+54.5628 | 23:26:02.05 +54:34:25.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:02.05 +54:34:25.4: 15.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:02.05 +54:34:25.4: 14.77 +/- 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 08 28.2058* 23 26 02.05 +54 34 25.4 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
ATO J351.4987+54.5628,2461280.7058,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J351.4987+54.5628 20260828.2058 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 13.96 23:19:24.23 +54:26:59.2
109.72152 -6.04429 galactic Cas Second-epoch detections are separated by 7.0" and 6.3 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 J349.8413+54.4406 | 23:19:24.23 +54:26:59.2 (user input) | STOCH (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:24.23 +54:26:59.2: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:24.23 +54:26:59.2: 14.83 +/- 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 08 28.2058* 23 19 24.23 +54 26 59.2 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
ATO J349.8413+54.4406,2461280.7058,13.96,0.05,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
ATO J349.8413+54.4406 20260828.2058 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 08 28.2058 2461280.7058 13.98 23:45:40.78 +51:00:36.0
112.49758 -10.52466 galactic Cas Second-epoch detections are separated by 7.9" and 6.6 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 | 23:45:40.78 +51:00:36.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:40.78 +51:00:36.0: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:40.78 +51:00:36.0: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 45 40.78 +51 00 36.0 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,2461280.7058,13.98,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.05 23:19:13.36 +52:17:54.8
108.93546 -8.04928 galactic And Second-epoch detections are separated by 4.1" and 6.3 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 | 23:19:13.36 +52:17:54.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:13.36 +52:17:54.8: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:13.36 +52:17:54.8: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 13.36 +52 17 54.8 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.02 23:23:12.46 +54:50:18.9
110.37528 -5.86776 galactic Cas Second-epoch detections are separated by 5.3" and 6.4 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 | 23:23:12.46 +54:50:18.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:12.46 +54:50:18.9: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:12.46 +54:50:18.9: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 12.46 +54 50 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
target,2461280.7058,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.02CV 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 08 28.2058 2461280.7058 13.95 23:55:59.18 +52:04:34.3
114.33558 -9.86760 galactic Cas Second-epoch detections are separated by 2.2" and 6.4 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 | 23:55:59.18 +52:04:34.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:55:59.18 +52:04:34.3: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:55:59.18 +52:04:34.3: 15.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 55 59.18 +52 04 34.3 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,2461280.7058,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.12 23:58:37.65 +53:26:04.7
115.02177 -8.62408 galactic Cas Second-epoch detections are separated by 7.8" and 6.6 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 | 23:58:37.65 +53:26:04.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:37.65 +53:26:04.7: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:37.65 +53:26:04.7: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 58 37.65 +53 26 04.7 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,2461280.7058,14.12,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.07 23:23:22.45 +51:40:47.7
109.32632 -8.85034 galactic And Second-epoch detections are separated by 8.4" and 6.4 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 | 23:23:22.45 +51:40:47.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:22.45 +51:40:47.7: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:22.45 +51:40:47.7: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 22.45 +51 40 47.7 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.07,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.12 23:17:53.16 +53:31:56.3
109.18572 -6.82406 galactic Cas Second-epoch detections are separated by 6.6" and 6.4 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 | 23:17:53.16 +53:31:56.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:53.16 +53:31:56.3: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:53.16 +53:31:56.3: 14.92 +/- 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 08 28.2058* 23 17 53.16 +53 31 56.3 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,2461280.7058,14.12,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 13.99 23:34:13.73 +55:20:19.5
112.03802 -5.89150 galactic Cas Second-epoch detections are separated by 1.5" and 6.4 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 | 23:34:13.73 +55:20:19.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:13.73 +55:20:19.5: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:13.73 +55:20:19.5: 14.83 +/- 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 08 28.2058* 23 34 13.73 +55 20 19.5 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,2461280.7058,13.99,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.03 23:19:18.81 +51:15:50.4
108.58024 -9.02247 galactic And Second-epoch detections are separated by 3.8" and 6.5 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 1991528609478611200 | 23:19:17.87 +51:16:31.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:18.81 +51:15:50.4: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:18.81 +51:15:50.4: 14.81 +/- 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 08 28.2058* 23 19 18.81 +51 15 50.4 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991528609478611200,2461280.7058,14.03,0.05,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 1991528609478611200 20260828.2058 14.03CV 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 08 28.2058 2461280.7058 14.11 23:21:29.75 +53:08:48.8
109.55871 -7.37349 galactic And Second-epoch detections are separated by 8.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.3898+53.1477 | 23:21:29.75 +53:08:48.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:29.75 +53:08:48.8: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:29.75 +53:08:48.8: 14.81 +/- 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 08 28.2058* 23 21 29.75 +53 08 48.8 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.3898+53.1477,2461280.7058,14.11,0.05,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 J350.3898+53.1477 20260828.2058 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.01 23:45:18.59 +50:50:13.5
112.39508 -10.67680 galactic Cas Second-epoch detections are separated by 8.7" and 6.7 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 | 23:45:18.59 +50:50:13.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:18.59 +50:50:13.5: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:18.59 +50:50:13.5: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 45 18.59 +50 50 13.5 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,2461280.7058,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.15 23:40:03.08 +50:31:06.4
111.49137 -10.76080 galactic And Second-epoch detections are separated by 3.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:40:03.08 +50:31:06.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:40:03.08 +50:31:06.4: 15.46 +/- 0.29 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:40:03.08 +50:31:06.4: 15.04 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.46 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 40 03.08 +50 31 06.4 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.12 23:22:55.30 +54:14:50.9
110.13584 -6.41040 galactic Cas Second-epoch detections are separated by 7.0" and 6.4 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 | 23:22:55.30 +54:14:50.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:55.30 +54:14:50.9: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:55.30 +54:14:50.9: 14.83 +/- 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 08 28.2058* 23 22 55.30 +54 14 50.9 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.12,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.18 23:20:39.70 +55:02:04.7
110.09684 -5.55892 galactic Cas Second-epoch detections are separated by 5.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:20:39.70 +55:02:04.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:39.70 +55:02:04.7: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:39.70 +55:02:04.7: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 20 39.70 +55 02 04.7 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.11 23:28:08.91 +50:26:16.2
109.62944 -10.27023 galactic And Second-epoch detections are separated by 7.1" and 6.4 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 | 23:28:08.91 +50:26:16.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:08.91 +50:26:16.2: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:08.91 +50:26:16.2: 14.85 +/- 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 08 28.2058* 23 28 08.91 +50 26 16.2 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.11,0.05,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
target 20260828.2058 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.04 23:20:02.13 +49:55:45.5
108.21257 -10.31211 galactic And Second-epoch detections are separated by 6.0" and 6.5 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 | 23:20:02.13 +49:55:45.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:02.13 +49:55:45.5: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:02.13 +49:55:45.5: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 20 02.13 +49 55 45.5 14.0 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,2461280.7058,14.04,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.25 23:20:09.39 +49:57:06.1
108.23909 -10.29798 galactic And Second-epoch detections are separated by 1.5" and 6.6 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 | 23:20:09.39 +49:57:06.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:09.39 +49:57:06.1: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:09.39 +49:57:06.1: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 20 09.39 +49 57 06.1 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.20 23:40:20.54 +54:40:25.9
112.69297 -6.77836 galactic Cas Second-epoch detections are separated by 5.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J355.0644+54.6675 | 23:40:15.60 +54:40:28.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:40:20.54 +54:40:25.9: 15.47 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:40:20.54 +54:40:25.9: 15.05 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.47 +/- 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 08 28.2058* 23 40 20.54 +54 40 25.9 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 J355.0644+54.6675,2461280.7058,14.20,0.05,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 J355.0644+54.6675 20260828.2058 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 08 28.2058 2461280.7058 13.96 23:11:29.53 +55:33:26.0
109.06447 -4.60037 galactic Cas Second-epoch detections are separated by 8.2" and 6.5 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 1996776067387385344 | 23:11:31.80 +55:33:51.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:11:29.53 +55:33:26.0: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:11:29.53 +55:33:26.0: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 11 29.53 +55 33 26.0 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
Gaia DR3 1996776067387385344,2461280.7058,13.96,0.05,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
Gaia DR3 1996776067387385344 20260828.2058 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 08 28.2058 2461280.7058 13.99 23:14:58.79 +55:26:18.0
109.48041 -4.89403 galactic Cas Second-epoch detections are separated by 3.5" and 6.6 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 | 23:14:58.79 +55:26:18.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:14:58.79 +55:26:18.0: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:58.79 +55:26:18.0: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 14 58.79 +55 26 18.0 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,2461280.7058,13.99,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.19 23:20:52.75 +50:30:13.3
108.54488 -9.82111 galactic And Second-epoch detections are separated by 6.7" and 6.3 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 | 23:20:52.75 +50:30:13.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:52.75 +50:30:13.3: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:52.75 +50:30:13.3: 14.80 +/- 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 08 28.2058* 23 20 52.75 +50 30 13.3 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.19,0.05,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 20260828.2058 14.19CV 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 08 28.2058 2461280.7058 14.04 23:30:36.43 +50:51:22.0
110.13960 -9.99700 galactic Cas Second-epoch detections are separated by 4.4" and 6.9 pix
The object was found in VSX15" Gaia DR3 1943288503183172224
Type: ROT
# Max. Min./Amp. JD0 Period
14.880 G 14.920 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:36.43 +50:51:22.0: 15.16 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:36.43 +50:51:22.0: 14.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.16 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 36.43 +50 51 22.0 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
Gaia DR3 1943288503183172224,2461280.7058,14.04,0.05,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
Gaia DR3 1943288503183172224 20260828.2058 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 08 28.2058 2461280.7058 14.16 23:42:07.04 +54:29:32.0
112.89289 -7.02276 galactic Cas Second-epoch detections are separated by 3.9" and 6.6 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 | 23:42:07.04 +54:29:32.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:07.04 +54:29:32.0: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:07.04 +54:29:32.0: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 42 07.04 +54 29 32.0 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.16,0.05,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 20260828.2058 14.16CV 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 08 28.2058 2461280.7058 14.09 00:05:13.07 +51:50:35.0
115.70421 -10.37888 galactic Cas Second-epoch detections are separated by 7.7" and 6.5 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 395642392925365760 | 00:05:15.79 +51:50:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:13.07 +51:50:35.0: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:13.07 +51:50:35.0: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 05 13.07 +51 50 35.0 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395642392925365760,2461280.7058,14.09,0.05,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
Gaia DR3 395642392925365760 20260828.2058 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.12 23:39:43.83 +50:34:48.1
111.45899 -10.68747 galactic And Second-epoch detections are separated by 6.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J354.9429+50.5709 | 23:39:43.83 +50:34:48.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:43.83 +50:34:48.1: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:43.83 +50:34:48.1: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 39 43.83 +50 34 48.1 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.9429+50.5709,2461280.7058,14.12,0.05,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 J354.9429+50.5709 20260828.2058 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 08 28.2058 2461280.7058 14.08 23:30:29.85 +54:34:21.0
111.29120 -6.45959 galactic Cas Second-epoch detections are separated by 6.4" and 6.4 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 | 23:30:29.85 +54:34:21.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:29.85 +54:34:21.0: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:29.85 +54:34:21.0: 14.81 +/- 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 08 28.2058* 23 30 29.85 +54 34 21.0 14.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.08,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.08 23:18:52.90 +51:20:13.1
108.54241 -8.93035 galactic And Second-epoch detections are separated by 7.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:18:52.90 +51:20:13.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:52.90 +51:20:13.1: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:52.90 +51:20:13.1: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 52.90 +51 20 13.1 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.08,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.16 23:31:54.45 +55:25:34.1
111.74825 -5.70924 galactic Cas Second-epoch detections are separated by 3.5" and 6.5 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 | 23:31:54.45 +55:25:34.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:54.45 +55:25:34.1: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:54.45 +55:25:34.1: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 54.45 +55 25 34.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.16,0.05,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 20260828.2058 14.16CV 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 08 28.2058 2461280.7058 14.11 23:18:39.75 +50:05:36.4
108.06191 -10.08057 galactic And Second-epoch detections are separated by 4.9" and 6.8 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 | 23:18:39.75 +50:05:36.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:39.75 +50:05:36.4: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:39.75 +50:05:36.4: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 39.75 +50 05 36.4 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.11,0.05,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
target 20260828.2058 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.37 23:19:38.04 +50:35:21.3
108.38723 -9.67175 galactic And Second-epoch detections are separated by 2.0" and 6.6 pix
The object was found in VSX10" Gaia DR3 1991437113795719552
Type: ROT
# Max. Min./Amp. JD0 Period
15.730 G 15.800 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:38.04 +50:35:21.3: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:38.04 +50:35:21.3: 14.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 38.04 +50 35 21.3 14.4 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
Gaia DR3 1991437113795719552,2461280.7058,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991437113795719552 20260828.2058 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.16 23:33:45.37 +54:02:56.4
111.58689 -7.10279 galactic Cas Second-epoch detections are separated by 7.5" and 6.4 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 | 23:33:45.37 +54:02:56.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:45.37 +54:02:56.4: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:45.37 +54:02:56.4: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 33 45.37 +54 02 56.4 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.16,0.05,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 20260828.2058 14.16CV 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 08 28.2058 2461280.7058 14.17 00:08:59.67 +50:29:49.5
116.05914 -11.80742 galactic Cas Second-epoch detections are separated by 7.8" and 6.7 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 J002.2346+50.4989 | 00:08:59.67 +50:29:49.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:08:59.67 +50:29:49.5: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:08:59.67 +50:29:49.5: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 08 59.67 +50 29 49.5 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.2346+50.4989,2461280.7058,14.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J002.2346+50.4989 20260828.2058 14.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:31:48.80 +49:59:03.6
110.05019 -10.88535 galactic And Second-epoch detections are separated by 6.1" and 6.4 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 | 23:31:48.80 +49:59:03.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:48.80 +49:59:03.6: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:48.80 +49:59:03.6: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 48.80 +49 59 03.6 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.26,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.26 23:18:53.97 +54:28:24.4
109.66086 -5.99643 galactic Cas Second-epoch detections are separated by 2.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J349.7271+54.4820 | 23:18:53.97 +54:28:24.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:53.97 +54:28:24.4: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:53.97 +54:28:24.4: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 53.97 +54 28 24.4 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 J349.7271+54.4820,2461280.7058,14.26,0.05,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
ATO J349.7271+54.4820 20260828.2058 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 08 28.2058 2461280.7058 14.22 23:42:24.64 +53:39:51.6
112.71195 -7.83212 galactic Cas Second-epoch detections are separated by 8.3" and 6.3 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 | 23:42:24.64 +53:39:51.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:24.64 +53:39:51.6: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:24.64 +53:39:51.6: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 42 24.64 +53 39 51.6 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:22:55.83 +53:23:01.2
109.84335 -7.22392 galactic Cas Second-epoch detections are separated by 4.3" and 6.6 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 | 23:22:55.83 +53:23:01.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:55.83 +53:23:01.2: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:55.83 +53:23:01.2: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 22 55.83 +53 23 01.2 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,2461280.7058,14.26,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.22 23:26:17.36 +55:31:52.1
111.02227 -5.35934 galactic Cas Second-epoch detections are separated by 6.2" and 6.5 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 | 23:26:17.36 +55:31:52.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:17.36 +55:31:52.1: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:17.36 +55:31:52.1: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 26 17.36 +55 31 52.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.15 23:20:55.73 +54:36:44.9
109.98692 -5.96848 galactic Cas Second-epoch detections are separated by 2.2" and 6.2 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 | 23:20:55.73 +54:36:44.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:55.73 +54:36:44.9: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:55.73 +54:36:44.9: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 20 55.73 +54 36 44.9 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.18 00:01:38.26 +50:38:25.8
114.91293 -11.45424 galactic Cas Second-epoch detections are separated by 8.1" and 6.4 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 | 00:01:38.26 +50:38:25.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:01:38.26 +50:38:25.8: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:01:38.26 +50:38:25.8: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 01 38.26 +50 38 25.8 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
target,2461280.7058,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:35:28.82 +56:19:45.8
112.49856 -4.99593 galactic Cas Second-epoch detections are separated by 7.1" and 6.3 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 | 23:35:28.82 +56:19:45.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:28.82 +56:19:45.8: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:28.82 +56:19:45.8: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 35 28.82 +56 19 45.8 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,2461280.7058,14.26,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.28 23:37:16.30 +51:29:54.6
111.34636 -9.69717 galactic Cas Second-epoch detections are separated by 7.0" and 6.6 pix
The object was found in VSX21" Gaia DR3 1944820225960906496
Type: ROT
# Max. Min./Amp. JD0 Period
15.250 G 15.290 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:16.30 +51:29:54.6: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:16.30 +51:29:54.6: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 37 16.30 +51 29 54.6 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
Gaia DR3 1944820225960906496,2461280.7058,14.28,0.05,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
Gaia DR3 1944820225960906496 20260828.2058 14.28CV 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 08 28.2058 2461280.7058 14.29 23:30:10.24 +49:54:50.3
109.77218 -10.86986 galactic And Second-epoch detections are separated by 2.1" and 6.8 pix
The object was found in VSX22" Gaia DR3 1942992287878652288
Type: ROT
# Max. Min./Amp. JD0 Period
14.650 G 14.670 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:10.24 +49:54:50.3: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:10.24 +49:54:50.3: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 10.24 +49 54 50.3 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1942992287878652288,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1942992287878652288 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.12 23:22:06.03 +53:17:47.4
109.69606 -7.26386 galactic Cas Second-epoch detections are separated by 8.5" and 6.1 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 | 23:22:06.03 +53:17:47.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:06.03 +53:17:47.4: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:06.03 +53:17:47.4: 14.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 22 06.03 +53 17 47.4 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,2461280.7058,14.12,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.22 23:19:30.68 +55:40:18.3
110.16478 -4.90466 galactic Cas Second-epoch detections are separated by 7.2" and 6.6 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 | 23:19:30.68 +55:40:18.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:30.68 +55:40:18.3: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:30.68 +55:40:18.3: 14.80 +/- 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 08 28.2058* 23 19 30.68 +55 40 18.3 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.21 00:00:42.73 +51:44:33.3
114.98947 -10.34520 galactic Cas Second-epoch detections are separated by 5.7" and 6.8 pix
The object was found in VSX23" Gaia DR3 395602844869051392
Type: ROT
# Max. Min./Amp. JD0 Period
13.830 G 13.870 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:00:42.73 +51:44:33.3: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:00:42.73 +51:44:33.3: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 00 42.73 +51 44 33.3 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 395602844869051392,2461280.7058,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 395602844869051392 20260828.2058 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.33 23:40:46.84 +50:21:18.3
111.55905 -10.94989 galactic And Second-epoch detections are separated by 1.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:40:46.84 +50:21:18.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:40:46.84 +50:21:18.3: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:40:46.84 +50:21:18.3: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 40 46.84 +50 21 18.3 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.32 23:30:11.92 +56:22:07.2
111.80999 -4.73871 galactic Cas Second-epoch detections are separated by 3.1" and 6.6 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 | 23:30:11.92 +56:22:07.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:11.92 +56:22:07.2: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:11.92 +56:22:07.2: 14.92 +/- 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 08 28.2058* 23 30 11.92 +56 22 07.2 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,2461280.7058,14.32,0.05,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
target 20260828.2058 14.32CV 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 08 28.2058 2461280.7058 14.27 23:18:58.56 +54:09:25.0
109.55945 -6.29665 galactic Cas Second-epoch detections are separated by 7.5" and 6.3 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 J349.7438+54.1510 | 23:18:58.56 +54:09:25.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:58.56 +54:09:25.0: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:58.56 +54:09:25.0: 14.81 +/- 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 08 28.2058* 23 18 58.56 +54 09 25.0 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 J349.7438+54.1510,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.7438+54.1510 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.30 23:25:40.16 +54:34:40.4
110.62565 -6.23161 galactic Cas Second-epoch detections are separated by 4.5" and 6.6 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 | 23:25:40.16 +54:34:40.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:25:40.16 +54:34:40.4: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:25:40.16 +54:34:40.4: 14.73 +/- 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 08 28.2058* 23 25 40.16 +54 34 40.4 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,2461280.7058,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.15 23:36:13.21 +51:20:23.4
111.14058 -9.80167 galactic Cas Second-epoch detections are separated by 5.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:36:13.21 +51:20:23.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:13.21 +51:20:23.4: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:13.21 +51:20:23.4: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 36 13.21 +51 20 23.4 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.11 23:23:02.09 +51:27:45.7
109.20169 -9.03691 galactic And Second-epoch detections are separated by 8.3" and 6.4 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 J350.7452+51.4677 | 23:23:02.09 +51:27:45.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:02.09 +51:27:45.7: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:02.09 +51:27:45.7: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 23 02.09 +51 27 45.7 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.7452+51.4677,2461280.7058,14.11,0.05,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 J350.7452+51.4677 20260828.2058 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.29 23:31:12.32 +50:01:53.6
109.97050 -10.81020 galactic And Second-epoch detections are separated by 3.7" and 6.8 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 | 23:31:12.32 +50:01:53.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:12.32 +50:01:53.6: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:12.32 +50:01:53.6: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 12.32 +50 01 53.6 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.20 23:48:55.40 +52:57:31.1
113.48107 -8.76215 galactic Cas Second-epoch detections are separated by 4.6" and 6.5 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 J357.2472+52.9613 | 23:48:55.40 +52:57:31.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:55.40 +52:57:31.1: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:55.40 +52:57:31.1: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 48 55.40 +52 57 31.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.2472+52.9613,2461280.7058,14.20,0.05,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 J357.2472+52.9613 20260828.2058 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 08 28.2058 2461280.7058 14.21 23:20:22.98 +50:39:45.9
108.52622 -9.64457 galactic And Second-epoch detections are separated by 6.3" and 6.7 pix
The object was found in VSX 2" Gaia DR3 1991438488185587712
Type: S
# Max. Min./Amp. JD0 Period
16.160 G 16.660 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:22.98 +50:39:45.9: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:22.98 +50:39:45.9: 14.92 +/- 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 08 28.2058* 23 20 22.98 +50 39 45.9 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1991438488185587712,2461280.7058,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1991438488185587712 20260828.2058 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.32 23:49:21.12 +50:23:22.7
112.91339 -11.27048 galactic Cas Second-epoch detections are separated by 7.3" and 6.7 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 | 23:49:21.12 +50:23:22.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:49:21.12 +50:23:22.7: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:49:21.12 +50:23:22.7: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 49 21.12 +50 23 22.7 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,2461280.7058,14.32,0.05,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
target 20260828.2058 14.32CV 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 08 28.2058 2461280.7058 14.16 00:24:27.13 +54:50:40.5
119.01687 -7.82190 galactic Cas Second-epoch detections are separated by 4.7" and 6.7 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 419672872389944064 | 00:24:27.63 +54:51:19.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:24:27.13 +54:50:40.5: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:24:27.13 +54:50:40.5: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 24 27.13 +54 50 40.5 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 419672872389944064,2461280.7058,14.16,0.05,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 419672872389944064 20260828.2058 14.16CV 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 08 28.2058 2461280.7058 14.28 00:08:31.57 +52:43:57.6
116.36776 -9.59130 galactic Cas Second-epoch detections are separated by 6.9" and 6.4 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 | 00:08:31.57 +52:43:57.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:08:31.57 +52:43:57.6: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:08:31.57 +52:43:57.6: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 08 31.57 +52 43 57.6 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,2461280.7058,14.28,0.05,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 20260828.2058 14.28CV 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 08 28.2058 2461280.7058 14.38 23:49:17.93 +50:14:11.3
112.86703 -11.41700 galactic Cas Second-epoch detections are separated by 4.0" and 6.1 pix
The object was found in VSX18" Gaia DR3 1943894986926043008
Type: ROT
# Max. Min./Amp. JD0 Period
14.310 G 14.350 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:49:17.93 +50:14:11.3: 15.60 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:49:17.93 +50:14:11.3: 15.07 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.60 +/- 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 08 28.2058* 23 49 17.93 +50 14 11.3 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
Gaia DR3 1943894986926043008,2461280.7058,14.38,0.05,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 1943894986926043008 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.27 23:20:41.10 +49:38:25.8
108.20956 -10.61934 galactic And Second-epoch detections are separated by 5.1" and 6.6 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 | 23:20:41.10 +49:38:25.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:41.10 +49:38:25.8: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:41.10 +49:38:25.8: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 20 41.10 +49 38 25.8 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.20 23:37:28.30 +55:09:05.4
112.42824 -6.20467 galactic Cas Second-epoch detections are separated by 3.1" and 6.4 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 J354.3880+55.1572 | 23:37:28.30 +55:09:05.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:28.30 +55:09:05.4: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:28.30 +55:09:05.4: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 37 28.30 +55 09 05.4 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 J354.3880+55.1572,2461280.7058,14.20,0.05,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 J354.3880+55.1572 20260828.2058 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 08 28.2058 2461280.7058 14.13 23:22:43.60 +51:19:45.4
109.11001 -9.14607 galactic And Second-epoch detections are separated by 7.9" and 6.6 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 | 23:22:43.60 +51:19:45.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:43.60 +51:19:45.4: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:43.60 +51:19:45.4: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 22 43.60 +51 19 45.4 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.13,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.21 23:37:26.45 +50:09:49.4
110.98245 -10.98332 galactic And Second-epoch detections are separated by 6.8" and 6.5 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 | 23:37:26.45 +50:09:49.4 (user input) | T | P | (position from user input) J-Ks=0.883+/-0.170 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:26.45 +50:09:49.4: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:26.45 +50:09:49.4: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 37 26.45 +50 09 49.4 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.34 23:16:32.51 +55:23:17.9
109.66961 -5.02094 galactic Cas Second-epoch detections are separated by 5.2" and 6.1 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 J349.1405+55.3946 | 23:16:32.51 +55:23:17.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.091+/-0.260 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:16:32.51 +55:23:17.9: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:16:32.51 +55:23:17.9: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 16 32.51 +55 23 17.9 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.1405+55.3946,2461280.7058,14.34,0.05,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
ATO J349.1405+55.3946 20260828.2058 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 08 28.2058 2461280.7058 14.36 23:25:13.81 +51:29:54.3
109.53994 -9.11779 galactic And Second-epoch detections are separated by 3.7" and 6.8 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 | 23:25:13.81 +51:29:54.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:25:13.81 +51:29:54.3: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:25:13.81 +51:29:54.3: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 25 13.81 +51 29 54.3 14.4 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,2461280.7058,14.36,0.05,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 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.33 23:32:19.47 +55:17:56.4
111.76622 -5.84837 galactic Cas Second-epoch detections are separated by 8.3" and 6.7 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 | 23:32:19.47 +55:17:56.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:19.47 +55:17:56.4: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:19.47 +55:17:56.4: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 32 19.47 +55 17 56.4 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,2461280.7058,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.34 23:59:59.89 +53:02:02.6
115.14268 -9.05797 galactic Cas Second-epoch detections are separated by 5.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:59:59.89 +53:02:02.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:59:59.89 +53:02:02.6: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:59:59.89 +53:02:02.6: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 59 59.89 +53 02 02.6 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,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.39 23:34:38.18 +52:09:25.3
111.14635 -8.94852 galactic Cas Second-epoch detections are separated by 5.2" and 6.6 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 | 23:34:38.18 +52:09:25.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:38.18 +52:09:25.3: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:38.18 +52:09:25.3: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 38.18 +52 09 25.3 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
target,2461280.7058,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.29 23:40:24.59 +51:36:30.4
111.85266 -9.72887 galactic Cas Second-epoch detections are separated by 1.7" and 6.7 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 | 23:40:24.59 +51:36:30.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:40:24.59 +51:36:30.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:40:24.59 +51:36:30.4: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 40 24.59 +51 36 30.4 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,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:45:27.28 +54:31:03.7
113.37084 -7.12456 galactic Cas Second-epoch detections are separated by 5.1" and 6.5 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 | 23:45:27.28 +54:31:03.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:27.28 +54:31:03.7: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:27.28 +54:31:03.7: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 45 27.28 +54 31 03.7 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,2461280.7058,14.26,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.34 23:44:12.54 +51:12:02.8
112.32108 -10.28063 galactic Cas Second-epoch detections are separated by 8.2" and 6.6 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 | 23:44:12.54 +51:12:02.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:44:12.54 +51:12:02.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:44:12.54 +51:12:02.8: 15.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 44 12.54 +51 12 02.8 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,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.24 23:59:42.82 +53:21:57.0
115.16795 -8.72440 galactic Cas Second-epoch detections are separated by 8.2" and 6.5 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 | 23:59:42.82 +53:21:57.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:59:42.82 +53:21:57.0: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:59:42.82 +53:21:57.0: 15.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 59 42.82 +53 21 57.0 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.31 23:33:42.34 +53:53:39.6
111.53324 -7.24819 galactic Cas Second-epoch detections are separated by 7.0" and 6.3 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 | 23:33:42.34 +53:53:39.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:42.34 +53:53:39.6: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:42.34 +53:53:39.6: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 33 42.34 +53 53 39.6 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,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.24 23:26:38.84 +55:07:00.1
110.93577 -5.76793 galactic Cas Second-epoch detections are separated by 8.8" and 6.3 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 | 23:26:38.84 +55:07:00.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:26:38.84 +55:07:00.1: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:38.84 +55:07:00.1: 14.85 +/- 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 08 28.2058* 23 26 38.84 +55 07 00.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.39 00:13:23.95 +51:50:59.6
116.97260 -10.58118 galactic Cas Second-epoch detections are separated by 7.2" and 6.7 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 | 00:13:23.95 +51:50:59.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:13:23.95 +51:50:59.6: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:13:23.95 +51:50:59.6: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 13 23.95 +51 50 59.6 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,2461280.7058,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.27 23:40:53.24 +53:47:05.7
112.52573 -7.65531 galactic Cas Second-epoch detections are separated by 8.0" and 6.4 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 | 23:40:53.24 +53:47:05.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:40:53.24 +53:47:05.7: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:40:53.24 +53:47:05.7: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 40 53.24 +53 47 05.7 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,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.29 23:22:01.22 +53:10:19.2
109.64187 -7.37680 galactic And Second-epoch detections are separated by 7.4" and 6.8 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 | 23:22:01.22 +53:10:19.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:01.22 +53:10:19.2: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:01.22 +53:10:19.2: 14.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 22 01.22 +53 10 19.2 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.29 23:31:14.34 +51:34:01.0
110.45905 -9.35209 galactic Cas Second-epoch detections are separated by 7.1" and 6.5 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 J352.8113+51.5553 | 23:31:14.34 +51:34:01.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:14.34 +51:34:01.0: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:14.34 +51:34:01.0: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 14.34 +51 34 01.0 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 J352.8113+51.5553,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.8113+51.5553 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:39:45.96 +51:11:03.9
111.63556 -10.10854 galactic Cas Second-epoch detections are separated by 5.8" and 6.4 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 1944659589886025984 | 23:39:48.39 +51:11:29.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:45.96 +51:11:03.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:45.96 +51:11:03.9: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 39 45.96 +51 11 03.9 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1944659589886025984,2461280.7058,14.26,0.05,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
Gaia DR3 1944659589886025984 20260828.2058 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 08 28.2058 2461280.7058 14.38 23:30:36.18 +54:38:27.4
111.32714 -6.39924 galactic Cas Second-epoch detections are separated by 2.9" and 6.6 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 | 23:30:36.18 +54:38:27.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:36.18 +54:38:27.4: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:36.18 +54:38:27.4: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 36.18 +54 38 27.4 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,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.38 23:18:17.92 +53:44:14.7
109.31662 -6.65402 galactic Cas Second-epoch detections are separated by 7.1" and 6.5 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 J349.5597+53.7283 | 23:18:17.92 +53:44:14.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:17.92 +53:44:14.7: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:17.92 +53:44:14.7: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 17.92 +53 44 14.7 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 J349.5597+53.7283,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.5597+53.7283 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.35 23:41:40.88 +51:46:14.0
112.08986 -9.62670 galactic Cas Second-epoch detections are separated by 5.7" and 6.4 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 | 23:41:40.88 +51:46:14.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:41:40.88 +51:46:14.0: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:41:40.88 +51:46:14.0: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 41 40.88 +51 46 14.0 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,2461280.7058,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.40 23:38:10.01 +50:55:36.5
111.31693 -10.28509 galactic Cas Second-epoch detections are separated by 6.4" and 6.5 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 | 23:38:10.01 +50:55:36.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:10.01 +50:55:36.5: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:10.01 +50:55:36.5: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 38 10.01 +50 55 36.5 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,2461280.7058,14.40,0.05,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
target 20260828.2058 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 08 28.2058 2461280.7058 14.30 23:19:02.25 +55:54:02.7
110.18248 -4.66682 galactic Cas Second-epoch detections are separated by 8.3" and 6.3 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 | 23:19:02.25 +55:54:02.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:02.25 +55:54:02.7: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:02.25 +55:54:02.7: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 02.25 +55 54 02.7 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,2461280.7058,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.38 00:04:39.10 +50:18:00.2
115.32763 -11.87963 galactic Cas Second-epoch detections are separated by 3.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:04:39.10 +50:18:00.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:04:39.10 +50:18:00.2: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:04:39.10 +50:18:00.2: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 04 39.10 +50 18 00.2 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,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.23 23:29:27.14 +50:48:42.5
109.94970 -9.98175 galactic Cas Second-epoch detections are separated by 1.9" and 6.5 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 J352.3787+50.8163 | 23:29:27.14 +50:48:42.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:27.14 +50:48:42.5: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:29:27.14 +50:48:42.5: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 29 27.14 +50 48 42.5 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J352.3787+50.8163,2461280.7058,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J352.3787+50.8163 20260828.2058 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.32 23:27:53.79 +50:38:36.4
109.65816 -10.06267 galactic And Second-epoch detections are separated by 6.5" and 6.6 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 | 23:27:53.79 +50:38:36.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:53.79 +50:38:36.4: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:53.79 +50:38:36.4: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 27 53.79 +50 38 36.4 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.32,0.05,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
target 20260828.2058 14.32CV 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 08 28.2058 2461280.7058 14.27 23:18:11.41 +54:19:57.5
109.51377 -6.09175 galactic Cas Second-epoch detections are separated by 4.9" and 6.3 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 | 23:18:11.41 +54:19:57.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:11.41 +54:19:57.5: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:11.41 +54:19:57.5: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 11.41 +54 19 57.5 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,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.28 23:35:12.04 +54:13:18.5
111.84201 -7.00022 galactic Cas Second-epoch detections are separated by 3.9" and 6.6 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 | 23:35:12.04 +54:13:18.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:12.04 +54:13:18.5: 15.58 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:12.04 +54:13:18.5: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 35 12.04 +54 13 18.5 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,2461280.7058,14.28,0.05,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 20260828.2058 14.28CV 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 08 28.2058 2461280.7058 14.34 23:22:28.19 +54:17:33.2
110.08872 -6.34567 galactic Cas Second-epoch detections are separated by 6.4" and 6.6 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 | 23:22:28.19 +54:17:33.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:28.19 +54:17:33.2: 15.40 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:28.19 +54:17:33.2: 14.96 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.40 +/- 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 08 28.2058* 23 22 28.19 +54 17 33.2 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,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.33 23:38:09.64 +50:41:37.0
111.24855 -10.50838 galactic Cas Second-epoch detections are separated by 4.4" and 6.4 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 | 23:38:09.64 +50:41:37.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:09.64 +50:41:37.0: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:09.64 +50:41:37.0: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 38 09.64 +50 41 37.0 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,2461280.7058,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.22 23:12:49.41 +54:42:07.9
108.91964 -5.46435 galactic Cas Second-epoch detections are separated by 7.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.2102+54.7117 | 23:12:49.41 +54:42:07.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:49.41 +54:42:07.9: 15.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:49.41 +54:42:07.9: 14.81 +/- 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 08 28.2058* 23 12 49.41 +54 42 07.9 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 J348.2102+54.7117,2461280.7058,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.2102+54.7117 20260828.2058 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.32 23:20:47.45 +49:41:56.4
108.24666 -10.57050 galactic And Second-epoch detections are separated by 3.1" and 6.6 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 | 23:20:47.45 +49:41:56.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:47.45 +49:41:56.4: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:47.45 +49:41:56.4: 14.85 +/- 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 08 28.2058* 23 20 47.45 +49 41 56.4 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.32,0.05,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
target 20260828.2058 14.32CV 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 08 28.2058 2461280.7058 14.28 00:20:06.47 +55:24:13.8
118.45880 -7.19558 galactic Cas Second-epoch detections are separated by 1.5" and 6.4 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 | 00:20:06.47 +55:24:13.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:20:06.47 +55:24:13.8: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:20:06.47 +55:24:13.8: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 20 06.47 +55 24 13.8 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,2461280.7058,14.28,0.05,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 20260828.2058 14.28CV 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 08 28.2058 2461280.7058 14.31 23:37:52.25 +50:23:10.1
111.11442 -10.78995 galactic And Second-epoch detections are separated by 4.3" and 6.5 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 | 23:37:52.25 +50:23:10.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:52.25 +50:23:10.1: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:52.25 +50:23:10.1: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 37 52.25 +50 23 10.1 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.34 23:49:43.32 +50:42:41.7
113.05092 -10.97233 galactic Cas Second-epoch detections are separated by 3.4" and 6.4 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 | 23:49:43.32 +50:42:41.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:49:43.32 +50:42:41.7: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:49:43.32 +50:42:41.7: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 49 43.32 +50 42 41.7 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,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.31 23:50:33.67 +50:47:47.1
113.20287 -10.92177 galactic Cas Second-epoch detections are separated by 6.9" and 6.2 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 | 23:50:33.67 +50:47:47.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:50:33.67 +50:47:47.1: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:50:33.67 +50:47:47.1: 15.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 50 33.67 +50 47 47.1 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,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.33 00:13:12.27 +50:29:47.9
116.73446 -11.91447 galactic Cas Second-epoch detections are separated by 5.2" and 6.8 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 | 00:13:12.27 +50:29:47.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:13:12.27 +50:29:47.9: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:13:12.27 +50:29:47.9: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 13 12.27 +50 29 47.9 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.29 23:17:16.38 +51:02:57.6
108.20006 -9.10905 galactic And Second-epoch detections are separated by 1.4" and 6.5 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 | 23:17:16.38 +51:02:57.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:17:16.38 +51:02:57.6: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:16.38 +51:02:57.6: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 17 16.38 +51 02 57.6 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.25 23:29:56.83 +51:09:25.5
110.13521 -9.67865 galactic Cas Second-epoch detections are separated by 7.0" and 6.6 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 | 23:29:56.83 +51:09:25.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:56.83 +51:09:25.5: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:29:56.83 +51:09:25.5: 14.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 29 56.83 +51 09 25.5 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:34:13.54 +56:18:02.1
112.32313 -4.97250 galactic Cas Second-epoch detections are separated by 7.1" and 6.5 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 | 23:34:13.54 +56:18:02.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:13.54 +56:18:02.1: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:13.54 +56:18:02.1: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 13.54 +56 18 02.1 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,2461280.7058,14.26,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.27 23:36:06.52 +55:53:51.7
112.45718 -5.43449 galactic Cas Second-epoch detections are separated by 4.0" and 6.3 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 | 23:36:06.52 +55:53:51.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:06.52 +55:53:51.7: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:06.52 +55:53:51.7: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 36 06.52 +55 53 51.7 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,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.21 00:03:29.54 +51:28:01.8
115.36608 -10.69888 galactic Cas Second-epoch detections are separated by 3.1" and 6.6 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 | 00:03:29.54 +51:28:01.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:03:29.54 +51:28:01.8: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:03:29.54 +51:28:01.8: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 03 29.54 +51 28 01.8 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
target,2461280.7058,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.38 00:03:44.44 +50:01:24.4
115.12841 -12.12423 galactic Cas Second-epoch detections are separated by 5.3" and 6.6 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 | 00:03:44.44 +50:01:24.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:03:44.44 +50:01:24.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:03:44.44 +50:01:24.4: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 03 44.44 +50 01 24.4 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,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:13:07.51 +56:44:48.1
109.72192 -3.58228 galactic Cas Second-epoch detections are separated by 5.6" and 6.3 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 J348.2939+56.7447 | 23:13:07.51 +56:44:48.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:13:07.51 +56:44:48.1: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:13:07.51 +56:44:48.1: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 13 07.51 +56 44 48.1 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 J348.2939+56.7447,2461280.7058,14.26,0.05,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
ATO J348.2939+56.7447 20260828.2058 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 08 28.2058 2461280.7058 14.44 23:25:12.62 +54:01:38.1
110.38007 -6.72976 galactic Cas Second-epoch detections are separated by 2.5" and 6.6 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 | 23:25:12.62 +54:01:38.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:25:12.62 +54:01:38.1: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:25:12.62 +54:01:38.1: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 25 12.62 +54 01 38.1 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,2461280.7058,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.44CV 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 08 28.2058 2461280.7058 14.26 23:16:30.14 +57:22:30.2
110.37974 -3.16473 galactic Cas Second-epoch detections are separated by 6.4" and 6.4 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 | 23:16:30.14 +57:22:30.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:16:30.14 +57:22:30.2: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:16:30.14 +57:22:30.2: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 16 30.14 +57 22 30.2 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,2461280.7058,14.26,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.35 23:43:52.25 +51:14:12.9
112.27878 -10.23187 galactic Cas Second-epoch detections are separated by 3.4" and 6.7 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 | 23:43:52.25 +51:14:12.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:43:52.25 +51:14:12.9: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:43:52.25 +51:14:12.9: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 43 52.25 +51 14 12.9 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.36 23:22:16.77 +52:07:23.0
109.31780 -8.37620 galactic And Second-epoch detections are separated by 4.1" and 6.4 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 | 23:22:16.77 +52:07:23.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:16.77 +52:07:23.0: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:16.77 +52:07:23.0: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 22 16.77 +52 07 23.0 14.4 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,2461280.7058,14.36,0.05,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 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.38 00:08:00.03 +50:31:24.7
115.90462 -11.75459 galactic Cas Second-epoch detections are separated by 2.7" and 6.8 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 | 00:08:00.03 +50:31:24.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:08:00.03 +50:31:24.7: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:08:00.03 +50:31:24.7: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 08 00.03 +50 31 24.7 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,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.42 00:25:26.11 +53:44:41.0
119.04570 -8.93070 galactic Cas Second-epoch detections are separated by 7.9" and 6.7 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 | 00:25:26.11 +53:44:41.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:25:26.11 +53:44:41.0: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:25:26.11 +53:44:41.0: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 25 26.11 +53 44 41.0 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,2461280.7058,14.42,0.05,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 20260828.2058 14.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.41 23:55:18.97 +53:33:58.1
114.56335 -8.39125 galactic Cas Second-epoch detections are separated by 5.7" and 6.9 pix
The object was found in VSX13" ZTF J235517.92+533407.2
Type: BY
# Max. Min./Amp. JD0 Period
16.642 r Y 0.059 r 2458355.82780 5.195131100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:55:18.97 +53:33:58.1: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:55:18.97 +53:33:58.1: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 55 18.97 +53 33 58.1 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
ZTF J235517.92+533407.2,2461280.7058,14.41,0.05,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
ZTF J235517.92+533407.2 20260828.2058 14.41CV 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 08 28.2058 2461280.7058 14.31 00:13:10.45 +50:30:07.3
116.73042 -11.90841 galactic Cas Second-epoch detections are separated by 3.4" and 6.6 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 J003.2772+50.4947 | 00:13:10.45 +50:30:07.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:13:10.45 +50:30:07.3: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:13:10.45 +50:30:07.3: 14.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 13 10.45 +50 30 07.3 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.2772+50.4947,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J003.2772+50.4947 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.24 23:11:05.31 +56:36:32.0
109.41035 -3.60530 galactic Cas Second-epoch detections are separated by 2.0" and 6.4 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 J347.7826+56.6111 | 23:11:06.96 +56:35:59.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:11:05.31 +56:36:32.0: 15.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:11:05.31 +56:36:32.0: 14.70 +/- 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 08 28.2058* 23 11 05.31 +56 36 32.0 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J347.7826+56.6111,2461280.7058,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.7826+56.6111 20260828.2058 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.24 23:15:48.11 +56:59:18.1
110.15157 -3.49131 galactic Cas Second-epoch detections are separated by 1.3" and 6.1 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 | 23:15:48.11 +56:59:18.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:48.11 +56:59:18.1: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:48.11 +56:59:18.1: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 15 48.11 +56 59 18.1 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.45 23:28:43.61 +56:40:16.9
111.71148 -4.38773 galactic Cas Second-epoch detections are separated by 6.3" and 6.4 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 | 23:28:43.61 +56:40:16.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:43.61 +56:40:16.9: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:43.61 +56:40:16.9: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 28 43.61 +56 40 16.9 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,2461280.7058,14.45,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.51 23:31:25.50 +52:51:49.0
110.89103 -8.12740 galactic Cas Second-epoch detections are separated by 7.3" and 6.6 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 | 23:31:25.50 +52:51:49.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:25.50 +52:51:49.0: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:25.50 +52:51:49.0: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 25.50 +52 51 49.0 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
target,2461280.7058,14.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.48 23:27:34.88 +57:18:22.3
111.76498 -3.73619 galactic Cas Second-epoch detections are separated by 7.4" and 6.3 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 | 23:27:34.88 +57:18:22.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:34.88 +57:18:22.3: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:34.88 +57:18:22.3: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 27 34.88 +57 18 22.3 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
target,2461280.7058,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.34 00:12:57.02 +51:31:46.9
116.85355 -10.88725 galactic Cas Second-epoch detections are separated by 7.9" and 6.7 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 J003.2503+51.5304 | 00:12:57.02 +51:31:46.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:12:57.02 +51:31:46.9: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:12:57.02 +51:31:46.9: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 12 57.02 +51 31 46.9 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J003.2503+51.5304,2461280.7058,14.34,0.05,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
ATO J003.2503+51.5304 20260828.2058 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 08 28.2058 2461280.7058 14.19 23:15:39.64 +52:17:05.5
108.41706 -7.86690 galactic And Second-epoch detections are separated by 4.6" and 6.7 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 J348.8986+52.2905 | 23:15:39.64 +52:17:05.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:39.64 +52:17:05.5: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:39.64 +52:17:05.5: 14.76 +/- 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 08 28.2058* 23 15 39.64 +52 17 05.5 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.8986+52.2905,2461280.7058,14.19,0.05,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 J348.8986+52.2905 20260828.2058 14.19CV 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 08 28.2058 2461280.7058 14.31 00:12:14.63 +53:43:20.0
117.08498 -8.70398 galactic Cas Second-epoch detections are separated by 6.5" and 6.6 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 | 00:12:14.63 +53:43:20.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:12:14.63 +53:43:20.0: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:12:14.63 +53:43:20.0: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 12 14.63 +53 43 20.0 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,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.39 00:09:18.60 +53:05:18.0
116.54588 -9.26026 galactic Cas Second-epoch detections are separated by 2.2" and 6.4 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 | 00:09:18.60 +53:05:18.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:18.60 +53:05:18.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:18.60 +53:05:18.0: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 09 18.60 +53 05 18.0 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,2461280.7058,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.39 00:24:08.76 +50:06:52.4
118.45611 -12.51986 galactic Cas Second-epoch detections are separated by 2.9" and 6.8 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 | 00:24:08.76 +50:06:52.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:24:08.76 +50:06:52.4: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:24:08.76 +50:06:52.4: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 24 08.76 +50 06 52.4 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,2461280.7058,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.32 00:18:53.29 +52:28:12.8
117.90750 -10.08370 galactic Cas Second-epoch detections are separated by 4.6" and 6.6 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 | 00:18:53.29 +52:28:12.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:18:53.29 +52:28:12.8: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:18:53.29 +52:28:12.8: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 18 53.29 +52 28 12.8 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,2461280.7058,14.32,0.05,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
target 20260828.2058 14.32CV 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 08 28.2058 2461280.7058 14.50 23:29:01.56 +50:30:26.5
109.78647 -10.24902 galactic And Second-epoch detections are separated by 3.6" and 6.4 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 | 23:29:01.56 +50:30:26.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:01.56 +50:30:26.5: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:29:01.56 +50:30:26.5: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 29 01.56 +50 30 26.5 14.5 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,2461280.7058,14.50,0.05,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 20260828.2058 14.50CV 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 08 28.2058 2461280.7058 14.36 23:44:26.65 +52:35:34.9
112.72456 -8.94593 galactic Cas Second-epoch detections are separated by 8.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1944988519961581696 | 23:44:21.73 +52:35:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:44:26.65 +52:35:34.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:44:26.65 +52:35:34.9: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 44 26.65 +52 35 34.9 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 1944988519961581696,2461280.7058,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1944988519961581696 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.39 23:28:53.48 +49:44:55.5
109.51956 -10.96115 galactic And Second-epoch detections are separated by 8.4" and 6.2 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 | 23:28:53.48 +49:44:55.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:53.48 +49:44:55.5: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:53.48 +49:44:55.5: 14.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 28 53.48 +49 44 55.5 14.4 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,2461280.7058,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.34 23:19:01.95 +55:54:17.3
110.18325 -4.66277 galactic Cas Second-epoch detections are separated by 6.2" and 6.2 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 | 23:19:01.95 +55:54:17.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:01.95 +55:54:17.3: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:01.95 +55:54:17.3: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 01.95 +55 54 17.3 14.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.26 23:44:40.46 +54:40:58.5
113.30340 -6.93591 galactic Cas Second-epoch detections are separated by 6.1" and 6.4 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 | 23:44:40.46 +54:40:58.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:44:40.46 +54:40:58.5: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:44:40.46 +54:40:58.5: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 44 40.46 +54 40 58.5 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,2461280.7058,14.26,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.39 23:32:25.39 +57:31:51.7
112.45585 -3.72471 galactic Cas Second-epoch detections are separated by 8.4" and 6.2 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 | 23:32:25.39 +57:31:51.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:25.39 +57:31:51.7: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:25.39 +57:31:51.7: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 32 25.39 +57 31 51.7 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,2461280.7058,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.38 00:09:56.28 +51:29:47.0
116.37693 -10.84640 galactic Cas Second-epoch detections are separated by 4.2" and 6.6 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 J002.5058+51.4813 | 00:09:57.31 +51:29:02.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:56.28 +51:29:47.0: 15.60 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:56.28 +51:29:47.0: 15.07 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.60 +/- 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 08 28.2058* 00 09 56.28 +51 29 47.0 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 J002.5058+51.4813,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J002.5058+51.4813 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.35 23:22:04.92 +50:07:50.1
108.59686 -10.23759 galactic And Second-epoch detections are separated by 4.1" and 6.5 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 | 23:22:04.92 +50:07:50.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:04.92 +50:07:50.1: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:04.92 +50:07:50.1: 14.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 22 04.92 +50 07 50.1 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.43 23:34:48.44 +54:22:16.9
111.83096 -6.84041 galactic Cas Second-epoch detections are separated by 8.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1994309622285951232 | 23:34:52.04 +54:22:07.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:48.44 +54:22:16.9: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:48.44 +54:22:16.9: 14.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 48.44 +54 22 16.9 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 1994309622285951232,2461280.7058,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1994309622285951232 20260828.2058 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.38 23:42:43.39 +53:34:06.0
112.73128 -7.93699 galactic Cas Second-epoch detections are separated by 2.2" and 6.6 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 | 23:42:43.39 +53:34:06.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:43.39 +53:34:06.0: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:43.39 +53:34:06.0: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 42 43.39 +53 34 06.0 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,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.34 23:52:19.18 +54:21:38.8
114.30899 -7.51821 galactic Cas Second-epoch detections are separated by 4.2" and 6.6 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 | 23:52:19.18 +54:21:38.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:52:19.18 +54:21:38.8: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:52:19.18 +54:21:38.8: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 52 19.18 +54 21 38.8 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,2461280.7058,14.34,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.31 23:34:55.94 +51:11:11.8
110.89946 -9.88899 galactic Cas Second-epoch detections are separated by 2.0" and 6.1 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 | 23:34:55.94 +51:11:11.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:55.94 +51:11:11.8: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:55.94 +51:11:11.8: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 55.94 +51 11 11.8 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,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.36 23:34:27.35 +56:45:26.0
112.48864 -4.54551 galactic Cas Second-epoch detections are separated by 1.6" and 6.3 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 | 23:34:27.35 +56:45:26.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:27.35 +56:45:26.0: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:27.35 +56:45:26.0: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 27.35 +56 45 26.0 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,2461280.7058,14.36,0.05,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 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.50 23:19:02.46 +54:30:07.8
109.69035 -5.97676 galactic Cas Second-epoch detections are separated by 3.7" and 6.8 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 | 23:19:02.46 +54:30:07.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:02.46 +54:30:07.8: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:02.46 +54:30:07.8: 14.83 +/- 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 08 28.2058* 23 19 02.46 +54 30 07.8 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
target,2461280.7058,14.50,0.05,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 20260828.2058 14.50CV 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 08 28.2058 2461280.7058 14.36 23:31:20.91 +52:54:38.0
110.89452 -8.07918 galactic Cas Second-epoch detections are separated by 6.8" and 6.4 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 J352.8199+52.9052 | 23:31:20.91 +52:54:38.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:20.91 +52:54:38.0: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:20.91 +52:54:38.0: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 31 20.91 +52 54 38.0 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 J352.8199+52.9052,2461280.7058,14.36,0.05,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 J352.8199+52.9052 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.37 23:54:30.23 +54:01:29.4
114.54685 -7.91741 galactic Cas Second-epoch detections are separated by 4.2" and 6.6 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 1993574044704001792 | 23:54:34.92 +54:01:22.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:54:30.23 +54:01:29.4: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:54:30.23 +54:01:29.4: 15.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 54 30.23 +54 01 29.4 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 1993574044704001792,2461280.7058,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1993574044704001792 20260828.2058 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.50 23:48:22.59 +53:58:07.2
113.64964 -7.76268 galactic Cas Second-epoch detections are separated by 7.4" and 6.7 pix
The object was found in VSX17" Gaia DR3 1993699595190662400
Type: E
# Max. Min./Amp. JD0 Period
19.030 G 20.050 G 0.966280000000
ATTENTION: measured mag 14.50 is 4.5 mag brighter than the VSX record maximum brightness 19.03 - 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_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:22.59 +53:58:07.2: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:22.59 +53:58:07.2: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 48 22.59 +53 58 07.2 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 1993699595190662400,2461280.7058,14.50,0.05,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
Gaia DR3 1993699595190662400 20260828.2058 14.50CV 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 08 28.2058 2461280.7058 14.34 23:39:48.32 +51:17:42.2
111.67280 -10.00397 galactic Cas Second-epoch detections are separated by 7.6" and 6.6 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 J354.9427+51.2894 | 23:39:48.32 +51:17:42.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:48.32 +51:17:42.2: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:48.32 +51:17:42.2: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 39 48.32 +51 17 42.2 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 J354.9427+51.2894,2461280.7058,14.34,0.05,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
ATO J354.9427+51.2894 20260828.2058 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 08 28.2058 2461280.7058 14.30 00:24:43.89 +53:17:18.5
118.89252 -9.37369 galactic Cas Second-epoch detections are separated by 5.4" and 6.6 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 419469497101020288 | 00:24:47.43 +53:16:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:24:43.89 +53:17:18.5: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:24:43.89 +53:17:18.5: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 24 43.89 +53 17 18.5 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
Gaia DR3 419469497101020288,2461280.7058,14.30,0.05,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
Gaia DR3 419469497101020288 20260828.2058 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.47 23:19:17.20 +52:12:32.3
108.91288 -8.13658 galactic And Second-epoch detections are separated by 4.0" and 6.6 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 | 23:19:17.20 +52:12:32.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:17.20 +52:12:32.3: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:17.20 +52:12:32.3: 14.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 17.20 +52 12 32.3 14.5 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,2461280.7058,14.47,0.05,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 20260828.2058 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.31 23:20:56.42 +53:10:52.9
109.49186 -7.31247 galactic And Second-epoch detections are separated by 4.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.2255+53.1761 | 23:20:56.42 +53:10:52.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:56.42 +53:10:52.9: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:56.42 +53:10:52.9: 14.92 +/- 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 08 28.2058* 23 20 56.42 +53 10 52.9 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J350.2255+53.1761,2461280.7058,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J350.2255+53.1761 20260828.2058 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.46 23:44:37.70 +51:40:35.6
112.51106 -9.83831 galactic Cas Second-epoch detections are separated by 7.7" and 6.7 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 | 23:44:37.70 +51:40:35.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:44:37.70 +51:40:35.6: 15.42 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:44:37.70 +51:40:35.6: 15.06 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.42 +/- 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 08 28.2058* 23 44 37.70 +51 40 35.6 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
target,2461280.7058,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.44 23:19:27.23 +51:48:29.4
108.79475 -8.52082 galactic And Second-epoch detections are separated by 8.4" and 6.7 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 | 23:19:27.23 +51:48:29.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:27.23 +51:48:29.4: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:27.23 +51:48:29.4: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 27.23 +51 48 29.4 14.4 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,2461280.7058,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.44CV 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 08 28.2058 2461280.7058 14.38 23:21:03.75 +49:30:36.1
108.22164 -10.76296 galactic And Second-epoch detections are separated by 2.0" and 6.5 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 | 23:21:03.75 +49:30:36.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:03.75 +49:30:36.1: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:03.75 +49:30:36.1: 14.79 +/- 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 08 28.2058* 23 21 03.75 +49 30 36.1 14.4 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,2461280.7058,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.39 23:22:36.33 +49:57:50.0
108.61901 -10.42300 galactic And Second-epoch detections are separated by 7.9" and 6.4 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 | 23:22:36.33 +49:57:50.0 (user input) | T | P | (position from user input) J-Ks=0.182+/-0.203 (F)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:36.33 +49:57:50.0: 15.48 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:36.33 +49:57:50.0: 14.88 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.48 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 22 36.33 +49 57 50.0 14.4 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,2461280.7058,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.36 23:33:09.14 +52:28:51.3
111.02533 -8.57165 galactic Cas Second-epoch detections are separated by 5.4" and 6.4 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 | 23:33:09.14 +52:28:51.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:09.14 +52:28:51.3: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:09.14 +52:28:51.3: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 33 09.14 +52 28 51.3 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
target,2461280.7058,14.36,0.05,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 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.50 23:36:25.62 +50:36:51.0
110.95765 -10.50539 galactic And Second-epoch detections are separated by 6.4" and 6.6 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 1944536307143365248 | 23:36:30.53 +50:36:50.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:25.62 +50:36:51.0: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:25.62 +50:36:51.0: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 36 25.62 +50 36 51.0 14.5 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
Gaia DR3 1944536307143365248,2461280.7058,14.50,0.05,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
Gaia DR3 1944536307143365248 20260828.2058 14.50CV 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 08 28.2058 2461280.7058 14.51 23:43:28.60 +51:58:13.4
112.41482 -9.50816 galactic Cas Second-epoch detections are separated by 6.7" and 6.4 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 | 23:43:28.60 +51:58:13.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:43:28.60 +51:58:13.4: 15.53 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:43:28.60 +51:58:13.4: 15.05 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.53 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 43 28.60 +51 58 13.4 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
target,2461280.7058,14.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.36 23:30:33.53 +51:17:36.4
110.27077 -9.57913 galactic Cas Second-epoch detections are separated by 5.6" and 6.6 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 | 23:30:33.53 +51:17:36.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:33.53 +51:17:36.4: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:30:33.53 +51:17:36.4: 14.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 30 33.53 +51 17 36.4 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,2461280.7058,14.36,0.05,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 20260828.2058 14.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.23 23:40:12.45 +51:49:27.7
111.88248 -9.51268 galactic Cas Second-epoch detections are separated by 3.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:40:12.45 +51:49:27.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:40:12.45 +51:49:27.7: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:40:12.45 +51:49:27.7: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 40 12.45 +51 49 27.7 14.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461280.7058,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.48 23:35:09.83 +51:10:28.4
110.93103 -9.91123 galactic Cas Second-epoch detections are separated by 2.8" and 6.5 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 | 23:35:09.83 +51:10:28.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:09.83 +51:10:28.4: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:09.83 +51:10:28.4: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 35 09.83 +51 10 28.4 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
target,2461280.7058,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.41 23:19:01.25 +51:51:44.9
108.75080 -8.44643 galactic And Second-epoch detections are separated by 4.5" and 6.0 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 | 23:19:01.25 +51:51:44.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:01.25 +51:51:44.9: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:19:01.25 +51:51:44.9: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 19 01.25 +51 51 44.9 14.4 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,2461280.7058,14.41,0.05,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 20260828.2058 14.41CV 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 08 28.2058 2461280.7058 14.43 23:34:34.54 +50:32:21.8
110.64959 -10.49031 galactic And Second-epoch detections are separated by 6.7" and 6.4 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 | 23:34:34.54 +50:32:21.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:34.54 +50:32:21.8: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:34.54 +50:32:21.8: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 34.54 +50 32 21.8 14.4 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,2461280.7058,14.43,0.05,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 20260828.2058 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.45 23:24:33.15 +53:38:51.1
110.16137 -7.05605 galactic Cas Second-epoch detections are separated by 6.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:24:33.15 +53:38:51.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:33.15 +53:38:51.1: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:33.15 +53:38:51.1: 14.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 24 33.15 +53 38 51.1 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,2461280.7058,14.45,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 14.46 23:18:19.31 +56:04:31.1
110.15006 -4.46822 galactic Cas Second-epoch detections are separated by 5.4" and 6.2 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 J349.5575+56.0737 | 23:18:19.31 +56:04:31.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:19.31 +56:04:31.1: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:19.31 +56:04:31.1: 14.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 18 19.31 +56 04 31.1 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
ATO J349.5575+56.0737,2461280.7058,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.5575+56.0737 20260828.2058 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.47 23:52:18.62 +50:33:10.0
113.41908 -11.22364 galactic Cas Second-epoch detections are separated by 7.4" and 6.7 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 | 23:52:18.62 +50:33:10.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:52:18.62 +50:33:10.0: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:52:18.62 +50:33:10.0: 15.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 52 18.62 +50 33 10.0 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
target,2461280.7058,14.47,0.05,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 20260828.2058 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.41 00:07:28.60 +51:49:30.6
116.05021 -10.45822 galactic Cas Second-epoch detections are separated by 3.6" and 6.5 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 | 00:07:28.60 +51:49:30.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:07:28.60 +51:49:30.6: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:07:28.60 +51:49:30.6: 15.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 07 28.60 +51 49 30.6 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,2461280.7058,14.41,0.05,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 20260828.2058 14.41CV 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 08 28.2058 2461280.7058 14.55 23:38:18.43 +54:09:41.6
112.26319 -7.18839 galactic Cas Second-epoch detections are separated by 6.2" and 6.6 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 J354.5928+54.1628 | 23:38:18.43 +54:09:41.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:18.43 +54:09:41.6: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:18.43 +54:09:41.6: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 38 18.43 +54 09 41.6 14.6 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 J354.5928+54.1628,2461280.7058,14.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.5928+54.1628 20260828.2058 14.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.27 00:22:29.93 +51:55:46.7
118.39933 -10.68724 galactic Cas Second-epoch detections are separated by 5.6" and 6.5 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 | 00:22:29.93 +51:55:46.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:22:29.93 +51:55:46.7: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:22:29.93 +51:55:46.7: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 22 29.93 +51 55 46.7 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,2461280.7058,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.42 23:58:42.03 +52:17:51.8
114.79571 -9.73894 galactic Cas Second-epoch detections are separated by 5.6" and 6.6 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 | 23:58:42.03 +52:17:51.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:42.03 +52:17:51.8: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:42.03 +52:17:51.8: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 58 42.03 +52 17 51.8 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
target,2461280.7058,14.42,0.05,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 20260828.2058 14.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.29 23:09:50.10 +57:19:55.1
109.52744 -2.87157 galactic Cas Second-epoch detections are separated by 3.3" and 6.8 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 | 23:09:50.10 +57:19:55.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:09:50.10 +57:19:55.1: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:09:50.10 +57:19:55.1: 14.81 +/- 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 08 28.2058* 23 09 50.10 +57 19 55.1 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,2461280.7058,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.46 00:26:02.62 +52:49:56.8
119.04407 -9.84750 galactic Cas Second-epoch detections are separated by 8.6" and 6.6 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 J006.5013+52.8257 | 00:26:02.62 +52:49:56.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:26:02.62 +52:49:56.8: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:26:02.62 +52:49:56.8: 14.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 26 02.62 +52 49 56.8 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
ATO J006.5013+52.8257,2461280.7058,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.5013+52.8257 20260828.2058 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.41 23:20:29.03 +54:17:15.4
109.81309 -6.25105 galactic Cas Second-epoch detections are separated by 8.6" and 6.4 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 J350.1161+54.2771 | 23:20:29.03 +54:17:15.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:29.03 +54:17:15.4: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:29.03 +54:17:15.4: 14.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 20 29.03 +54 17 15.4 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 J350.1161+54.2771,2461280.7058,14.41,0.05,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
ATO J350.1161+54.2771 20260828.2058 14.41CV 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 08 28.2058 2461280.7058 14.40 00:26:38.74 +56:33:57.6
119.50187 -6.14055 galactic Cas Second-epoch detections are separated by 4.4" and 6.3 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 J006.6648+56.5610 | 00:26:38.74 +56:33:57.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:26:38.74 +56:33:57.6: 15.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:26:38.74 +56:33:57.6: 14.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 00 26 38.74 +56 33 57.6 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 J006.6648+56.5610,2461280.7058,14.40,0.05,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
ATO J006.6648+56.5610 20260828.2058 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 08 28.2058 2461280.7058 14.54 23:11:03.57 +57:24:20.6
109.70838 -2.86610 galactic Cas Second-epoch detections are separated by 4.1" and 6.2 pix
The object was found in VSX18" ZTF J231101.41+572426.3
Type: VAR
# Max. Min./Amp. JD0 Period
18.104 r Y 0.068 r 2458288.97300 0.143290000000
ATTENTION: measured mag 14.54 is 3.5 mag brighter than the VSX record maximum brightness 18.04 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:11:03.57 +57:24:20.6: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:11:03.57 +57:24:20.6: 14.86 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 11 03.57 +57 24 20.6 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
ZTF J231101.41+572426.3,2461280.7058,14.54,0.05,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
ZTF J231101.41+572426.3 20260828.2058 14.54CV 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 08 28.2058 2461280.7058 14.48 23:21:35.56 +56:30:06.9
110.72535 -4.22554 galactic Cas Second-epoch detections are separated by 4.0" and 6.1 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 | 23:21:35.56 +56:30:06.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:35.56 +56:30:06.9: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:35.56 +56:30:06.9: 14.92 +/- 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 08 28.2058* 23 21 35.56 +56 30 06.9 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
target,2461280.7058,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 28.2058 2461280.7058 14.26 23:16:08.34 +55:39:57.0
109.71654 -4.74151 galactic Cas Second-epoch detections are separated by 4.2" and 6.4 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 | 23:16:08.34 +55:39:57.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:16:08.34 +55:39:57.0: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:16:08.34 +55:39:57.0: 14.80 +/- 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 08 28.2058* 23 16 08.34 +55 39 57.0 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,2461280.7058,14.26,0.05,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 20260828.2058 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 08 28.2058 2461280.7058 13.02 00:19:57.98 +56:35:35.9
118.58557 -6.01262 galactic Cas Second-epoch detections are separated by 2.9" and 6.6 pix
The object was found in VSX12" NSV 15071
Type: M
# Max. Min./Amp. JD0 Period
13.300 V < 17.300 V 2451313.00000 315.000000000000 :
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:19:57.98 +56:35:35.9: 14.90 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:19:57.98 +56:35:35.9: 14.74 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.85 +/- 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 08 28.2058* 00 19 57.98 +56 35 35.9 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
NSV 15071,2461280.7058,13.02,0.05,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
NSV 15071 20260828.2058 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 08 28.2058 2461280.7058 12.38 23:34:04.31 +55:18:58.3
112.00987 -5.90644 galactic Cas Second-epoch detections are separated by 6.4" and 6.4 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 | 23:34:04.31 +55:18:58.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:04.31 +55:18:58.3: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:04.31 +55:18:58.3: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 28.2058* 23 34 04.31 +55 18 58.3 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,2461280.7058,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260828.2058 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461239.82421699 18.07.2026 07:46:42.348 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
First image: 2461239.82421699 18.07.2026 07:46:42.348 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Last image: 2461280.70604080 28.08.2026 04:56:31.925 /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 38
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.76
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 45 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 22744
Objects passed selection criteria: 22733
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: 20646
Average stars matched: 20319 (98.4162 %)
Memory usage VmPeak: 251352 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Aug 28 00:10:22 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461239.82421699 18.07.2026 07:46:42.348 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
First image: 2461239.82421699 18.07.2026 07:46:42.348 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Last image: 2461280.70604080 28.08.2026 04:56:31.925 /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1835
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 258 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 150733
Objects passed selection criteria: 150451
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 140158
Average stars matched: 131208 (93.6143 %)
Memory usage VmPeak: 518184 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Aug 28 00:18:46 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461280.70551288
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.062 +54:00:02.05 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.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: 23:59:57.530 +54:00:53.50 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.062 +54:00:02.05
Second-epoch image center 23:59:57.530 +54:00:53.50
Angular distance between the image centers 0.0167 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
Image size: 926.7'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: 23:59:59.349 +54:01:28.50 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.062 +54:00:02.05
Second-epoch image center 23:59:59.349 +54:01:28.50
Angular distance between the image centers 0.0244 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 23:59:57.530 +54:00:53.50
Second-epoch second image center 23:59:59.349 +54:01:28.50
Angular distance between the image centers 0.01069 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits &> /tmp/tmp.0r4ZUlH50X
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits &> /tmp/tmp.FcZhg0XDzq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits &> /tmp/tmp.n6xV7cy8az
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits &> /tmp/tmp.Frh3fCeQfk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits and wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits and wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits and wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 33669 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.3600 to 15.3869 deg, Dec +47.7769 to +59.3470 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 345.3600 to 15.3869 deg, Dec 47.7769 to 59.3470 deg
Loaded 26243 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 16959 out of 18283 total matches.
Matched with Tycho-2 18283 out of 33669 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.677900
a=0.000000 b=1.000000 c=22.677900
From vast_summary.log: estimated ref. image limiting mag.: -7.76
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.92
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.92
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 33669 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 345.3600 to 15.3869 deg, Dec +47.7769 to +59.3470 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 345.3600 to 15.3869 deg, Dec 47.7769 to 59.3470 deg
Loaded 26243 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 16959 out of 18283 total matches.
Matched with Tycho-2 18283 out of 33669 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits (aperture=7.3)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 14903 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 344.8488 to 14.8386 deg, Dec +48.0248 to +59.2553 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 344.8488 to 14.8386 deg, Dec 48.0248 to 59.2553 deg
Loaded 25721 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 11593 out of 12074 total matches.
Matched with Tycho-2 12074 out of 14903 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 32 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
3.5 pix Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
2.3 pix Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
2.4 pix fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
2.4 pix fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
Limiting magnitude estimates:
14.9 mag. Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
14.3 mag. Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
14.9 mag. fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
14.9 mag. fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.0r4ZUlH50X (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits' -> 'wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2621, bad_region=6655, passed=33669
Got 33669 stars (including 24831 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat
util/solve_plate_with_UCAC5 got 33669 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3600 through 0 to 15.3869, gap 15.3869 to 345.3600
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.8 to 59.3)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 4904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 28540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3592 through 0 to 15.3870, gap 15.3870 to 345.3592
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.8 to 59.3)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 28540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 28540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4904 stars left (next iteration limit 5394)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits N_match=4904 sigma_overall_arcsec=0.398 sigma_q1_arcsec=0.441 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.363 sigma_q4_arcsec=0.358 n_q1=1555 n_q2=802 n_q3=1643 n_q4=904 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits -region wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.FcZhg0XDzq (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits' -> 'wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1092, bad_region=2856, passed=14903
Got 14903 stars (including 11103 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat
util/solve_plate_with_UCAC5 got 14903 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8488 through 0 to 14.8386, gap 14.8386 to 344.8488
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 4904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 12704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8478 through 0 to 14.8387, gap 14.8387 to 344.8478
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 12704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 12704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4902 stars left (next iteration limit 5394)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits N_match=4902 sigma_overall_arcsec=0.528 sigma_q1_arcsec=0.495 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.586 sigma_q4_arcsec=0.534 n_q1=1550 n_q2=795 n_q3=1659 n_q4=898 worst_quadrant_to_overall_ratio=1.109
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits -region wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.n6xV7cy8az (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2356, bad_region=5279, passed=27332
Got 27332 stars (including 20033 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat
util/solve_plate_with_UCAC5 got 27332 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 345.0826 through 0 to 14.8808, gap 14.8808 to 345.0826
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3515 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2194 matched stars entering correct_measured_positions(), 2409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2042 matched stars entering correct_measured_positions(), 23019 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.09"
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 345.0815 through 0 to 14.9000, gap 14.9000 to 345.0815
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3617 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2502 matched stars entering correct_measured_positions(), 23021 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.22"
Accuracy estimation diagnostic: 2421 matched stars entering correct_measured_positions(), 23092 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.11"
Excluding outliers - 2421 stars left (next iteration limit 2246)
SIP_REFIT: SIP order 2 trial: matched=2421 robust_rms=26.414 arcsec worst_quadrant_rms=29.259 arcsec
SIP_REFIT: SIP order 3 trial: matched=2421 robust_rms=25.841 arcsec worst_quadrant_rms=30.496 arcsec
SIP_REFIT: SIP order 5 trial: matched=2421 robust_rms=23.492 arcsec worst_quadrant_rms=29.362 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2421 robust_rms_before=32.448 arcsec robust_rms_before_corrected=19.541 arcsec robust_rms_after=26.414 arcsec worst_quadrant_rms_before=24.333 worst_quadrant_rms_after=29.259
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.333 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits N_match=2421 sigma_overall_arcsec=13.976 sigma_q1_arcsec=28.542 sigma_q2_arcsec=28.466 sigma_q3_arcsec=7.977 sigma_q4_arcsec=4.918 n_q1=547 n_q2=282 n_q3=931 n_q4=661 worst_quadrant_to_overall_ratio=2.042
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Frh3fCeQfk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2390, bad_region=5330, passed=27256
Got 27256 stars (including 19879 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat
util/solve_plate_with_UCAC5 got 27256 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0821 through 0 to 14.8805, gap 14.8805 to 345.0821
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3523 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2191 matched stars entering correct_measured_positions(), 2418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2058 matched stars entering correct_measured_positions(), 22867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.80"
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 345.0814 through 0 to 14.9002, gap 14.9002 to 345.0814
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3632 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2470 matched stars entering correct_measured_positions(), 22868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.94"
Accuracy estimation diagnostic: 2403 matched stars entering correct_measured_positions(), 22958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.89"
Excluding outliers - 2403 stars left (next iteration limit 2263)
SIP_REFIT: SIP order 2 trial: matched=2403 robust_rms=25.888 arcsec worst_quadrant_rms=28.973 arcsec
SIP_REFIT: SIP order 3 trial: matched=2403 robust_rms=25.133 arcsec worst_quadrant_rms=29.949 arcsec
SIP_REFIT: SIP order 5 trial: matched=2403 robust_rms=22.675 arcsec worst_quadrant_rms=29.110 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2403 robust_rms_before=32.705 arcsec robust_rms_before_corrected=19.223 arcsec robust_rms_after=25.888 arcsec worst_quadrant_rms_before=24.327 worst_quadrant_rms_after=28.973
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.327 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits N_match=2403 sigma_overall_arcsec=13.275 sigma_q1_arcsec=28.154 sigma_q2_arcsec=28.782 sigma_q3_arcsec=7.211 sigma_q4_arcsec=5.779 n_q1=532 n_q2=281 n_q3=915 n_q4=675 worst_quadrant_to_overall_ratio=2.168
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits'
Saving the final (post-refit) wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits'
Saving the final (post-refit) wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits'
Saving the final (post-refit) wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits sigma_overall=0.398 worst_q_ratio=1.108
ref2=Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits sigma_overall=0.528 worst_q_ratio=1.109
new1=fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits sigma_overall=13.976 worst_q_ratio=2.042
new2=fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits sigma_overall=13.275 worst_q_ratio=2.168
reference average sigma_overall=0.463 worst_q_ratio=1.1085
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits) flagged: sigma=13.976 (ref avg 0.463), ratio=2.042 (ref avg 1.1085), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/lib/make_outxyls_for_astrometric_calibration found 26094 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.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: "out4179930.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out4179930.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 23.9262 (2.46046e+10), 7 match, 0 conflict, 18 distractors, 25 index.
RA,Dec = (359.987,54.0132), pixel scale 5.93053 arcsec/pix.
Hit/miss: Hit/miss: ----+--++--+----+---+---+(best)-----+---------------------------------------------------------------------
fit-wcs.c:118:fit_sip_wcs: Too few correspondences for the SIP order specified (5 < 6)
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out4179930.solved to indicate this.
Field: out4179930.xyls
Field center: (RA,Dec) = (359.988321, 54.014041) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:57.197, +54:00:50.546).
Field size: 15.6037 x 10.4313 degrees
Field rotation angle: up is 3.9467 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits' -> 'fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Aug 28 00:12 fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
-rw-r--r-- 1 apache apache 8.5K Aug 28 00:12 out4179930.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits (fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.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: "out4179930.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out4179930.axy"...
Only searching for solutions within 15.4433 degrees of RA,Dec (359.99,54.0149)
log-odds ratio 23.9262 (2.46046e+10), 7 match, 0 conflict, 18 distractors, 25 index.
RA,Dec = (359.987,54.0132), pixel scale 5.93053 arcsec/pix.
Hit/miss: Hit/miss: ----+--++--+----+---+---+(best)-----+---------------------------------------------------------------------
fit-wcs.c:118:fit_sip_wcs: Too few correspondences for the SIP order specified (5 < 6)
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out4179930.solved to indicate this.
Field: out4179930.xyls
Field center: (RA,Dec) = (359.988321, 54.014041) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:57.197, +54:00:50.546).
Field size: 15.6037 x 10.4313 degrees
Field rotation angle: up is 3.9467 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Aug 28 00:12 fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
-rw-r--r-- 1 apache apache 8.5K Aug 28 00:12 out4179930.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat from image00003.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.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: 23:59:57.530 +54:00:53.50 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 27332 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/correct_sextractor_wcs_catalog_usingxy2sky659.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2356, bad_region=5279, passed=27332
Got 27332 stars (including 20033 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat
util/solve_plate_with_UCAC5 got 27332 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 345.0826 through 0 to 14.8808, gap 14.8808 to 345.0826
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3515 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2194 matched stars entering correct_measured_positions(), 2409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2042 matched stars entering correct_measured_positions(), 23019 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.09"
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 345.0815 through 0 to 14.9000, gap 14.9000 to 345.0815
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3617 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2502 matched stars entering correct_measured_positions(), 23021 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.22"
Accuracy estimation diagnostic: 2421 matched stars entering correct_measured_positions(), 23092 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 21.11"
Excluding outliers - 2421 stars left (next iteration limit 2246)
SIP_REFIT: SIP order 2 trial: matched=2421 robust_rms=26.414 arcsec worst_quadrant_rms=29.259 arcsec
SIP_REFIT: SIP order 3 trial: matched=2421 robust_rms=25.841 arcsec worst_quadrant_rms=30.496 arcsec
SIP_REFIT: SIP order 5 trial: matched=2421 robust_rms=23.492 arcsec worst_quadrant_rms=29.362 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2421 robust_rms_before=32.448 arcsec robust_rms_before_corrected=19.541 arcsec robust_rms_after=26.414 arcsec worst_quadrant_rms_before=24.333 worst_quadrant_rms_after=29.259
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.333 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits N_match=2421 sigma_overall_arcsec=13.976 sigma_q1_arcsec=28.542 sigma_q2_arcsec=28.466 sigma_q3_arcsec=7.977 sigma_q4_arcsec=4.918 n_q1=547 n_q2=282 n_q3=931 n_q4=661 worst_quadrant_to_overall_ratio=2.042
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits): sigma 13.976->13.976, ratio 2.042->2.042; reverting to order 3
WCS_QUALITY_RETRY: 2nd new image (fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits) flagged: sigma=13.275 (ref avg 0.463), ratio=2.168 (ref avg 1.1085), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/lib/make_outxyls_for_astrometric_calibration found 26134 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.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: "out20982.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out20982.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 24.5439 (4.56348e+10), 7 match, 0 conflict, 18 distractors, 24 index.
RA,Dec = (359.995,54.0229), pixel scale 5.93069 arcsec/pix.
Hit/miss: Hit/miss: ----+----+++----+---+---+(best)---------+-----------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out20982.solved to indicate this.
Field: out20982.xyls
Field center: (RA,Dec) = (359.995903, 54.023761) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:59.017, +54:01:25.541).
Field size: 15.6044 x 10.4319 degrees
Field rotation angle: up is 3.94422 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits' -> 'fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Aug 28 00:13 fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
-rw-r--r-- 1 apache apache 8.5K Aug 28 00:13 out20982.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits (fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.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: "out20982.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out20982.axy"...
Only searching for solutions within 15.445 degrees of RA,Dec (359.997,54.0246)
log-odds ratio 24.5439 (4.56348e+10), 7 match, 0 conflict, 18 distractors, 24 index.
RA,Dec = (359.995,54.0229), pixel scale 5.93069 arcsec/pix.
Hit/miss: Hit/miss: ----+----+++----+---+---+(best)---------+-----------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out20982.solved to indicate this.
Field: out20982.xyls
Field center: (RA,Dec) = (359.995903, 54.023761) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:59.017, +54:01:25.541).
Field size: 15.6044 x 10.4319 degrees
Field rotation angle: up is 3.94422 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Aug 28 00:13 fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
-rw-r--r-- 1 apache apache 8.5K Aug 28 00:13 out20982.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat from image00004.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
Image size: 926.7'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: 23:59:59.349 +54:01:28.50 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 27256 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/correct_sextractor_wcs_catalog_usingxy2sky47527.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2390, bad_region=5330, passed=27256
Got 27256 stars (including 19879 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat
util/solve_plate_with_UCAC5 got 27256 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 926.7'
Seting catalog search parameters based on the expected field of view 926.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012871 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010297 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0821 through 0 to 14.8805, gap 14.8805 to 345.0821
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3523 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2191 matched stars entering correct_measured_positions(), 2418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 22.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2058 matched stars entering correct_measured_positions(), 22867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.80"
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 345.0814 through 0 to 14.9002, gap 14.9002 to 345.0814
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 691 to 748 (Dec 48.3 to 59.3)
Done reading UCAC5 zone files...
Matched 3632 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2470 matched stars entering correct_measured_positions(), 22868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.94"
Accuracy estimation diagnostic: 2403 matched stars entering correct_measured_positions(), 22958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 20.89"
Excluding outliers - 2403 stars left (next iteration limit 2263)
SIP_REFIT: SIP order 2 trial: matched=2403 robust_rms=25.888 arcsec worst_quadrant_rms=28.973 arcsec
SIP_REFIT: SIP order 3 trial: matched=2403 robust_rms=25.133 arcsec worst_quadrant_rms=29.949 arcsec
SIP_REFIT: SIP order 5 trial: matched=2403 robust_rms=22.675 arcsec worst_quadrant_rms=29.110 arcsec
SIP_REFIT: selected SIP order 2
SIP_REFIT: order=2 matched=2403 robust_rms_before=32.705 arcsec robust_rms_before_corrected=19.223 arcsec robust_rms_after=25.888 arcsec worst_quadrant_rms_before=24.327 worst_quadrant_rms_after=28.973
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 24.327 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits N_match=2403 sigma_overall_arcsec=13.275 sigma_q1_arcsec=28.154 sigma_q2_arcsec=28.782 sigma_q3_arcsec=7.211 sigma_q4_arcsec=5.779 n_q1=532 n_q2=281 n_q3=915 n_q4=675 worst_quadrant_to_overall_ratio=2.168
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits -region wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 2nd new image (fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits): sigma 13.275->13.275, ratio 2.168->2.168; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=13.976 -- 30.19x the reference average (0.463); plate solution may be of low accuracy
WARNING: 2nd new image has sigma_overall_arcsec=13.275 -- 28.67x the reference average (0.463); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246_astrometric_residuals.png (4904 matched stars from wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111_astrometric_residuals.png (4902 matched stars from wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100_astrometric_residuals.png (2421 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 11.79 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101_astrometric_residuals.png (2403 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 11.46 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-55-46_20.00sec_-0.00C_LIGHT_0100.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-28_CI_Cas-04-Q2b1x1_000122_TTUQ2b1x1_2739263_gucwPK03/wcs_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:42.49 +50:06:38.8: 15.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:03:28.56 +54:25:38.6: 11.71 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:19:20.29 +50:14:26.1: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:24.96 +54:18:51.5: 15.55 +/- 0.35 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:39.47 +57:08:01.3: 12.17 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:14.99 +52:50:25.3: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:14.48 +50:25:54.0: 15.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:20:05.34 +55:44:17.8: 15.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:54:34.26 +51:57:43.2: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:54.38 +52:08:13.6: 13.67 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:03:28.56 +54:25:38.6: 11.85 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:14.48 +50:25:54.0: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:39.47 +57:08:01.3: 12.28 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:42.49 +50:06:38.8: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:14.99 +52:50:25.3: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:05.34 +55:44:17.8: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:24.96 +54:18:51.5: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:19:20.29 +50:14:26.1: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:54:34.26 +51:57:43.2: 14.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.55 +/- 0.35
Forced photometry reference-image weighted average: 11.74 +/- 0.01
Forced photometry reference-image weighted average: 12.19 +/- 0.02
Forced photometry filter KEPT candidate at 23:45:24.96 +54:18:51.5: ref_mag=15.55 +/- 0.35 new_mean_mag=11.6436 delta=3.91 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:39:39.47 +57:08:01.3: ref_mag=12.19 +/- 0.02 new_mean_mag=11.9247 delta=0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:03:28.56 +54:25:38.6: ref_mag=11.74 +/- 0.01 new_mean_mag=11.9879 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:54.38 +52:08:13.6: 13.90 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.06
Forced photometry filter KEPT candidate at 23:34:54.38 +52:08:13.6: ref_mag=13.70 +/- 0.06 new_mean_mag=11.4670 delta=2.24 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:11.96 +57:53:08.8: 11.49 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:00:07.97 +51:20:34.4: 14.49 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:11.96 +57:53:08.8: 11.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Forced photometry filter REJECTED candidate at 23:48:11.96 +57:53:08.8: ref_mag=11.54 +/- 0.01 new_mean_mag=11.8773 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:00:07.97 +51:20:34.4: 14.92 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.49 +/- 0.13
Forced photometry filter KEPT candidate at 00:00:07.97 +51:20:34.4: ref_mag=14.49 +/- 0.13 new_mean_mag=11.6250 delta=2.86 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:22.76 +56:41:44.1: 12.16 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:22.76 +56:41:44.1: 12.07 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.04
Forced photometry filter REJECTED candidate at 23:57:22.76 +56:41:44.1: ref_mag=12.11 +/- 0.04 new_mean_mag=11.9487 delta=0.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:44.57 +53:36:12.5: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:44.57 +53:36:12.5: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:25:49.42 +50:28:02.5: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:25:49.42 +50:28:02.5: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:35:43.98 +55:35:51.8: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:15.89 +50:18:04.2: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:35:43.98 +55:35:51.8: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:15.89 +50:18:04.2: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:22:07.42 +49:54:19.3: 15.11 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:40.09 +56:54:44.7: 14.74 +/- 0.19 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:21.87 +54:04:28.5: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:19:20.06 +55:37:10.4: 15.10 +/- 0.28 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:28.46 +51:28:27.3: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:40.09 +56:54:44.7: 14.67 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:28.46 +51:28:27.3: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:21.87 +54:04:28.5: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:22:07.42 +49:54:19.3: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:19:20.06 +55:37:10.4: 14.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.72 +/- 0.17
Forced photometry filter KEPT candidate at 23:38:40.09 +56:54:44.7: ref_mag=14.72 +/- 0.17 new_mean_mag=12.1520 delta=2.57 (need > 0.90)
Forced photometry reference-image weighted average: 15.11 +/- 0.28
Forced photometry reference-image weighted average: 15.10 +/- 0.28
Forced photometry filter KEPT candidate at 23:22:07.42 +49:54:19.3: ref_mag=15.11 +/- 0.28 new_mean_mag=12.1735 delta=2.94 (need > 0.90)
Forced photometry filter KEPT candidate at 00:19:20.06 +55:37:10.4: ref_mag=15.10 +/- 0.28 new_mean_mag=12.2573 delta=2.84 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:12.21 +50:10:29.9: 15.05 +/- 0.24 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:47:28.16 +57:22:18.7: 12.29 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:12.21 +50:10:29.9: 14.47 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.18
Forced photometry filter KEPT candidate at 23:33:12.21 +50:10:29.9: ref_mag=14.80 +/- 0.18 new_mean_mag=12.2879 delta=2.51 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:47:28.16 +57:22:18.7: 12.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Forced photometry filter REJECTED candidate at 23:47:28.16 +57:22:18.7: ref_mag=12.28 +/- 0.02 new_mean_mag=12.2351 delta=0.05 (need > 0.90)
Adding exclusion_list_local.txt__out50521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50792.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 33s
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: 17s
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Considering the candidate 50521_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50521_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50527_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50527_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50532_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50532_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50535_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50535_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50536_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50536_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 50538_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50538_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 50540_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50540_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 50543_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50543_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 50545_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50545_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 50551_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50551_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50557_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50557_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 50563_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50563_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50572_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50572_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:15:50.86 +57:32:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50573_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50573_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50576_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50576_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50583_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50583_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50629_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50629_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 50663_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50663_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 50680_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50680_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50732_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50732_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50735_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50735_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50744_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50744_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50746_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50746_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 50748_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50748_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50750_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50750_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50753_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50753_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50765_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50765_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 50789_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50789_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50791_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50791_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50792_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 50792_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 50793_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50793_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 50828_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 50828_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 191561_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191561_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 191573_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191573_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191580_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191580_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191585_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191585_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191589_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191589_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 191591_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191591_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191592_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191592_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191593_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191593_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191597_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191597_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 191599_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191599_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191609_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191609_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191614_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191614_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 191615_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191615_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191616_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191616_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 191617_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191617_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191626_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191626_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191627_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191627_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191628_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191628_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191639_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191639_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191640_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191640_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191642_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191642_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191643_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191643_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191644_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191644_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191647_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191647_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 191651_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191651_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191661_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191661_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191663_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191663_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 191667_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191667_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 191669_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191669_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 191672_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191672_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191673_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191673_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191685_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191685_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 191686_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191686_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191688_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191688_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191689_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191689_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.1") between the two second-epoch detections
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Considering the candidate 191690_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191690_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191692_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191692_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191694_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191694_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 191697_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191697_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 191702_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191702_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191703_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191703_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191705_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191705_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191706_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191706_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191711_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191711_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191712_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191712_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191715_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191715_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191716_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191716_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 191718_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191718_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191721_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191721_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 191724_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191724_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191725_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191725_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 191726_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191726_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 191727_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191727_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191729_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191729_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 191730_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191730_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191731_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191731_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191733_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191733_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191734_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191734_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191740_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191740_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191741_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191741_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 191742_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191742_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191743_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191743_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191744_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191744_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191746_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191746_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191747_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191747_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 191748_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191748_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191752_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191752_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191756_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191756_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191757_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191757_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191761_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191761_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 191762_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191762_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191765_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191765_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 191766_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191766_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191767_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191767_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191768_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191768_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191769_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191769_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 191772_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191772_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191773_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191773_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191774_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191774_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191778_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191778_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 191784_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191784_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191786_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191786_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 191788_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191788_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 191789_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191789_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 191792_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191792_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 191796_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191796_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 191799_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191799_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 191801_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191801_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191809_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191809_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191812_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191812_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 191813_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191813_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191814_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191814_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191815_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191815_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191821_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191821_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191824_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191824_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191825_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191825_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 191827_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191827_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191830_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191830_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191831_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191831_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191833_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191833_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191834_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191834_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191837_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191837_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 191838_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191838_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 191839_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191839_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 191840_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191840_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 191841_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191841_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191842_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191842_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 191844_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191844_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191848_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191848_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191849_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191849_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 191850_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191850_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191851_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191851_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 191853_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191853_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191855_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191855_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 191856_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191856_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191857_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191857_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 191859_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191859_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191860_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191860_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191861_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191861_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 191863_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191863_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191865_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191865_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191867_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191867_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191869_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191869_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191875_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191875_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 191877_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191877_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191878_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191878_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 191879_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191879_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191880_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191880_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191881_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191881_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191886_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191886_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191887_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191887_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191888_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191888_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191891_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191891_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191893_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191893_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191896_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191896_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 191898_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191898_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 191899_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191899_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191900_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191900_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 191901_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191901_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191903_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191903_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191905_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191905_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191906_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191906_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191908_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191908_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 191909_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191909_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 191910_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191910_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 191911_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191911_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191912_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191912_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191916_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191916_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (42.6") between the two second-epoch detections
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Considering the candidate 191917_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191917_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191918_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191918_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191922_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191922_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191923_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191923_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 191924_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191924_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191927_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191927_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 191928_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191928_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191931_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191931_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 191933_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191933_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 191934_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191934_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191938_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191938_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191939_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191939_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (36.7") between the two second-epoch detections
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Considering the candidate 191940_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191940_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191941_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191941_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191944_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191944_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191946_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191946_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191947_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191947_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191948_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191948_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191949_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191949_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 191950_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191950_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 191951_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191951_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 191953_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191953_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191954_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191954_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 191955_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191955_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191956_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191956_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191957_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191957_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 191961_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191961_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191964_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191964_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191965_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191965_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191966_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191966_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191967_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191967_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191968_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191968_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191971_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191971_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191973_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191973_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 191974_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191974_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 191975_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191975_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191978_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191978_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 191980_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191980_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 191981_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191981_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191983_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191983_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 191989_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191989_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 191990_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 191990_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 191992_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191992_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 191995_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 191995_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192002_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192002_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192003_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192003_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192004_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192004_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192006_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192006_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.7") between the two second-epoch detections
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Considering the candidate 192008_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192008_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192011_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192011_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192012_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192012_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 192016_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192016_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192017_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192017_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192018_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192018_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 192019_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192019_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192023_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192023_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192024_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192024_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192025_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192025_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 192027_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192027_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192029_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192029_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192030_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192030_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 192031_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192031_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192032_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192032_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
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Considering the candidate 192033_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192033_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192034_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192034_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192035_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192035_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 192037_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192037_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192039_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192039_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192040_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192040_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192044_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192044_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 192045_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192045_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 192047_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192047_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 192049_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192049_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192052_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192052_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192057_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192057_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192058_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192058_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192060_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192060_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 192061_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192061_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192063_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192063_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 192069_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192069_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192070_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192070_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192071_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192071_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 192072_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192072_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192074_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192074_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192075_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192075_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192076_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192076_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192079_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192079_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 192081_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192081_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192082_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192082_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192083_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192083_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 192086_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192086_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192087_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192087_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192089_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192089_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192091_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192091_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (31.4") between the two second-epoch detections
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Considering the candidate 192094_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192094_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192095_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192095_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192098_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192098_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192099_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192099_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192100_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192100_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192101_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192101_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192102_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192102_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192103_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192103_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192104_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192104_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192105_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192105_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192106_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192106_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 192108_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192108_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 192111_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192111_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192116_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192116_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192117_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192117_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192120_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192120_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192121_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192121_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 192123_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192123_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192124_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192124_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192125_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192125_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
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Considering the candidate 192126_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192126_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192133_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192133_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192134_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192134_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 192136_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192136_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192140_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192140_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192141_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192141_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192142_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192142_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192144_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192144_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192145_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192145_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192146_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192146_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 192147_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192147_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 192149_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192149_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 192151_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192151_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192160_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192160_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192161_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192161_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 192162_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192162_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192164_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192164_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 192165_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192165_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 192167_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192167_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192168_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192168_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192169_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192169_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 192171_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192171_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 192172_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192172_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 192175_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192175_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192176_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192176_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192182_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192182_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 192184_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192184_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192187_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192187_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192192_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192192_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192193_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192193_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 192197_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192197_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192198_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192198_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192200_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192200_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 192202_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192202_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 192203_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192203_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192205_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192205_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 192206_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192206_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192207_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192207_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192209_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192209_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192210_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192210_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192212_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192212_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192213_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192213_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 192214_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192214_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192216_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192216_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 192220_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192220_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192223_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192223_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192226_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192226_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (37.8") between the two second-epoch detections
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Considering the candidate 192228_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192228_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192231_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192231_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192233_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192233_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 192235_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192235_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
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Considering the candidate 192237_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192237_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192239_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192239_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192240_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192240_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 192246_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192246_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 192247_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192247_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192249_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192249_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 192250_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192250_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192251_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192251_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192252_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192252_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 192253_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192253_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192254_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192254_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192255_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192255_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 192257_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192257_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 192260_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192260_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192262_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192262_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 192265_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192265_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 192266_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192266_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
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Considering the candidate 192267_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192267_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192268_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192268_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192271_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192271_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192273_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192273_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192275_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192275_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 192280_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192280_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192285_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192285_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (30.3") between the two second-epoch detections
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Considering the candidate 192286_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192286_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192289_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192289_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192291_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192291_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192292_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192292_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192293_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192293_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192299_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192299_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192301_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192301_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192307_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192307_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192308_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192308_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192313_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192313_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 192314_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192314_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 192315_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192315_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (35.2") between the two second-epoch detections
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Considering the candidate 192317_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192317_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 192319_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192319_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192320_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192320_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192321_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192321_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192325_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192325_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 192326_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192326_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 192328_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192328_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 192329_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192329_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192332_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192332_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192337_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192337_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 192339_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192339_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192340_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192340_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192341_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192341_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 192342_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192342_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 192343_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192343_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 192348_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192348_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 192350_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192350_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192351_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192351_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192352_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192352_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192353_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192353_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192354_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192354_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 192355_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192355_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192356_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192356_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192357_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192357_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 192358_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192358_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192360_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192360_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192361_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192361_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192362_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192362_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192363_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192363_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 192364_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192364_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192365_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192365_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (35.1") between the two second-epoch detections
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Considering the candidate 192369_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192369_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 192373_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192373_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192374_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192374_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192378_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192378_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 192382_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192382_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 192384_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192384_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192385_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192385_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192387_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192387_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192389_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192389_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192390_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192390_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 192395_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192395_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 192396_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192396_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 192398_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192398_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192401_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192401_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 192402_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192402_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192403_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192403_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192404_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192404_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 192405_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192405_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192407_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192407_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:57:15.86 +54:22:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192408_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192408_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192413_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192413_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 192414_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192414_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 192415_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192415_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 192417_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192417_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192418_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192418_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192419_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192419_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192420_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192420_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192423_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192423_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192424_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192424_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192427_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192427_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192428_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192428_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 192431_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192431_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192436_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192436_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192438_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192438_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192440_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192440_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192445_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192445_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 192448_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192448_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 192452_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192452_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 192453_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192453_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192454_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192454_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192456_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192456_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 192457_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192457_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 192458_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192458_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192459_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192459_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192460_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192460_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 192463_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192463_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192465_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192465_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192467_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192467_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 192468_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192468_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192469_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192469_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192472_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192472_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192476_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192476_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192478_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192478_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 192479_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192479_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192480_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192480_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192481_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192481_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192482_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192482_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192484_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192484_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192485_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192485_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192486_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192486_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192487_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192487_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 192488_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192488_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192490_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192490_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192491_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192491_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (30.6") between the two second-epoch detections
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Considering the candidate 192493_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192493_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 192495_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192495_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 192496_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192496_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 192497_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192497_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 192498_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192498_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 192499_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192499_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192503_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192503_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192504_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192504_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 192510_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192510_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192511_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192511_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192515_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192515_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192516_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192516_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192517_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192517_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192518_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192518_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192519_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192519_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192520_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192520_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192523_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192523_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192524_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192524_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192527_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192527_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192528_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192528_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192538_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192538_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 192540_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192540_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 192542_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192542_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192543_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192543_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192544_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192544_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192546_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192546_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192547_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192547_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 192548_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192548_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192550_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192550_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192555_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192555_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192558_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192558_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192560_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192560_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 192561_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192561_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192562_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192562_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 192564_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192564_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192566_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192566_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192568_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192568_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192571_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192571_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192573_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192573_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192574_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192574_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192583_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192583_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 192584_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192584_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192588_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192588_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192589_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192589_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192592_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192592_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 192593_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192593_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192595_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192595_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192597_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192597_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192598_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192598_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 192599_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192599_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192601_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192601_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192602_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192602_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 192604_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192604_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 192606_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192606_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192608_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192608_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192613_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192613_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192614_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192614_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192615_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192615_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 192617_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192617_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192621_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192621_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192622_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192622_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:00:49.01 +56:12:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192624_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192624_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192625_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192625_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 192626_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192626_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 192628_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192628_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 192629_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192629_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192631_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192631_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 192632_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192632_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 192633_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192633_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192634_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192634_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 192639_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192639_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 192641_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192641_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192648_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192648_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 192649_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192649_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 192653_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192653_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192655_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192655_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (43.6") between the two second-epoch detections
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Considering the candidate 192656_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192656_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192662_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192662_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 192665_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192665_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192667_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192667_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 192668_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192668_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192669_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192669_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192670_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192670_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (34.5") between the two second-epoch detections
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Considering the candidate 192671_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192671_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192673_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192673_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192676_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192676_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192678_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192678_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 192679_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192679_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 192680_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192680_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192682_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192682_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192683_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192683_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192684_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192684_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 192685_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192685_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192686_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192686_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192687_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192687_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 192689_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192689_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 192690_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192690_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192692_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192692_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192695_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192695_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 192698_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192698_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192702_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192702_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 192704_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192704_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192705_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192705_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192706_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192706_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192707_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192707_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 192709_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192709_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 192710_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192710_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 192711_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192711_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192712_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192712_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 192713_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192713_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192714_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192714_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192715_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192715_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192717_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192717_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192719_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192719_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 192721_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192721_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192722_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192722_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 192723_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192723_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192726_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192726_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192730_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192730_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192731_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192731_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192734_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192734_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192738_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192738_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192740_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192740_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192741_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192741_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192742_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192742_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 192744_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192744_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192746_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192746_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192748_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192748_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192749_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192749_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192750_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192750_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192751_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192751_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192754_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192754_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192758_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192758_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192759_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192759_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192760_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192760_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192761_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192761_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 192762_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192762_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192767_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192767_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192768_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192768_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:54:47.79 +56:48:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192771_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192771_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192775_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192775_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192776_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192776_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192778_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192778_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192779_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192779_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192781_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192781_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192783_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192783_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 192785_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192785_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 192786_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192786_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 192787_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192787_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192789_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192789_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 192790_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192790_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192793_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192793_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192794_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192794_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192796_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192796_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 192803_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192803_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 192804_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192804_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192809_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192809_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192810_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192810_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192811_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192811_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192814_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192814_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192819_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192819_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192820_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192820_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 192823_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192823_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192824_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192824_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 192825_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192825_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 192826_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192826_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192827_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192827_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
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Considering the candidate 192828_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192828_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192832_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192832_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192833_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192833_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192835_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192835_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 192837_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192837_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 192838_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192838_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 192839_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192839_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192841_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192841_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 192842_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192842_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:54:57.16 +56:12:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192843_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192843_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 192845_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192845_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192846_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192846_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192851_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192851_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192855_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192855_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 192856_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192856_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192857_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192857_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192858_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192858_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192861_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192861_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192862_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192862_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:59:11.63 +57:36:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192865_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192865_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 192869_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192869_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 192870_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192870_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 192872_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192872_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192873_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192873_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192877_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192877_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192878_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192878_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 192881_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192881_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192886_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192886_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192889_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192889_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 192890_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192890_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (25.0") between the two second-epoch detections
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Considering the candidate 192900_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192900_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192902_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192902_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192907_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192907_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192908_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192908_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192909_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192909_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192913_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192913_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192922_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192922_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (32.9") between the two second-epoch detections
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Considering the candidate 192923_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192923_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192924_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192924_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 192926_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192926_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 192928_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192928_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192932_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192932_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 192933_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192933_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 192934_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192934_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 192938_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192938_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 192972_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192972_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192974_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192974_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192981_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192981_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192983_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192983_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 192984_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192984_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 192990_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 192990_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 192992_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192992_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 192996_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 192996_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193003_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193003_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193023_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193023_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193032_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193032_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:42:24.83 +56:49:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193043_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193043_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193046_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193046_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193059_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193059_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 193060_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193060_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193073_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193073_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193080_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193080_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 193082_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193082_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193084_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193084_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193086_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193086_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193088_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193088_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 193091_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193091_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193098_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193098_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:49:02.58 +56:44:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193101_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193101_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 193111_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193111_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193116_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193116_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 193117_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193117_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193125_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193125_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 193130_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193130_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193132_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193132_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 193135_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193135_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 193137_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193137_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193140_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193140_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 193158_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193158_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193160_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193160_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193165_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193165_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193173_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193173_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193177_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193177_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:53:17.26 +57:48:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193181_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193181_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193185_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193185_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193201_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193201_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193202_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193202_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193214_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193214_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193217_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193217_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 193218_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193218_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193230_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193230_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193231_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193231_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193233_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193233_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193234_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193234_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 193242_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193242_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 193253_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193253_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193255_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193255_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 193257_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193257_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 193264_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193264_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193276_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193276_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193278_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193278_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 193279_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193279_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 193280_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193280_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193284_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193284_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193295_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193295_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193300_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193300_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193306_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193306_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193318_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193318_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193320_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193320_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193322_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193322_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193323_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193323_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 193326_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193326_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193328_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193328_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193334_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193334_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193339_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193339_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193344_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193344_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 193345_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193345_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193349_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193349_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193354_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193354_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 193361_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193361_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193365_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193365_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193374_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193374_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193376_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193376_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 193380_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193380_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193385_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193385_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 193386_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193386_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193389_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193389_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 193393_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193393_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193400_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193400_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 193405_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193405_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 193409_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193409_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193418_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193418_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193419_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193419_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193432_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193432_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193433_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193433_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 193434_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193434_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 193437_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193437_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193439_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193439_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193442_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193442_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193444_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193444_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193448_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193448_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193450_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193450_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:09:23.56 +58:04:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193455_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193455_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193459_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193459_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 193461_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193461_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193468_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193468_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193469_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193469_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 193472_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193472_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193478_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193478_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 193481_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193481_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 193484_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193484_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193485_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193485_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:31:48.24 +54:10:40.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 193490_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193490_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193501_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193501_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193503_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193503_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 193504_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193504_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193510_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193510_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
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Considering the candidate 193513_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193513_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 193525_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193525_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193528_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193528_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193532_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193532_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (31.0") between the two second-epoch detections
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Considering the candidate 193534_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193534_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193536_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193536_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 193537_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193537_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193542_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193542_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193543_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193543_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 193544_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193544_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193550_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193550_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193555_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193555_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193557_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193557_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193558_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193558_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193559_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193559_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193562_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193562_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (35.4") between the two second-epoch detections
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Considering the candidate 193564_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193564_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193567_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193567_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193574_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193574_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193579_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193579_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 193583_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193583_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193587_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193587_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (34.0") between the two second-epoch detections
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Considering the candidate 193592_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193592_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193596_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193596_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193597_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193597_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 193605_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193605_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 193608_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193608_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 193617_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193617_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 193618_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193618_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193619_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193619_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193623_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193623_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193627_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193627_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 193628_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193628_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193630_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193630_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (30.2") between the two second-epoch detections
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Considering the candidate 193631_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193631_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193634_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193634_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 193636_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193636_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193641_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193641_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 193643_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193643_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193645_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193645_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193647_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193647_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:41:10.73 +57:16:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193654_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193654_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 193656_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193656_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (27.6") between the two second-epoch detections
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Considering the candidate 193657_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193657_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193659_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193659_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193660_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193660_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193662_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193662_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
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Considering the candidate 193663_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193663_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193664_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193664_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193666_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193666_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193668_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193668_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 193670_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193670_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193671_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193671_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 193672_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193672_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:28:10.03 +53:34:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 3.472 1992758383176329600 352.04017774798 +53.57905369788 14.9794 14.1514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193677_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193677_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 193679_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193679_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193683_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193683_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193684_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193684_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 193685_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193685_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193687_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193687_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 193689_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193689_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193695_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193695_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193710_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193710_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193711_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193711_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193716_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193716_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 193731_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193731_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193735_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193735_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 193737_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193737_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 193739_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193739_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193745_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193745_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 193758_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193758_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193760_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193760_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193761_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193761_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 193763_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193763_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193764_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193764_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 193768_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193768_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193774_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193774_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193777_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193777_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193778_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193778_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193783_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193783_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193787_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193787_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193789_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193789_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193791_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193791_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193792_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193792_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193798_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193798_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193802_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193802_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193806_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193806_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193809_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193809_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (33.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193825_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193825_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 193827_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193827_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193831_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193831_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193833_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193833_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193835_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193835_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193842_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193842_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193849_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193849_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193851_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193851_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193852_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193852_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193853_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193853_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193858_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193858_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193860_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193860_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:00:38.67 +56:13:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193861_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193861_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193865_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193865_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193870_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193870_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193872_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193872_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 193874_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193874_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 193876_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193876_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193882_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193882_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193883_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193883_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193884_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193884_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193885_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193885_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193895_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193895_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193900_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193900_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193901_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193901_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 193902_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193902_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:44:11.53 +53:43:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.626 1993328479955620608 356.04906627794 +53.72476679109 15.1868 14.6226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193906_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193906_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193909_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193909_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 193913_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193913_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193915_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193915_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193923_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193923_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 193925_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193925_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193926_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193926_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 193932_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193932_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193933_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193933_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193943_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193943_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 193945_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193945_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 193946_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193946_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193947_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193947_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193952_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193952_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193955_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193955_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193956_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193956_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 193958_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193958_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193965_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193965_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193974_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193974_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 193977_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193977_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 193978_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193978_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 193981_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193981_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 193991_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193991_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 193992_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 193992_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 193994_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 193994_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194002_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194002_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 194003_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194003_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194004_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194004_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194007_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194007_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194008_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194008_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194009_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194009_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194014_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194014_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 194016_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194016_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 194017_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194017_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194021_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194021_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 194023_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194023_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 194024_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194024_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 194032_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194032_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194033_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194033_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 194034_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194034_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 194036_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194036_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194039_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194039_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 194040_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194040_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194041_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194041_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194042_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194042_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 194045_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194045_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194047_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194047_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194048_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194048_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194061_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194061_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 194064_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194064_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 194066_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194066_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194068_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194068_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 194069_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194069_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194076_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194076_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194078_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194078_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 194080_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194080_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194086_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194086_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194087_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194087_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 194089_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194089_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194091_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194091_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194097_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194097_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194101_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194101_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 194102_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194102_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 194104_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194104_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194110_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194110_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194114_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194114_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 194118_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194118_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194119_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194119_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 194120_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194120_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194121_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194121_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194122_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194122_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194125_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194125_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194127_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194127_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194128_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194128_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194130_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194130_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (32.3") between the two second-epoch detections
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Considering the candidate 194133_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194133_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 194136_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194136_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 194137_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194137_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194138_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194138_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 194145_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194145_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194148_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194148_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 194149_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194149_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 194150_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194150_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194152_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194152_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (30.6") between the two second-epoch detections
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Considering the candidate 194153_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194153_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 194157_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194157_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194167_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194167_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194170_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194170_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194174_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194174_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194176_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194176_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194178_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194178_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194181_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194181_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194183_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194183_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194184_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194184_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194186_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194186_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194191_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194191_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194193_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194193_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194196_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194196_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 194198_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194198_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194201_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194201_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194203_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194203_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194205_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194205_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194207_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194207_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194209_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194209_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 194211_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194211_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194215_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194215_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194216_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194216_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 194219_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194219_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194220_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194220_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194221_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194221_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194224_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194224_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194230_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194230_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194231_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194231_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194232_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194232_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194236_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194236_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194238_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194238_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194243_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194243_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194245_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194245_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 194247_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194247_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194249_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194249_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194250_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194250_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 194253_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194253_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (33.5") between the two second-epoch detections
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Considering the candidate 194256_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194256_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 194258_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194258_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194259_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194259_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 194262_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194262_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 194263_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194263_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 194264_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194264_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194266_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194266_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194272_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194272_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194275_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194275_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194277_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194277_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194279_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194279_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194282_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194282_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194287_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194287_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194292_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194292_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194293_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194293_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194295_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194295_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194296_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194296_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194300_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194300_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194301_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194301_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194303_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194303_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194305_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194305_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194315_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194315_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194320_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194320_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194322_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194322_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 194323_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194323_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194331_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194331_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194339_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194339_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194345_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194345_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194346_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194346_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194348_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194348_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194350_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194350_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194355_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194355_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194360_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194360_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194361_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194361_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194363_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194363_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 194366_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194366_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (40.7") between the two second-epoch detections
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Considering the candidate 194374_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194374_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (33.9") between the two second-epoch detections
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Considering the candidate 194377_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194377_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194378_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194378_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194381_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194381_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194382_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194382_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194384_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194384_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194387_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194387_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194391_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194391_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194392_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194392_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 194393_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194393_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194394_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194394_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194398_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194398_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194400_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194400_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 194401_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194401_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 194402_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194402_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194404_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194404_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194405_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194405_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194407_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194407_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194411_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194411_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194412_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194412_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194413_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194413_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194414_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194414_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194420_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194420_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 194422_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194422_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194426_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194426_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194430_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194430_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 194431_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194431_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194433_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194433_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194437_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194437_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194438_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194438_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 194440_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194440_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194442_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194442_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
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Considering the candidate 194444_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194444_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194445_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194445_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
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Considering the candidate 194447_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194447_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 194448_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194448_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194453_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194453_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194455_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194455_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194460_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194460_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194463_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194463_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (41.3") between the two second-epoch detections
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Considering the candidate 194464_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194464_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194465_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194465_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194466_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194466_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194471_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194471_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194472_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194472_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 194473_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194473_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194474_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194474_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194475_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194475_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 194480_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194480_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194483_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194483_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 194484_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194484_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194485_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194485_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 194488_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194488_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 194492_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194492_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194497_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194497_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 194499_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194499_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194500_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194500_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 194501_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194501_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194503_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194503_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194507_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194507_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 194508_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194508_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 194513_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194513_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194514_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194514_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 194516_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194516_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194519_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194519_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 194521_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194521_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
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Considering the candidate 194523_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194523_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194524_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194524_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194531_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194531_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194540_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194540_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 194544_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194544_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194551_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194551_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 194558_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194558_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194559_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194559_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194562_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194562_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194566_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194566_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 194572_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194572_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194573_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194573_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (25.7") between the two second-epoch detections
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Considering the candidate 194578_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194578_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 194579_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194579_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 194582_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194582_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194583_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194583_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 194585_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194585_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194588_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194588_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194592_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194592_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194593_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194593_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 194596_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194596_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 194597_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194597_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194601_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194601_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194609_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194609_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194612_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194612_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 194613_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194613_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194615_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194615_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194616_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194616_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194621_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194621_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194623_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194623_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (45.7") between the two second-epoch detections
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Considering the candidate 194625_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194625_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 194626_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194626_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 194627_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194627_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.1") between the two second-epoch detections
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Considering the candidate 194630_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194630_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 194631_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194631_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194633_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194633_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194634_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194634_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 194636_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194636_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194637_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194637_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 194644_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194644_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194648_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194648_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194649_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194649_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 194651_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194651_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194660_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194660_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194661_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194661_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194662_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194662_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 194664_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194664_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 194665_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194665_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194667_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194667_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194668_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194668_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194676_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194676_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194679_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194679_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194680_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194680_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194684_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194684_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194686_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194686_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 194687_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194687_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 194695_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194695_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194698_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194698_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194699_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194699_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 194702_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194702_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194711_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194711_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 194713_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194713_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194714_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194714_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194721_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194721_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194722_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194722_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194724_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194724_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 194729_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194729_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194733_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194733_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194734_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194734_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194735_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194735_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 194737_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194737_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194739_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194739_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194743_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194743_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 194744_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194744_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 194746_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194746_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194747_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194747_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194754_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194754_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194756_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194756_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194757_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194757_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194758_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194758_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194760_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194760_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194764_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194764_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194765_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194765_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 194767_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194767_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 194769_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194769_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 194770_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194770_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194775_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194775_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194776_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194776_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 194778_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194778_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 194779_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194779_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194780_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194780_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194782_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194782_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194784_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194784_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 194785_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194785_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194787_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194787_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194792_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194792_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 194797_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194797_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194801_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194801_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194802_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194802_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194807_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194807_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194809_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194809_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194812_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194812_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 194813_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194813_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 194814_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194814_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194817_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194817_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 194823_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194823_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 194824_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194824_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194825_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194825_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194827_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194827_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194831_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194831_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 194833_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194833_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194834_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194834_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 194835_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194835_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 194836_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194836_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194838_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194838_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194840_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194840_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 194841_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194841_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (34.2") between the two second-epoch detections
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Considering the candidate 194842_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194842_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 194844_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194844_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194846_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194846_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 194851_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194851_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 194853_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194853_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194856_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194856_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194857_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194857_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 194860_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194860_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 194867_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194867_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194870_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194870_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194871_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194871_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 194873_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194873_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 194888_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194888_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194892_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194892_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194895_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194895_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (28.2") between the two second-epoch detections
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Considering the candidate 194897_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194897_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 194902_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194902_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194903_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194903_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194905_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194905_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194908_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194908_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 194912_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194912_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194914_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194914_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194915_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194915_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 194918_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194918_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194925_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194925_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194932_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194932_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194936_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194936_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 194948_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194948_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 194958_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194958_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194972_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194972_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194973_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194973_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 194974_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194974_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 194978_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 194978_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 194979_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194979_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 194989_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194989_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 194991_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194991_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 194996_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 194996_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 195000_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195000_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 195005_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195005_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195007_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195007_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195012_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 195012_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 195016_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195016_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195022_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195022_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195027_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195027_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195035_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195035_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195036_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 195036_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 195039_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195039_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 195045_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 195045_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 195047_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195047_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 195056_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195056_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 195061_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 195061_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 195068_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195068_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195069_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195069_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 195070_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195070_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195074_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 195074_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 195082_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195082_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195088_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195088_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195089_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195089_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 195090_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195090_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195094_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195094_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 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 195116_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195116_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195123_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195123_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195130_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195130_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195131_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 195131_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
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Considering the candidate 195145_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195145_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195151_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195151_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 195153_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195153_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (32.8") between the two second-epoch detections
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Considering the candidate 195159_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195159_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (29.7") between the two second-epoch detections
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Considering the candidate 195188_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195188_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
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Considering the candidate 195202_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195202_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195209_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195209_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195210_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195210_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195211_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195211_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195221_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195221_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195237_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 195237_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140319_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 140319_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109195_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 109195_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (37.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170697_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 170697_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 00:15:50.53 +57:32:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16337_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
The candidate 16337_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101 did not pass the final checks
**** FOUND 23:21:42.84 +50:06:42.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102558_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
Preparing report for the candidate 102558_fd_Cas-04-Q2b1x1_2026-08-27_23-56-31_20.00sec_-0.00C_LIGHT_0101
make_report_in_HTML.sh Phase 2 (HTML assembly): 83s
make_report_in_HTML.sh TOTAL: 975s
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 ####
23:38:14.48 +50:25:54.0
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23:20:05.34 +55:44:17.8
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23:45:24.96 +54:18:51.5
23:21:42.49 +50:06:38.8
23:54:34.26 +51:57:43.2
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00:00:07.97 +51:20:34.4
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00:00:01.36 +53:01:37.5
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00:16:21.72 +53:48:42.7
00:07:27.60 +51:29:05.2
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00:07:09.76 +50:30:14.6
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00:08:29.28 +51:35:14.5
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23:19:01.95 +55:54:17.3
23:44:40.46 +54:40:58.5
23:32:25.39 +57:31:51.7
00:09:56.28 +51:29:47.0
23:22:04.92 +50:07:50.1
23:34:48.44 +54:22:16.9
23:42:43.39 +53:34:06.0
23:52:19.18 +54:21:38.8
23:34:55.94 +51:11:11.8
23:34:27.35 +56:45:26.0
23:19:02.46 +54:30:07.8
23:31:20.91 +52:54:38.0
23:54:30.23 +54:01:29.4
23:48:22.59 +53:58:07.2
23:39:48.32 +51:17:42.2
00:24:43.89 +53:17:18.5
23:19:17.20 +52:12:32.3
23:20:56.42 +53:10:52.9
23:44:37.70 +51:40:35.6
23:19:27.23 +51:48:29.4
23:21:03.75 +49:30:36.1
23:22:36.33 +49:57:50.0
23:33:09.14 +52:28:51.3
23:36:25.62 +50:36:51.0
23:43:28.60 +51:58:13.4
23:30:33.53 +51:17:36.4
23:40:12.45 +51:49:27.7
23:35:09.83 +51:10:28.4
23:19:01.25 +51:51:44.9
23:34:34.54 +50:32:21.8
23:24:33.15 +53:38:51.1
23:18:19.31 +56:04:31.1
23:52:18.62 +50:33:10.0
00:07:28.60 +51:49:30.6
23:38:18.43 +54:09:41.6
00:22:29.93 +51:55:46.7
23:58:42.03 +52:17:51.8
23:09:50.10 +57:19:55.1
00:26:02.62 +52:49:56.8
23:20:29.03 +54:17:15.4
00:26:38.74 +56:33:57.6
23:11:03.57 +57:24:20.6
23:21:35.56 +56:30:06.9
23:16:08.34 +55:39:57.0
########### 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 ####
23:38:14.48 +50:25:54.0
00:19:20.29 +50:14:26.1
23:20:05.34 +55:44:17.8
23:35:14.99 +52:50:25.3
23:45:24.96 +54:18:51.5
23:21:42.49 +50:06:38.8
23:54:34.26 +51:57:43.2
23:34:54.38 +52:08:13.6
00:00:07.97 +51:20:34.4
23:32:44.57 +53:36:12.5
00:25:49.42 +50:28:02.5
23:35:43.98 +55:35:51.8
23:28:15.89 +50:18:04.2
23:22:07.42 +49:54:19.3
23:38:40.09 +56:54:44.7
23:33:21.87 +54:04:28.5
00:19:20.06 +55:37:10.4
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23:25:03.71 +57:01:59.5
23:33:53.29 +55:45:09.2
23:18:03.58 +55:43:10.1
23:31:39.33 +56:24:27.2
23:33:16.96 +55:43:28.3
23:25:14.02 +55:36:09.2
00:04:10.84 +53:29:33.7
23:11:16.06 +56:36:21.6
23:25:35.82 +57:55:06.6
23:34:32.46 +54:30:26.4
23:37:31.07 +54:37:57.2
23:23:31.78 +55:24:15.3
23:18:53.90 +53:45:26.0
23:20:39.97 +55:09:31.8
00:23:24.29 +54:04:50.0
23:42:03.14 +51:28:48.3
23:10:28.92 +57:11:08.3
23:10:29.21 +57:13:04.4
23:26:30.09 +51:45:22.5
23:28:37.29 +56:49:15.5
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00:09:23.43 +51:02:03.8
23:30:35.12 +53:14:45.6
23:11:28.21 +56:37:54.0
23:28:24.32 +51:59:26.8
23:36:27.75 +57:32:22.4
23:19:26.47 +50:59:21.6
00:10:51.20 +52:25:07.5
23:37:04.13 +54:30:54.1
00:13:26.58 +53:19:41.1
23:24:25.61 +53:57:00.3
00:12:38.00 +53:52:11.1
23:15:04.32 +55:33:55.7
23:17:29.14 +51:35:32.9
23:31:42.78 +55:31:56.5
23:18:24.24 +53:43:23.0
23:53:22.44 +53:30:17.8
00:12:29.83 +53:38:35.5
00:10:19.86 +50:21:11.1
00:00:01.36 +53:01:37.5
00:12:07.85 +52:25:18.0
23:51:27.72 +54:14:05.2
23:24:52.09 +54:41:49.4
00:16:21.72 +53:48:42.7
00:07:27.60 +51:29:05.2
00:11:38.66 +54:02:13.9
23:28:01.21 +55:38:38.0
23:11:20.95 +56:24:15.5
23:23:47.98 +53:18:18.4
00:07:09.76 +50:30:14.6
23:38:01.96 +57:01:56.2
23:09:04.86 +57:24:42.0
23:23:36.32 +52:43:39.9
23:21:26.05 +51:16:44.1
23:35:59.42 +51:23:05.6
23:29:05.04 +55:58:56.1
00:13:29.41 +53:19:49.2
23:15:34.34 +55:01:27.8
23:52:55.59 +53:55:19.6
23:43:57.22 +51:35:21.9
23:46:45.03 +50:07:53.8
23:32:52.30 +53:44:57.6
00:25:07.42 +56:25:13.5
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23:42:42.37 +53:38:55.8
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23:29:57.38 +55:09:17.0
23:34:23.08 +50:30:41.4
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23:39:10.80 +52:38:27.8
00:08:58.01 +52:27:28.7
00:03:29.46 +53:34:39.7
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00:08:29.28 +51:35:14.5
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23:31:17.80 +54:01:18.7
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00:05:44.31 +50:40:09.1
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23:25:37.16 +51:45:06.5
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23:26:19.28 +53:47:48.6
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00:10:41.39 +53:58:59.5
23:56:48.43 +50:59:50.3
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23:37:39.47 +51:21:05.3
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00:07:29.15 +51:05:33.0
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23:17:32.53 +56:09:21.0
23:57:13.66 +51:50:40.9
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00:06:07.57 +50:16:46.8
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00:16:59.35 +52:47:31.5
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00:17:09.91 +50:18:49.9
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00:02:47.38 +51:31:20.4
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00:24:08.31 +50:22:15.3
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23:36:30.79 +50:26:34.8
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00:05:32.75 +50:54:18.9
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00:07:16.31 +51:00:11.3
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00:03:29.54 +51:28:01.8
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23:25:12.62 +54:01:38.1
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23:43:52.25 +51:14:12.9
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00:08:00.03 +50:31:24.7
00:25:26.11 +53:44:41.0
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23:44:37.70 +51:40:35.6
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23:33:09.14 +52:28:51.3
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23:30:33.53 +51:17:36.4
23:40:12.45 +51:49:27.7
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23:58:42.03 +52:17:51.8
23:09:50.10 +57:19:55.1
00:26:02.62 +52:49:56.8
23:20:29.03 +54:17:15.4
00:26:38.74 +56:33:57.6
23:11:03.57 +57:24:20.6
23:21:35.56 +56:30:06.9
23:16:08.34 +55:39:57.0
00:19:57.98 +56:35:35.9
23:34:04.31 +55:18:58.3
###################################################################################
23:38:14.48 +50:25:54.0 -- not an asteroid (will add it to exclusion list)
00:19:20.29 +50:14:26.1 -- not an asteroid (will add it to exclusion list)
23:20:05.34 +55:44:17.8 -- not an asteroid (will add it to exclusion list)
23:35:14.99 +52:50:25.3 -- not an asteroid (will add it to exclusion list)
23:45:24.96 +54:18:51.5 -- not an asteroid (will add it to exclusion list)
23:21:42.49 +50:06:38.8 -- not an asteroid (will add it to exclusion list)
23:54:34.26 +51:57:43.2 -- not an asteroid (will add it to exclusion list)
23:34:54.38 +52:08:13.6 -- not an asteroid (will add it to exclusion list)
00:00:07.97 +51:20:34.4 -- not an asteroid (will add it to exclusion list)
23:32:44.57 +53:36:12.5 -- not an asteroid (will add it to exclusion list)
00:25:49.42 +50:28:02.5 -- not an asteroid (will add it to exclusion list)
23:35:43.98 +55:35:51.8 -- not an asteroid (will add it to exclusion list)
23:28:15.89 +50:18:04.2 -- not an asteroid (will add it to exclusion list)
23:22:07.42 +49:54:19.3 -- not an asteroid (will add it to exclusion list)
23:38:40.09 +56:54:44.7 -- not an asteroid (will add it to exclusion list)
23:33:21.87 +54:04:28.5 -- not an asteroid (will add it to exclusion list)
00:19:20.06 +55:37:10.4 -- not an asteroid (will add it to exclusion list)
23:39:28.46 +51:28:27.3 -- not an asteroid (will add it to exclusion list)
23:33:12.21 +50:10:29.9 -- not an asteroid (will add it to exclusion list)
23:25:03.71 +57:01:59.5 -- not an asteroid (will add it to exclusion list)
23:33:53.29 +55:45:09.2 -- not an asteroid (will add it to exclusion list)
23:18:03.58 +55:43:10.1 -- not an asteroid (will add it to exclusion list)
23:31:39.33 +56:24:27.2 -- not an asteroid (will add it to exclusion list)
23:33:16.96 +55:43:28.3 -- not an asteroid (will add it to exclusion list)
23:25:14.02 +55:36:09.2 -- not an asteroid (will add it to exclusion list)
00:04:10.84 +53:29:33.7 -- not an asteroid (will add it to exclusion list)
23:11:16.06 +56:36:21.6 -- not an asteroid (will add it to exclusion list)
23:25:35.82 +57:55:06.6 -- not an asteroid (will add it to exclusion list)
23:34:32.46 +54:30:26.4 -- not an asteroid (will add it to exclusion list)
23:37:31.07 +54:37:57.2 -- not an asteroid (will add it to exclusion list)
23:23:31.78 +55:24:15.3 -- not an asteroid (will add it to exclusion list)
23:18:53.90 +53:45:26.0 -- not an asteroid (will add it to exclusion list)
23:20:39.97 +55:09:31.8 -- not an asteroid (will add it to exclusion list)
00:23:24.29 +54:04:50.0 -- not an asteroid (will add it to exclusion list)
23:42:03.14 +51:28:48.3 -- not an asteroid (will add it to exclusion list)
23:10:28.92 +57:11:08.3 -- not an asteroid (will add it to exclusion list)
23:10:29.21 +57:13:04.4 -- not an asteroid (will add it to exclusion list)
23:26:30.09 +51:45:22.5 -- not an asteroid (will add it to exclusion list)
23:28:37.29 +56:49:15.5 -- not an asteroid (will add it to exclusion list)
23:47:45.19 +49:57:10.9 -- not an asteroid (will add it to exclusion list)
23:48:36.95 +50:34:52.5 -- not an asteroid (will add it to exclusion list)
00:09:23.43 +51:02:03.8 -- not an asteroid (will add it to exclusion list)
23:30:35.12 +53:14:45.6 -- not an asteroid (will add it to exclusion list)
23:11:28.21 +56:37:54.0 -- not an asteroid (will add it to exclusion list)
23:28:24.32 +51:59:26.8 -- not an asteroid (will add it to exclusion list)
23:36:27.75 +57:32:22.4 -- not an asteroid (will add it to exclusion list)
23:19:26.47 +50:59:21.6 -- not an asteroid (will add it to exclusion list)
00:10:51.20 +52:25:07.5 -- not an asteroid (will add it to exclusion list)
23:37:04.13 +54:30:54.1 -- not an asteroid (will add it to exclusion list)
00:13:26.58 +53:19:41.1 -- not an asteroid (will add it to exclusion list)
23:24:25.61 +53:57:00.3 -- not an asteroid (will add it to exclusion list)
00:12:38.00 +53:52:11.1 -- not an asteroid (will add it to exclusion list)
23:15:04.32 +55:33:55.7 -- not an asteroid (will add it to exclusion list)
23:17:29.14 +51:35:32.9 -- not an asteroid (will add it to exclusion list)
23:31:42.78 +55:31:56.5 -- not an asteroid (will add it to exclusion list)
23:18:24.24 +53:43:23.0 -- not an asteroid (will add it to exclusion list)
23:53:22.44 +53:30:17.8 -- not an asteroid (will add it to exclusion list)
00:12:29.83 +53:38:35.5 -- not an asteroid (will add it to exclusion list)
00:10:19.86 +50:21:11.1 -- not an asteroid (will add it to exclusion list)
00:00:01.36 +53:01:37.5 -- not an asteroid (will add it to exclusion list)
00:12:07.85 +52:25:18.0 -- not an asteroid (will add it to exclusion list)
23:51:27.72 +54:14:05.2 -- not an asteroid (will add it to exclusion list)
23:24:52.09 +54:41:49.4 -- not an asteroid (will add it to exclusion list)
00:16:21.72 +53:48:42.7 -- not an asteroid (will add it to exclusion list)
00:07:27.60 +51:29:05.2 -- not an asteroid (will add it to exclusion list)
00:11:38.66 +54:02:13.9 -- not an asteroid (will add it to exclusion list)
23:28:01.21 +55:38:38.0 -- not an asteroid (will add it to exclusion list)
23:11:20.95 +56:24:15.5 -- not an asteroid (will add it to exclusion list)
23:23:47.98 +53:18:18.4 -- not an asteroid (will add it to exclusion list)
00:07:09.76 +50:30:14.6 -- not an asteroid (will add it to exclusion list)
23:38:01.96 +57:01:56.2 -- not an asteroid (will add it to exclusion list)
23:09:04.86 +57:24:42.0 -- not an asteroid (will add it to exclusion list)
23:23:36.32 +52:43:39.9 -- not an asteroid (will add it to exclusion list)
23:21:26.05 +51:16:44.1 -- not an asteroid (will add it to exclusion list)
23:35:59.42 +51:23:05.6 -- not an asteroid (will add it to exclusion list)
23:29:05.04 +55:58:56.1 -- not an asteroid (will add it to exclusion list)
00:13:29.41 +53:19:49.2 -- not an asteroid (will add it to exclusion list)
23:15:34.34 +55:01:27.8 -- not an asteroid (will add it to exclusion list)
23:52:55.59 +53:55:19.6 -- not an asteroid (will add it to exclusion list)
23:43:57.22 +51:35:21.9 -- not an asteroid (will add it to exclusion list)
23:46:45.03 +50:07:53.8 -- not an asteroid (will add it to exclusion list)
23:32:52.30 +53:44:57.6 -- not an asteroid (will add it to exclusion list)
00:25:07.42 +56:25:13.5 -- not an asteroid (will add it to exclusion list)
23:41:50.24 +55:02:54.1 -- not an asteroid (will add it to exclusion list)
23:42:42.37 +53:38:55.8 -- not an asteroid (will add it to exclusion list)
23:34:22.88 +52:49:51.6 -- not an asteroid (will add it to exclusion list)
23:46:00.08 +52:44:54.5 -- not an asteroid (will add it to exclusion list)
23:26:47.97 +57:24:35.9 -- not an asteroid (will add it to exclusion list)
23:16:13.35 +55:12:31.4 -- not an asteroid (will add it to exclusion list)
23:54:00.82 +50:12:59.3 -- not an asteroid (will add it to exclusion list)
23:29:29.10 +51:00:39.4 -- not an asteroid (will add it to exclusion list)
23:29:57.38 +55:09:17.0 -- not an asteroid (will add it to exclusion list)
23:34:23.08 +50:30:41.4 -- not an asteroid (will add it to exclusion list)
23:27:52.16 +57:08:13.7 -- not an asteroid (will add it to exclusion list)
23:39:10.80 +52:38:27.8 -- not an asteroid (will add it to exclusion list)
00:08:58.01 +52:27:28.7 -- not an asteroid (will add it to exclusion list)
00:03:29.46 +53:34:39.7 -- not an asteroid (will add it to exclusion list)
23:09:15.63 +57:16:03.9 -- not an asteroid (will add it to exclusion list)
23:26:02.96 +53:45:44.1 -- not an asteroid (will add it to exclusion list)
23:19:34.37 +50:14:46.9 -- not an asteroid (will add it to exclusion list)
23:17:51.12 +53:37:04.6 -- not an asteroid (will add it to exclusion list)
23:29:02.05 +50:39:49.2 -- not an asteroid (will add it to exclusion list)
23:24:52.23 +53:53:18.9 -- not an asteroid (will add it to exclusion list)
23:24:18.43 +51:34:22.7 -- not an asteroid (will add it to exclusion list)
23:23:04.40 +52:25:37.5 -- not an asteroid (will add it to exclusion list)
00:08:29.28 +51:35:14.5 -- not an asteroid (will add it to exclusion list)
00:04:32.67 +51:18:17.9 -- not an asteroid (will add it to exclusion list)
23:18:26.78 +53:20:30.8 -- not an asteroid (will add it to exclusion list)
23:15:46.07 +57:41:56.2 -- not an asteroid (will add it to exclusion list)
23:16:41.88 +57:37:13.2 -- not an asteroid (will add it to exclusion list)
23:15:56.98 +56:35:14.2 -- not an asteroid (will add it to exclusion list)
23:17:31.57 +57:13:09.0 -- not an asteroid (will add it to exclusion list)
23:32:54.99 +53:38:40.9 -- not an asteroid (will add it to exclusion list)
23:22:19.10 +54:46:28.8 -- not an asteroid (will add it to exclusion list)
23:36:05.96 +54:46:13.3 -- not an asteroid (will add it to exclusion list)
23:31:17.80 +54:01:18.7 -- not an asteroid (will add it to exclusion list)
23:23:47.22 +52:32:55.6 -- not an asteroid (will add it to exclusion list)
00:05:44.31 +50:40:09.1 -- not an asteroid (will add it to exclusion list)
23:18:06.71 +50:59:08.4 -- not an asteroid (will add it to exclusion list)
23:52:25.64 +52:52:42.7 -- not an asteroid (will add it to exclusion list)
23:18:48.13 +50:21:35.5 -- not an asteroid (will add it to exclusion list)
23:38:11.37 +52:05:02.3 -- not an asteroid (will add it to exclusion list)
23:25:37.16 +51:45:06.5 -- not an asteroid (will add it to exclusion list)
23:17:39.13 +56:25:45.6 -- not an asteroid (will add it to exclusion list)
23:26:19.28 +53:47:48.6 -- not an asteroid (will add it to exclusion list)
23:19:52.88 +49:51:22.2 -- not an asteroid (will add it to exclusion list)
23:45:01.22 +55:19:04.4 -- not an asteroid (will add it to exclusion list)
00:10:41.39 +53:58:59.5 -- not an asteroid (will add it to exclusion list)
23:56:48.43 +50:59:50.3 -- not an asteroid (will add it to exclusion list)
23:21:29.67 +54:16:21.5 -- not an asteroid (will add it to exclusion list)
23:28:38.20 +51:01:20.5 -- not an asteroid (will add it to exclusion list)
23:30:52.31 +54:23:23.5 -- not an asteroid (will add it to exclusion list)
23:37:39.47 +51:21:05.3 -- not an asteroid (will add it to exclusion list)
00:08:10.60 +52:36:10.1 -- not an asteroid (will add it to exclusion list)
23:30:21.39 +50:22:09.6 -- not an asteroid (will add it to exclusion list)
00:20:28.23 +54:57:49.1 -- not an asteroid (will add it to exclusion list)
23:43:35.35 +55:18:49.6 -- not an asteroid (will add it to exclusion list)
23:53:59.45 +50:05:18.9 -- not an asteroid (will add it to exclusion list)
23:40:12.92 +55:26:29.3 -- not an asteroid (will add it to exclusion list)
00:07:29.15 +51:05:33.0 -- not an asteroid (will add it to exclusion list)
23:39:36.07 +51:31:08.8 -- not an asteroid (will add it to exclusion list)
23:18:04.96 +55:30:11.1 -- not an asteroid (will add it to exclusion list)
23:17:32.53 +56:09:21.0 -- not an asteroid (will add it to exclusion list)
23:57:13.66 +51:50:40.9 -- not an asteroid (will add it to exclusion list)
23:23:07.34 +49:28:50.7 -- not an asteroid (will add it to exclusion list)
00:06:07.57 +50:16:46.8 -- not an asteroid (will add it to exclusion list)
23:23:13.80 +51:43:35.2 -- not an asteroid (will add it to exclusion list)
23:30:43.51 +55:32:50.3 -- not an asteroid (will add it to exclusion list)
23:24:54.00 +51:36:31.5 -- not an asteroid (will add it to exclusion list)
23:14:42.54 +55:59:12.5 -- not an asteroid (will add it to exclusion list)
23:59:31.46 +54:09:40.4 -- not an asteroid (will add it to exclusion list)
23:17:49.47 +51:39:33.9 -- not an asteroid (will add it to exclusion list)
23:35:50.44 +54:56:06.3 -- not an asteroid (will add it to exclusion list)
00:07:34.46 +51:47:00.5 -- not an asteroid (will add it to exclusion list)
23:35:16.90 +50:04:40.1 -- not an asteroid (will add it to exclusion list)
23:39:11.14 +57:04:18.8 -- not an asteroid (will add it to exclusion list)
23:30:06.64 +55:31:12.4 -- not an asteroid (will add it to exclusion list)
00:16:59.35 +52:47:31.5 -- not an asteroid (will add it to exclusion list)
23:23:12.70 +56:57:56.7 -- not an asteroid (will add it to exclusion list)
23:45:23.37 +50:21:07.2 -- not an asteroid (will add it to exclusion list)
00:19:26.40 +49:42:31.1 -- not an asteroid (will add it to exclusion list)
00:06:29.74 +51:42:56.0 -- not an asteroid (will add it to exclusion list)
23:27:25.43 +56:44:45.4 -- not an asteroid (will add it to exclusion list)
23:38:26.80 +56:58:36.3 -- not an asteroid (will add it to exclusion list)
23:27:41.36 +54:21:24.4 -- not an asteroid (will add it to exclusion list)
23:23:09.84 +53:47:00.6 -- not an asteroid (will add it to exclusion list)
23:13:46.60 +54:38:25.2 -- not an asteroid (will add it to exclusion list)
23:11:38.67 +56:35:48.7 -- not an asteroid (will add it to exclusion list)
23:31:16.51 +51:15:13.0 -- not an asteroid (will add it to exclusion list)
00:16:18.85 +56:42:06.0 -- not an asteroid (will add it to exclusion list)
23:12:08.53 +57:31:17.6 -- not an asteroid (will add it to exclusion list)
23:34:14.03 +52:18:18.2 -- not an asteroid (will add it to exclusion list)
23:17:18.12 +56:04:16.7 -- not an asteroid (will add it to exclusion list)
23:59:22.19 +50:46:57.6 -- not an asteroid (will add it to exclusion list)
00:00:44.99 +52:08:03.4 -- not an asteroid (will add it to exclusion list)
23:26:05.54 +54:30:20.9 -- not an asteroid (will add it to exclusion list)
23:33:46.42 +50:32:46.8 -- not an asteroid (will add it to exclusion list)
23:30:40.30 +54:19:13.7 -- not an asteroid (will add it to exclusion list)
23:42:33.85 +53:51:34.2 -- not an asteroid (will add it to exclusion list)
23:49:27.48 +51:58:31.5 -- not an asteroid (will add it to exclusion list)
23:58:27.86 +52:16:14.1 -- not an asteroid (will add it to exclusion list)
23:23:34.50 +52:08:32.1 -- not an asteroid (will add it to exclusion list)
23:52:37.11 +53:51:53.0 -- not an asteroid (will add it to exclusion list)
00:10:19.20 +51:21:32.1 -- not an asteroid (will add it to exclusion list)
23:36:52.38 +55:44:54.7 -- not an asteroid (will add it to exclusion list)
23:16:05.69 +53:59:27.5 -- not an asteroid (will add it to exclusion list)
00:17:09.91 +50:18:49.9 -- not an asteroid (will add it to exclusion list)
00:08:05.50 +51:46:22.3 -- not an asteroid (will add it to exclusion list)
23:27:04.72 +55:04:53.5 -- not an asteroid (will add it to exclusion list)
00:06:32.90 +54:39:32.0 -- not an asteroid (will add it to exclusion list)
23:14:26.97 +57:33:59.7 -- not an asteroid (will add it to exclusion list)
23:22:41.71 +50:08:48.8 -- not an asteroid (will add it to exclusion list)
23:17:19.53 +55:48:30.3 -- not an asteroid (will add it to exclusion list)
23:24:52.56 +55:09:33.4 -- not an asteroid (will add it to exclusion list)
23:18:52.99 +54:59:05.7 -- not an asteroid (will add it to exclusion list)
23:31:49.97 +56:40:30.7 -- not an asteroid (will add it to exclusion list)
23:14:33.20 +57:06:08.3 -- not an asteroid (will add it to exclusion list)
23:24:02.23 +55:45:42.7 -- not an asteroid (will add it to exclusion list)
00:07:46.77 +54:40:41.9 -- not an asteroid (will add it to exclusion list)
23:22:30.34 +55:44:27.1 -- not an asteroid (will add it to exclusion list)
23:21:36.05 +52:40:17.3 -- not an asteroid (will add it to exclusion list)
23:38:06.02 +51:03:58.2 -- not an asteroid (will add it to exclusion list)
23:46:39.65 +50:07:15.9 -- not an asteroid (will add it to exclusion list)
23:30:38.22 +55:00:24.1 -- not an asteroid (will add it to exclusion list)
23:24:06.72 +51:31:34.1 -- not an asteroid (will add it to exclusion list)
23:14:16.98 +56:27:23.4 -- not an asteroid (will add it to exclusion list)
00:02:47.38 +51:31:20.4 -- not an asteroid (will add it to exclusion list)
23:21:31.13 +51:34:43.0 -- not an asteroid (will add it to exclusion list)
00:24:08.31 +50:22:15.3 -- not an asteroid (will add it to exclusion list)
23:15:46.19 +55:44:39.1 -- not an asteroid (will add it to exclusion list)
23:15:30.94 +55:29:10.7 -- not an asteroid (will add it to exclusion list)
23:19:52.02 +49:24:30.4 -- not an asteroid (will add it to exclusion list)
23:25:50.46 +54:19:34.7 -- not an asteroid (will add it to exclusion list)
23:30:41.60 +51:38:08.5 -- not an asteroid (will add it to exclusion list)
23:54:20.86 +51:29:40.6 -- not an asteroid (will add it to exclusion list)
23:41:48.03 +51:06:34.3 -- not an asteroid (will add it to exclusion list)
23:22:50.20 +51:55:38.5 -- not an asteroid (will add it to exclusion list)
23:23:17.36 +55:37:43.3 -- not an asteroid (will add it to exclusion list)
23:45:28.49 +54:37:56.6 -- not an asteroid (will add it to exclusion list)
23:55:31.73 +51:24:35.3 -- not an asteroid (will add it to exclusion list)
23:20:42.25 +52:15:34.7 -- not an asteroid (will add it to exclusion list)
23:36:30.79 +50:26:34.8 -- not an asteroid (will add it to exclusion list)
23:27:27.22 +52:12:45.3 -- not an asteroid (will add it to exclusion list)
23:10:36.58 +56:49:29.7 -- not an asteroid (will add it to exclusion list)
23:43:54.73 +53:29:50.5 -- not an asteroid (will add it to exclusion list)
23:19:05.21 +50:33:42.9 -- not an asteroid (will add it to exclusion list)
23:37:43.66 +50:45:05.0 -- not an asteroid (will add it to exclusion list)
00:05:32.75 +50:54:18.9 -- not an asteroid (will add it to exclusion list)
23:30:32.15 +54:54:01.6 -- not an asteroid (will add it to exclusion list)
23:20:38.47 +54:42:03.0 -- not an asteroid (will add it to exclusion list)
23:18:17.24 +54:09:17.2 -- not an asteroid (will add it to exclusion list)
00:20:40.54 +52:18:07.6 -- not an asteroid (will add it to exclusion list)
23:15:06.10 +56:02:21.3 -- not an asteroid (will add it to exclusion list)
23:38:16.32 +56:01:28.1 -- not an asteroid (will add it to exclusion list)
23:12:55.82 +55:28:00.1 -- not an asteroid (will add it to exclusion list)
23:32:12.56 +57:11:42.1 -- not an asteroid (will add it to exclusion list)
23:21:10.38 +55:54:00.5 -- not an asteroid (will add it to exclusion list)
23:12:00.73 +56:27:20.8 -- not an asteroid (will add it to exclusion list)
00:07:16.31 +51:00:11.3 -- not an asteroid (will add it to exclusion list)
23:35:42.50 +52:19:08.8 -- not an asteroid (will add it to exclusion list)
23:30:13.36 +55:17:29.0 -- not an asteroid (will add it to exclusion list)
23:41:59.95 +54:41:41.0 -- not an asteroid (will add it to exclusion list)
23:12:59.24 +56:18:47.6 -- not an asteroid (will add it to exclusion list)
23:32:51.32 +54:47:13.9 -- not an asteroid (will add it to exclusion list)
23:23:37.36 +52:10:37.1 -- not an asteroid (will add it to exclusion list)
00:24:44.88 +53:56:10.0 -- not an asteroid (will add it to exclusion list)
00:11:25.51 +51:27:46.6 -- not an asteroid (will add it to exclusion list)
23:17:13.51 +56:09:04.4 -- not an asteroid (will add it to exclusion list)
23:42:01.24 +52:33:44.2 -- not an asteroid (will add it to exclusion list)
23:10:20.45 +56:50:57.4 -- not an asteroid (will add it to exclusion list)
23:24:13.25 +57:04:21.3 -- not an asteroid (will add it to exclusion list)
23:13:11.90 +55:44:22.2 -- not an asteroid (will add it to exclusion list)
23:13:46.75 +55:05:40.2 -- not an asteroid (will add it to exclusion list)
23:57:03.64 +52:12:14.7 -- not an asteroid (will add it to exclusion list)
23:43:56.31 +50:48:29.6 -- not an asteroid (will add it to exclusion list)
23:13:43.46 +55:17:10.3 -- not an asteroid (will add it to exclusion list)
23:36:56.18 +53:26:38.5 -- not an asteroid (will add it to exclusion list)
23:35:07.39 +50:23:49.7 -- not an asteroid (will add it to exclusion list)
23:18:28.53 +51:19:29.9 -- not an asteroid (will add it to exclusion list)
00:14:23.52 +53:09:22.5 -- not an asteroid (will add it to exclusion list)
23:46:19.77 +51:19:58.5 -- not an asteroid (will add it to exclusion list)
23:17:55.99 +56:24:54.8 -- not an asteroid (will add it to exclusion list)
23:37:56.65 +56:26:03.7 -- not an asteroid (will add it to exclusion list)
23:15:11.52 +57:21:43.1 -- not an asteroid (will add it to exclusion list)
00:09:56.98 +50:50:46.1 -- not an asteroid (will add it to exclusion list)
23:14:18.44 +57:19:41.7 -- not an asteroid (will add it to exclusion list)
00:22:11.58 +52:16:55.0 -- not an asteroid (will add it to exclusion list)
23:26:02.05 +54:34:25.4 -- not an asteroid (will add it to exclusion list)
23:19:24.23 +54:26:59.2 -- not an asteroid (will add it to exclusion list)
23:45:40.78 +51:00:36.0 -- not an asteroid (will add it to exclusion list)
23:19:13.36 +52:17:54.8 -- not an asteroid (will add it to exclusion list)
23:23:12.46 +54:50:18.9 -- not an asteroid (will add it to exclusion list)
23:55:59.18 +52:04:34.3 -- not an asteroid (will add it to exclusion list)
23:58:37.65 +53:26:04.7 -- not an asteroid (will add it to exclusion list)
23:23:22.45 +51:40:47.7 -- not an asteroid (will add it to exclusion list)
23:17:53.16 +53:31:56.3 -- not an asteroid (will add it to exclusion list)
23:34:13.73 +55:20:19.5 -- not an asteroid (will add it to exclusion list)
23:19:18.81 +51:15:50.4 -- not an asteroid (will add it to exclusion list)
23:21:29.75 +53:08:48.8 -- not an asteroid (will add it to exclusion list)
23:45:18.59 +50:50:13.5 -- not an asteroid (will add it to exclusion list)
23:40:03.08 +50:31:06.4 -- not an asteroid (will add it to exclusion list)
23:22:55.30 +54:14:50.9 -- not an asteroid (will add it to exclusion list)
23:20:39.70 +55:02:04.7 -- not an asteroid (will add it to exclusion list)
23:28:08.91 +50:26:16.2 -- not an asteroid (will add it to exclusion list)
23:20:02.13 +49:55:45.5 -- not an asteroid (will add it to exclusion list)
23:20:09.39 +49:57:06.1 -- not an asteroid (will add it to exclusion list)
23:40:20.54 +54:40:25.9 -- not an asteroid (will add it to exclusion list)
23:11:29.53 +55:33:26.0 -- not an asteroid (will add it to exclusion list)
23:14:58.79 +55:26:18.0 -- not an asteroid (will add it to exclusion list)
23:20:52.75 +50:30:13.3 -- not an asteroid (will add it to exclusion list)
23:30:36.43 +50:51:22.0 -- not an asteroid (will add it to exclusion list)
23:42:07.04 +54:29:32.0 -- not an asteroid (will add it to exclusion list)
00:05:13.07 +51:50:35.0 -- not an asteroid (will add it to exclusion list)
23:39:43.83 +50:34:48.1 -- not an asteroid (will add it to exclusion list)
23:30:29.85 +54:34:21.0 -- not an asteroid (will add it to exclusion list)
23:18:52.90 +51:20:13.1 -- not an asteroid (will add it to exclusion list)
23:31:54.45 +55:25:34.1 -- not an asteroid (will add it to exclusion list)
23:18:39.75 +50:05:36.4 -- not an asteroid (will add it to exclusion list)
23:19:38.04 +50:35:21.3 -- not an asteroid (will add it to exclusion list)
23:33:45.37 +54:02:56.4 -- not an asteroid (will add it to exclusion list)
00:08:59.67 +50:29:49.5 -- not an asteroid (will add it to exclusion list)
23:31:48.80 +49:59:03.6 -- not an asteroid (will add it to exclusion list)
23:18:53.97 +54:28:24.4 -- not an asteroid (will add it to exclusion list)
23:42:24.64 +53:39:51.6 -- not an asteroid (will add it to exclusion list)
23:22:55.83 +53:23:01.2 -- not an asteroid (will add it to exclusion list)
23:26:17.36 +55:31:52.1 -- not an asteroid (will add it to exclusion list)
23:20:55.73 +54:36:44.9 -- not an asteroid (will add it to exclusion list)
00:01:38.26 +50:38:25.8 -- not an asteroid (will add it to exclusion list)
23:35:28.82 +56:19:45.8 -- not an asteroid (will add it to exclusion list)
23:37:16.30 +51:29:54.6 -- not an asteroid (will add it to exclusion list)
23:30:10.24 +49:54:50.3 -- not an asteroid (will add it to exclusion list)
23:22:06.03 +53:17:47.4 -- not an asteroid (will add it to exclusion list)
23:19:30.68 +55:40:18.3 -- not an asteroid (will add it to exclusion list)
00:00:42.73 +51:44:33.3 -- not an asteroid (will add it to exclusion list)
23:40:46.84 +50:21:18.3 -- not an asteroid (will add it to exclusion list)
23:30:11.92 +56:22:07.2 -- not an asteroid (will add it to exclusion list)
23:18:58.56 +54:09:25.0 -- not an asteroid (will add it to exclusion list)
23:25:40.16 +54:34:40.4 -- not an asteroid (will add it to exclusion list)
23:36:13.21 +51:20:23.4 -- not an asteroid (will add it to exclusion list)
23:23:02.09 +51:27:45.7 -- not an asteroid (will add it to exclusion list)
23:31:12.32 +50:01:53.6 -- not an asteroid (will add it to exclusion list)
23:48:55.40 +52:57:31.1 -- not an asteroid (will add it to exclusion list)
23:20:22.98 +50:39:45.9 -- not an asteroid (will add it to exclusion list)
23:49:21.12 +50:23:22.7 -- not an asteroid (will add it to exclusion list)
00:24:27.13 +54:50:40.5 -- not an asteroid (will add it to exclusion list)
00:08:31.57 +52:43:57.6 -- not an asteroid (will add it to exclusion list)
23:49:17.93 +50:14:11.3 -- not an asteroid (will add it to exclusion list)
23:20:41.10 +49:38:25.8 -- not an asteroid (will add it to exclusion list)
23:37:28.30 +55:09:05.4 -- not an asteroid (will add it to exclusion list)
23:22:43.60 +51:19:45.4 -- not an asteroid (will add it to exclusion list)
23:37:26.45 +50:09:49.4 -- not an asteroid (will add it to exclusion list)
23:16:32.51 +55:23:17.9 -- not an asteroid (will add it to exclusion list)
23:25:13.81 +51:29:54.3 -- not an asteroid (will add it to exclusion list)
23:32:19.47 +55:17:56.4 -- not an asteroid (will add it to exclusion list)
23:59:59.89 +53:02:02.6 -- not an asteroid (will add it to exclusion list)
23:34:38.18 +52:09:25.3 -- not an asteroid (will add it to exclusion list)
23:40:24.59 +51:36:30.4 -- not an asteroid (will add it to exclusion list)
23:45:27.28 +54:31:03.7 -- not an asteroid (will add it to exclusion list)
23:44:12.54 +51:12:02.8 -- not an asteroid (will add it to exclusion list)
23:59:42.82 +53:21:57.0 -- not an asteroid (will add it to exclusion list)
23:33:42.34 +53:53:39.6 -- not an asteroid (will add it to exclusion list)
23:26:38.84 +55:07:00.1 -- not an asteroid (will add it to exclusion list)
00:13:23.95 +51:50:59.6 -- not an asteroid (will add it to exclusion list)
23:40:53.24 +53:47:05.7 -- not an asteroid (will add it to exclusion list)
23:22:01.22 +53:10:19.2 -- not an asteroid (will add it to exclusion list)
23:31:14.34 +51:34:01.0 -- not an asteroid (will add it to exclusion list)
23:39:45.96 +51:11:03.9 -- not an asteroid (will add it to exclusion list)
23:30:36.18 +54:38:27.4 -- not an asteroid (will add it to exclusion list)
23:18:17.92 +53:44:14.7 -- not an asteroid (will add it to exclusion list)
23:41:40.88 +51:46:14.0 -- not an asteroid (will add it to exclusion list)
23:38:10.01 +50:55:36.5 -- not an asteroid (will add it to exclusion list)
23:19:02.25 +55:54:02.7 -- not an asteroid (will add it to exclusion list)
00:04:39.10 +50:18:00.2 -- not an asteroid (will add it to exclusion list)
23:29:27.14 +50:48:42.5 -- not an asteroid (will add it to exclusion list)
23:27:53.79 +50:38:36.4 -- not an asteroid (will add it to exclusion list)
23:18:11.41 +54:19:57.5 -- not an asteroid (will add it to exclusion list)
23:35:12.04 +54:13:18.5 -- not an asteroid (will add it to exclusion list)
23:22:28.19 +54:17:33.2 -- not an asteroid (will add it to exclusion list)
23:38:09.64 +50:41:37.0 -- not an asteroid (will add it to exclusion list)
23:12:49.41 +54:42:07.9 -- not an asteroid (will add it to exclusion list)
23:20:47.45 +49:41:56.4 -- not an asteroid (will add it to exclusion list)
00:20:06.47 +55:24:13.8 -- not an asteroid (will add it to exclusion list)
23:37:52.25 +50:23:10.1 -- not an asteroid (will add it to exclusion list)
23:49:43.32 +50:42:41.7 -- not an asteroid (will add it to exclusion list)
23:50:33.67 +50:47:47.1 -- not an asteroid (will add it to exclusion list)
00:13:12.27 +50:29:47.9 -- not an asteroid (will add it to exclusion list)
23:17:16.38 +51:02:57.6 -- not an asteroid (will add it to exclusion list)
23:29:56.83 +51:09:25.5 -- not an asteroid (will add it to exclusion list)
23:34:13.54 +56:18:02.1 -- not an asteroid (will add it to exclusion list)
23:36:06.52 +55:53:51.7 -- not an asteroid (will add it to exclusion list)
00:03:29.54 +51:28:01.8 -- not an asteroid (will add it to exclusion list)
00:03:44.44 +50:01:24.4 -- not an asteroid (will add it to exclusion list)
23:13:07.51 +56:44:48.1 -- not an asteroid (will add it to exclusion list)
23:25:12.62 +54:01:38.1 -- not an asteroid (will add it to exclusion list)
23:16:30.14 +57:22:30.2 -- not an asteroid (will add it to exclusion list)
23:43:52.25 +51:14:12.9 -- not an asteroid (will add it to exclusion list)
23:22:16.77 +52:07:23.0 -- not an asteroid (will add it to exclusion list)
00:08:00.03 +50:31:24.7 -- not an asteroid (will add it to exclusion list)
00:25:26.11 +53:44:41.0 -- not an asteroid (will add it to exclusion list)
23:55:18.97 +53:33:58.1 -- not an asteroid (will add it to exclusion list)
00:13:10.45 +50:30:07.3 -- not an asteroid (will add it to exclusion list)
23:11:05.31 +56:36:32.0 -- not an asteroid (will add it to exclusion list)
23:15:48.11 +56:59:18.1 -- not an asteroid (will add it to exclusion list)
23:28:43.61 +56:40:16.9 -- not an asteroid (will add it to exclusion list)
23:31:25.50 +52:51:49.0 -- not an asteroid (will add it to exclusion list)
23:27:34.88 +57:18:22.3 -- not an asteroid (will add it to exclusion list)
00:12:57.02 +51:31:46.9 -- not an asteroid (will add it to exclusion list)
23:15:39.64 +52:17:05.5 -- not an asteroid (will add it to exclusion list)
00:12:14.63 +53:43:20.0 -- not an asteroid (will add it to exclusion list)
00:09:18.60 +53:05:18.0 -- not an asteroid (will add it to exclusion list)
00:24:08.76 +50:06:52.4 -- not an asteroid (will add it to exclusion list)
00:18:53.29 +52:28:12.8 -- not an asteroid (will add it to exclusion list)
23:29:01.56 +50:30:26.5 -- not an asteroid (will add it to exclusion list)
23:44:26.65 +52:35:34.9 -- not an asteroid (will add it to exclusion list)
23:28:53.48 +49:44:55.5 -- not an asteroid (will add it to exclusion list)
23:19:01.95 +55:54:17.3 -- not an asteroid (will add it to exclusion list)
23:44:40.46 +54:40:58.5 -- not an asteroid (will add it to exclusion list)
23:32:25.39 +57:31:51.7 -- not an asteroid (will add it to exclusion list)
00:09:56.28 +51:29:47.0 -- not an asteroid (will add it to exclusion list)
23:22:04.92 +50:07:50.1 -- not an asteroid (will add it to exclusion list)
23:34:48.44 +54:22:16.9 -- not an asteroid (will add it to exclusion list)
23:42:43.39 +53:34:06.0 -- not an asteroid (will add it to exclusion list)
23:52:19.18 +54:21:38.8 -- not an asteroid (will add it to exclusion list)
23:34:55.94 +51:11:11.8 -- not an asteroid (will add it to exclusion list)
23:34:27.35 +56:45:26.0 -- not an asteroid (will add it to exclusion list)
23:19:02.46 +54:30:07.8 -- not an asteroid (will add it to exclusion list)
23:31:20.91 +52:54:38.0 -- not an asteroid (will add it to exclusion list)
23:54:30.23 +54:01:29.4 -- not an asteroid (will add it to exclusion list)
23:48:22.59 +53:58:07.2 -- not an asteroid (will add it to exclusion list)
23:39:48.32 +51:17:42.2 -- not an asteroid (will add it to exclusion list)
00:24:43.89 +53:17:18.5 -- not an asteroid (will add it to exclusion list)
23:19:17.20 +52:12:32.3 -- not an asteroid (will add it to exclusion list)
23:20:56.42 +53:10:52.9 -- not an asteroid (will add it to exclusion list)
23:44:37.70 +51:40:35.6 -- not an asteroid (will add it to exclusion list)
23:19:27.23 +51:48:29.4 -- not an asteroid (will add it to exclusion list)
23:21:03.75 +49:30:36.1 -- not an asteroid (will add it to exclusion list)
23:22:36.33 +49:57:50.0 -- not an asteroid (will add it to exclusion list)
23:33:09.14 +52:28:51.3 -- not an asteroid (will add it to exclusion list)
23:36:25.62 +50:36:51.0 -- not an asteroid (will add it to exclusion list)
23:43:28.60 +51:58:13.4 -- not an asteroid (will add it to exclusion list)
23:30:33.53 +51:17:36.4 -- not an asteroid (will add it to exclusion list)
23:40:12.45 +51:49:27.7 -- not an asteroid (will add it to exclusion list)
23:35:09.83 +51:10:28.4 -- not an asteroid (will add it to exclusion list)
23:19:01.25 +51:51:44.9 -- not an asteroid (will add it to exclusion list)
23:34:34.54 +50:32:21.8 -- not an asteroid (will add it to exclusion list)
23:24:33.15 +53:38:51.1 -- not an asteroid (will add it to exclusion list)
23:18:19.31 +56:04:31.1 -- not an asteroid (will add it to exclusion list)
23:52:18.62 +50:33:10.0 -- not an asteroid (will add it to exclusion list)
00:07:28.60 +51:49:30.6 -- not an asteroid (will add it to exclusion list)
23:38:18.43 +54:09:41.6 -- not an asteroid (will add it to exclusion list)
00:22:29.93 +51:55:46.7 -- not an asteroid (will add it to exclusion list)
23:58:42.03 +52:17:51.8 -- not an asteroid (will add it to exclusion list)
23:09:50.10 +57:19:55.1 -- not an asteroid (will add it to exclusion list)
00:26:02.62 +52:49:56.8 -- not an asteroid (will add it to exclusion list)
23:20:29.03 +54:17:15.4 -- not an asteroid (will add it to exclusion list)
00:26:38.74 +56:33:57.6 -- not an asteroid (will add it to exclusion list)
23:11:03.57 +57:24:20.6 -- not an asteroid (will add it to exclusion list)
23:21:35.56 +56:30:06.9 -- not an asteroid (will add it to exclusion list)
23:16:08.34 +55:39:57.0 -- not an asteroid (will add it to exclusion list)
00:19:57.98 +56:35:35.9 -- not an asteroid (will add it to exclusion list)
23:34:04.31 +55:18:58.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:00:01.36 +53:01:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:00:07.97 +51:20:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:00:42.73 +51:44:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:00:44.99 +52:08:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:38.26 +50:38:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:47.38 +51:31:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:29.46 +53:34:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:29.54 +51:28:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:44.44 +50:01:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:10.84 +53:29:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:32.67 +51:18:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:39.10 +50:18:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:13.07 +51:50:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:32.75 +50:54:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:44.31 +50:40:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:07.57 +50:16:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:29.74 +51:42:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:32.90 +54:39:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:09.76 +50:30:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:16.31 +51:00:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:27.60 +51:29:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:28.60 +51:49:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:29.15 +51:05:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:34.46 +51:47:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:46.77 +54:40:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:00.03 +50:31:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:05.50 +51:46:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:10.60 +52:36:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:29.28 +51:35:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:31.57 +52:43:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:58.01 +52:27:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:59.67 +50:29:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:18.60 +53:05:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:23.43 +51:02:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:56.28 +51:29:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:56.98 +50:50:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:19.20 +51:21:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:19.86 +50:21:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:41.39 +53:58:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:51.20 +52:25:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:25.51 +51:27:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:38.66 +54:02:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:07.85 +52:25:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:14.63 +53:43:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:29.83 +53:38:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:38.00 +53:52:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:57.02 +51:31:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:10.45 +50:30:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:12.27 +50:29:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:23.95 +51:50:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:26.58 +53:19:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:13:29.41 +53:19:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:23.52 +53:09:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:18.85 +56:42:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:21.72 +53:48:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:59.35 +52:47:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:09.91 +50:18:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:53.29 +52:28:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:20.06 +55:37:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:20.29 +50:14:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:26.40 +49:42:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:57.98 +56:35:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:06.47 +55:24:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:28.23 +54:57:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:40.54 +52:18:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:11.58 +52:16:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:29.93 +51:55:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:23:24.29 +54:04:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:08.31 +50:22:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:08.76 +50:06:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:27.13 +54:50:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:43.89 +53:17:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:44.88 +53:56:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:07.42 +56:25:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:26.11 +53:44:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:49.42 +50:28:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:02.62 +52:49:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:38.74 +56:33:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:04.86 +57:24:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:15.63 +57:16:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:09:50.10 +57:19:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:20.45 +56:50:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:28.92 +57:11:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:29.21 +57:13:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:36.58 +56:49:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:03.57 +57:24:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:05.31 +56:36:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:16.06 +56:36:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:20.95 +56:24:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:28.21 +56:37:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:29.53 +55:33:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:38.67 +56:35:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:00.73 +56:27:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:08.53 +57:31:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:49.41 +54:42:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:55.82 +55:28:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:59.24 +56:18:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:07.51 +56:44:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:11.90 +55:44:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:43.46 +55:17:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:46.60 +54:38:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:46.75 +55:05:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:16.98 +56:27:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:18.44 +57:19:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:26.97 +57:33:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:33.20 +57:06:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:42.54 +55:59:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:58.79 +55:26:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:04.32 +55:33:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:06.10 +56:02:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:11.52 +57:21:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:30.94 +55:29:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:34.34 +55:01:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:39.64 +52:17:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:46.07 +57:41:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:46.19 +55:44:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:48.11 +56:59:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:56.98 +56:35:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:05.69 +53:59:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:08.34 +55:39:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:13.35 +55:12:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:30.14 +57:22:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:32.51 +55:23:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:41.88 +57:37:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:13.51 +56:09:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:16.38 +51:02:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:18.12 +56:04:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:19.53 +55:48:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:29.14 +51:35:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:31.57 +57:13:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:32.53 +56:09:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:39.13 +56:25:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:49.47 +51:39:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:51.12 +53:37:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:53.16 +53:31:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:55.99 +56:24:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:03.58 +55:43:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:04.96 +55:30:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:06.71 +50:59:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:11.41 +54:19:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:17.24 +54:09:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:17.92 +53:44:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:19.31 +56:04:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:24.24 +53:43:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:26.78 +53:20:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:28.53 +51:19:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:39.75 +50:05:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:48.13 +50:21:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:52.90 +51:20:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:52.99 +54:59:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:53.90 +53:45:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:53.97 +54:28:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:58.56 +54:09:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:01.25 +51:51:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:01.95 +55:54:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:02.25 +55:54:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:02.46 +54:30:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:05.21 +50:33:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:13.36 +52:17:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:17.20 +52:12:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:18.81 +51:15:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:24.23 +54:26:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:26.47 +50:59:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:27.23 +51:48:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:30.68 +55:40:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:34.37 +50:14:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:38.04 +50:35:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:52.02 +49:24:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:52.88 +49:51:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:02.13 +49:55:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:05.34 +55:44:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:09.39 +49:57:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:22.98 +50:39:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:29.03 +54:17:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:38.47 +54:42:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:39.70 +55:02:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:39.97 +55:09:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:41.10 +49:38:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:42.25 +52:15:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:47.45 +49:41:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:52.75 +50:30:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:55.73 +54:36:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:56.42 +53:10:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:03.75 +49:30:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:10.38 +55:54:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:26.05 +51:16:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:29.67 +54:16:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:29.75 +53:08:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:31.13 +51:34:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:35.56 +56:30:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:36.05 +52:40:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:42.49 +50:06:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:01.22 +53:10:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:04.92 +50:07:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:06.03 +53:17:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:07.42 +49:54:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:16.77 +52:07:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:19.10 +54:46:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:28.19 +54:17:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:30.34 +55:44:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:36.33 +49:57:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:41.71 +50:08:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:43.60 +51:19:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:50.20 +51:55:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:55.30 +54:14:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:55.83 +53:23:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:02.09 +51:27:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:04.40 +52:25:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:07.34 +49:28:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:09.84 +53:47:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:12.46 +54:50:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:12.70 +56:57:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:13.80 +51:43:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:17.36 +55:37:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:22.45 +51:40:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:31.78 +55:24:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:34.50 +52:08:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:36.32 +52:43:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:37.36 +52:10:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:47.22 +52:32:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:47.98 +53:18:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:02.23 +55:45:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:06.72 +51:31:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:13.25 +57:04:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:18.43 +51:34:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:25.61 +53:57:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:33.15 +53:38:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:52.09 +54:41:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:52.23 +53:53:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:52.56 +55:09:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:54.00 +51:36:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:03.71 +57:01:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:12.62 +54:01:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:13.81 +51:29:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:14.02 +55:36:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:35.82 +57:55:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:37.16 +51:45:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:40.16 +54:34:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:50.46 +54:19:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:02.05 +54:34:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:02.96 +53:45:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:05.54 +54:30:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:17.36 +55:31:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:19.28 +53:47:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:30.09 +51:45:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:38.84 +55:07:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:47.97 +57:24:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:04.72 +55:04:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:25.43 +56:44:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:27.22 +52:12:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:34.88 +57:18:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:41.36 +54:21:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:52.16 +57:08:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:53.79 +50:38:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:01.21 +55:38:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:08.91 +50:26:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:15.89 +50:18:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:24.32 +51:59:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:37.29 +56:49:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:38.20 +51:01:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:43.61 +56:40:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:53.48 +49:44:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:01.56 +50:30:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:02.05 +50:39:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:05.04 +55:58:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:27.14 +50:48:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:29.10 +51:00:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:56.83 +51:09:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:57.38 +55:09:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:06.64 +55:31:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:10.24 +49:54:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:11.92 +56:22:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:13.36 +55:17:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:21.39 +50:22:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:29.85 +54:34:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:32.15 +54:54:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:33.53 +51:17:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:35.12 +53:14:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:36.18 +54:38:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:36.43 +50:51:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:38.22 +55:00:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:40.30 +54:19:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:41.60 +51:38:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:43.51 +55:32:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:52.31 +54:23:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:12.32 +50:01:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:14.34 +51:34:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:16.51 +51:15:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:17.80 +54:01:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:20.91 +52:54:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:25.50 +52:51:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:39.33 +56:24:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:42.78 +55:31:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:48.80 +49:59:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:49.97 +56:40:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:54.45 +55:25:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:12.56 +57:11:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:19.47 +55:17:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:25.39 +57:31:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:44.57 +53:36:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:51.32 +54:47:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:52.30 +53:44:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:54.99 +53:38:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:09.14 +52:28:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:12.21 +50:10:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:16.96 +55:43:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:21.87 +54:04:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:42.34 +53:53:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:45.37 +54:02:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:46.42 +50:32:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:53.29 +55:45:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:04.31 +55:18:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:13.54 +56:18:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:13.73 +55:20:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:14.03 +52:18:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:22.88 +52:49:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:23.08 +50:30:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:27.35 +56:45:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:32.46 +54:30:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:34.54 +50:32:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:38.18 +52:09:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:48.44 +54:22:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:54.38 +52:08:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:55.94 +51:11:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:07.39 +50:23:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:09.83 +51:10:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:12.04 +54:13:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:14.99 +52:50:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:16.90 +50:04:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:28.82 +56:19:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:42.50 +52:19:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:43.98 +55:35:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:50.44 +54:56:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:59.42 +51:23:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:05.96 +54:46:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:06.52 +55:53:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:13.21 +51:20:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:25.62 +50:36:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:27.75 +57:32:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:30.79 +50:26:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:52.38 +55:44:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:56.18 +53:26:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:04.13 +54:30:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:16.30 +51:29:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:26.45 +50:09:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:28.30 +55:09:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:31.07 +54:37:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:39.47 +51:21:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:43.66 +50:45:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:52.25 +50:23:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:56.65 +56:26:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:01.96 +57:01:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:06.02 +51:03:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:09.64 +50:41:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:10.01 +50:55:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:11.37 +52:05:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:14.48 +50:25:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:16.32 +56:01:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:18.43 +54:09:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:26.80 +56:58:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:40.09 +56:54:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:10.80 +52:38:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:11.14 +57:04:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:28.46 +51:28:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:36.07 +51:31:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:43.83 +50:34:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:45.96 +51:11:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:48.32 +51:17:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:03.08 +50:31:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:12.45 +51:49:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:12.92 +55:26:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:20.54 +54:40:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:24.59 +51:36:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:46.84 +50:21:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:53.24 +53:47:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:40.88 +51:46:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:48.03 +51:06:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:50.24 +55:02:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:59.95 +54:41:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:01.24 +52:33:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:03.14 +51:28:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:07.04 +54:29:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:24.64 +53:39:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:33.85 +53:51:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:42.37 +53:38:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:43.39 +53:34:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:28.60 +51:58:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:35.35 +55:18:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:52.25 +51:14:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:54.73 +53:29:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:56.31 +50:48:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:57.22 +51:35:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:12.54 +51:12:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:26.65 +52:35:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:37.70 +51:40:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:40.46 +54:40:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:01.22 +55:19:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:18.59 +50:50:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:23.37 +50:21:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:24.96 +54:18:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:27.28 +54:31:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:28.49 +54:37:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:40.78 +51:00:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:00.08 +52:44:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:19.77 +51:19:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:39.65 +50:07:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:45.03 +50:07:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:45.19 +49:57:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:22.59 +53:58:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:36.95 +50:34:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:55.40 +52:57:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:17.93 +50:14:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:21.12 +50:23:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:27.48 +51:58:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:43.32 +50:42:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:33.67 +50:47:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:27.72 +54:14:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:18.62 +50:33:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:19.18 +54:21:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:25.64 +52:52:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:37.11 +53:51:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:55.59 +53:55:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:22.44 +53:30:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:59.45 +50:05:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:00.82 +50:12:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:20.86 +51:29:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:30.23 +54:01:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:34.26 +51:57:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:18.97 +53:33:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:31.73 +51:24:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:59.18 +52:04:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:48.43 +50:59:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:03.64 +52:12:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:13.66 +51:50:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:27.86 +52:16:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:37.65 +53:26:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:42.03 +52:17:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:22.19 +50:46:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:31.46 +54:09:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:42.82 +53:21:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:59.89 +53:02:02.6 -- 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)
00:00:01.36 +53:01:37.5 -- not a known variable star
00:00:07.97 +51:20:34.4 -- not a known variable star
00:00:42.73 +51:44:33.3 -- a known variable star
00:00:44.99 +52:08:03.4 -- not a known variable star
00:01:38.26 +50:38:25.8 -- not a known variable star
00:02:47.38 +51:31:20.4 -- not a known variable star
00:03:29.46 +53:34:39.7 -- not a known variable star
00:03:29.54 +51:28:01.8 -- not a known variable star
00:03:44.44 +50:01:24.4 -- not a known variable star
00:04:10.84 +53:29:33.7 -- a known variable star
00:04:32.67 +51:18:17.9 -- not a known variable star
00:04:39.10 +50:18:00.2 -- not a known variable star
00:05:13.07 +51:50:35.0 -- not a known variable star
00:05:32.75 +50:54:18.9 -- not a known variable star
00:05:44.31 +50:40:09.1 -- not a known variable star
00:06:07.57 +50:16:46.8 -- not a known variable star
00:06:29.74 +51:42:56.0 -- not a known variable star
00:06:32.90 +54:39:32.0 -- not a known variable star
00:07:09.76 +50:30:14.6 -- not a known variable star
00:07:16.31 +51:00:11.3 -- not a known variable star
00:07:27.60 +51:29:05.2 -- not a known variable star
00:07:28.60 +51:49:30.6 -- not a known variable star
00:07:29.15 +51:05:33.0 -- not a known variable star
00:07:34.46 +51:47:00.5 -- not a known variable star
00:07:46.77 +54:40:41.9 -- not a known variable star
00:08:00.03 +50:31:24.7 -- not a known variable star
00:08:05.50 +51:46:22.3 -- not a known variable star
00:08:10.60 +52:36:10.1 -- not a known variable star
00:08:29.28 +51:35:14.5 -- not a known variable star
00:08:31.57 +52:43:57.6 -- not a known variable star
00:08:58.01 +52:27:28.7 -- not a known variable star
00:08:59.67 +50:29:49.5 -- not a known variable star
00:09:18.60 +53:05:18.0 -- not a known variable star
00:09:23.43 +51:02:03.8 -- not a known variable star
00:09:56.28 +51:29:47.0 -- not a known variable star
00:09:56.98 +50:50:46.1 -- not a known variable star
00:10:19.20 +51:21:32.1 -- not a known variable star
00:10:19.86 +50:21:11.1 -- not a known variable star
00:10:41.39 +53:58:59.5 -- not a known variable star
00:10:51.20 +52:25:07.5 -- not a known variable star
00:11:25.51 +51:27:46.6 -- not a known variable star
00:11:38.66 +54:02:13.9 -- not a known variable star
00:12:07.85 +52:25:18.0 -- not a known variable star
00:12:14.63 +53:43:20.0 -- not a known variable star
00:12:29.83 +53:38:35.5 -- not a known variable star
00:12:38.00 +53:52:11.1 -- not a known variable star
00:12:57.02 +51:31:46.9 -- not a known variable star
00:13:10.45 +50:30:07.3 -- not a known variable star
00:13:12.27 +50:29:47.9 -- not a known variable star
00:13:23.95 +51:50:59.6 -- not a known variable star
00:13:26.58 +53:19:41.1 -- not a known variable star
00:13:29.41 +53:19:49.2 -- not a known variable star
00:14:23.52 +53:09:22.5 -- not a known variable star
00:16:18.85 +56:42:06.0 -- a known variable star
00:16:21.72 +53:48:42.7 -- not a known variable star
00:16:59.35 +52:47:31.5 -- not a known variable star
00:17:09.91 +50:18:49.9 -- not a known variable star
00:18:53.29 +52:28:12.8 -- not a known variable star
00:19:20.06 +55:37:10.4 -- not a known variable star
00:19:20.29 +50:14:26.1 -- not a known variable star
00:19:26.40 +49:42:31.1 -- not a known variable star
00:19:57.98 +56:35:35.9 -- a known variable star
00:20:06.47 +55:24:13.8 -- not a known variable star
00:20:28.23 +54:57:49.1 -- not a known variable star
00:20:40.54 +52:18:07.6 -- not a known variable star
00:22:11.58 +52:16:55.0 -- not a known variable star
00:22:29.93 +51:55:46.7 -- not a known variable star
00:23:24.29 +54:04:50.0 -- not a known variable star
00:24:08.31 +50:22:15.3 -- not a known variable star
00:24:08.76 +50:06:52.4 -- not a known variable star
00:24:27.13 +54:50:40.5 -- not a known variable star
00:24:43.89 +53:17:18.5 -- not a known variable star
00:24:44.88 +53:56:10.0 -- not a known variable star
00:25:07.42 +56:25:13.5 -- not a known variable star
00:25:26.11 +53:44:41.0 -- not a known variable star
00:25:49.42 +50:28:02.5 -- not a known variable star
00:26:02.62 +52:49:56.8 -- not a known variable star
00:26:38.74 +56:33:57.6 -- not a known variable star
23:09:04.86 +57:24:42.0 -- not a known variable star
23:09:15.63 +57:16:03.9 -- not a known variable star
23:09:50.10 +57:19:55.1 -- not a known variable star
23:10:20.45 +56:50:57.4 -- not a known variable star
23:10:28.92 +57:11:08.3 -- not a known variable star
23:10:29.21 +57:13:04.4 -- not a known variable star
23:10:36.58 +56:49:29.7 -- not a known variable star
23:11:03.57 +57:24:20.6 -- a known variable star
23:11:05.31 +56:36:32.0 -- not a known variable star
23:11:16.06 +56:36:21.6 -- not a known variable star
23:11:20.95 +56:24:15.5 -- not a known variable star
23:11:28.21 +56:37:54.0 -- not a known variable star
23:11:29.53 +55:33:26.0 -- not a known variable star
23:11:38.67 +56:35:48.7 -- not a known variable star
23:12:00.73 +56:27:20.8 -- not a known variable star
23:12:08.53 +57:31:17.6 -- not a known variable star
23:12:49.41 +54:42:07.9 -- not a known variable star
23:12:55.82 +55:28:00.1 -- a known variable star
23:12:59.24 +56:18:47.6 -- not a known variable star
23:13:07.51 +56:44:48.1 -- not a known variable star
23:13:11.90 +55:44:22.2 -- not a known variable star
23:13:43.46 +55:17:10.3 -- not a known variable star
23:13:46.60 +54:38:25.2 -- not a known variable star
23:13:46.75 +55:05:40.2 -- not a known variable star
23:14:16.98 +56:27:23.4 -- not a known variable star
23:14:18.44 +57:19:41.7 -- not a known variable star
23:14:26.97 +57:33:59.7 -- not a known variable star
23:14:33.20 +57:06:08.3 -- not a known variable star
23:14:42.54 +55:59:12.5 -- not a known variable star
23:14:58.79 +55:26:18.0 -- not a known variable star
23:15:04.32 +55:33:55.7 -- not a known variable star
23:15:06.10 +56:02:21.3 -- not a known variable star
23:15:11.52 +57:21:43.1 -- not a known variable star
23:15:30.94 +55:29:10.7 -- a known variable star
23:15:34.34 +55:01:27.8 -- not a known variable star
23:15:39.64 +52:17:05.5 -- not a known variable star
23:15:46.07 +57:41:56.2 -- not a known variable star
23:15:46.19 +55:44:39.1 -- not a known variable star
23:15:48.11 +56:59:18.1 -- not a known variable star
23:15:56.98 +56:35:14.2 -- not a known variable star
23:16:05.69 +53:59:27.5 -- not a known variable star
23:16:08.34 +55:39:57.0 -- not a known variable star
23:16:13.35 +55:12:31.4 -- not a known variable star
23:16:30.14 +57:22:30.2 -- not a known variable star
23:16:32.51 +55:23:17.9 -- not a known variable star
23:16:41.88 +57:37:13.2 -- not a known variable star
23:17:13.51 +56:09:04.4 -- not a known variable star
23:17:16.38 +51:02:57.6 -- not a known variable star
23:17:18.12 +56:04:16.7 -- not a known variable star
23:17:19.53 +55:48:30.3 -- not a known variable star
23:17:29.14 +51:35:32.9 -- a known variable star
23:17:31.57 +57:13:09.0 -- not a known variable star
23:17:32.53 +56:09:21.0 -- not a known variable star
23:17:39.13 +56:25:45.6 -- not a known variable star
23:17:49.47 +51:39:33.9 -- not a known variable star
23:17:51.12 +53:37:04.6 -- not a known variable star
23:17:53.16 +53:31:56.3 -- not a known variable star
23:17:55.99 +56:24:54.8 -- not a known variable star
23:18:03.58 +55:43:10.1 -- not a known variable star
23:18:04.96 +55:30:11.1 -- not a known variable star
23:18:06.71 +50:59:08.4 -- not a known variable star
23:18:11.41 +54:19:57.5 -- not a known variable star
23:18:17.24 +54:09:17.2 -- not a known variable star
23:18:17.92 +53:44:14.7 -- not a known variable star
23:18:19.31 +56:04:31.1 -- not a known variable star
23:18:24.24 +53:43:23.0 -- not a known variable star
23:18:26.78 +53:20:30.8 -- not a known variable star
23:18:28.53 +51:19:29.9 -- not a known variable star
23:18:39.75 +50:05:36.4 -- not a known variable star
23:18:48.13 +50:21:35.5 -- not a known variable star
23:18:52.90 +51:20:13.1 -- not a known variable star
23:18:52.99 +54:59:05.7 -- a known variable star
23:18:53.90 +53:45:26.0 -- not a known variable star
23:18:53.97 +54:28:24.4 -- not a known variable star
23:18:58.56 +54:09:25.0 -- not a known variable star
23:19:01.25 +51:51:44.9 -- not a known variable star
23:19:01.95 +55:54:17.3 -- not a known variable star
23:19:02.25 +55:54:02.7 -- not a known variable star
23:19:02.46 +54:30:07.8 -- not a known variable star
23:19:05.21 +50:33:42.9 -- not a known variable star
23:19:13.36 +52:17:54.8 -- not a known variable star
23:19:17.20 +52:12:32.3 -- not a known variable star
23:19:18.81 +51:15:50.4 -- not a known variable star
23:19:24.23 +54:26:59.2 -- not a known variable star
23:19:26.47 +50:59:21.6 -- not a known variable star
23:19:27.23 +51:48:29.4 -- not a known variable star
23:19:30.68 +55:40:18.3 -- not a known variable star
23:19:34.37 +50:14:46.9 -- not a known variable star
23:19:38.04 +50:35:21.3 -- a known variable star
23:19:52.02 +49:24:30.4 -- not a known variable star
23:19:52.88 +49:51:22.2 -- a known variable star
23:20:02.13 +49:55:45.5 -- not a known variable star
23:20:05.34 +55:44:17.8 -- not a known variable star
23:20:09.39 +49:57:06.1 -- not a known variable star
23:20:22.98 +50:39:45.9 -- a known variable star
23:20:29.03 +54:17:15.4 -- not a known variable star
23:20:38.47 +54:42:03.0 -- not a known variable star
23:20:39.70 +55:02:04.7 -- not a known variable star
23:20:39.97 +55:09:31.8 -- not a known variable star
23:20:41.10 +49:38:25.8 -- not a known variable star
23:20:42.25 +52:15:34.7 -- not a known variable star
23:20:47.45 +49:41:56.4 -- not a known variable star
23:20:52.75 +50:30:13.3 -- not a known variable star
23:20:55.73 +54:36:44.9 -- not a known variable star
23:20:56.42 +53:10:52.9 -- not a known variable star
23:21:03.75 +49:30:36.1 -- not a known variable star
23:21:10.38 +55:54:00.5 -- a known variable star
23:21:26.05 +51:16:44.1 -- not a known variable star
23:21:29.67 +54:16:21.5 -- a known variable star
23:21:29.75 +53:08:48.8 -- not a known variable star
23:21:31.13 +51:34:43.0 -- not a known variable star
23:21:35.56 +56:30:06.9 -- not a known variable star
23:21:36.05 +52:40:17.3 -- not a known variable star
23:21:42.49 +50:06:38.8 -- not a known variable star
23:22:01.22 +53:10:19.2 -- not a known variable star
23:22:04.92 +50:07:50.1 -- not a known variable star
23:22:06.03 +53:17:47.4 -- not a known variable star
23:22:07.42 +49:54:19.3 -- not a known variable star
23:22:16.77 +52:07:23.0 -- not a known variable star
23:22:19.10 +54:46:28.8 -- not a known variable star
23:22:28.19 +54:17:33.2 -- not a known variable star
23:22:30.34 +55:44:27.1 -- not a known variable star
23:22:36.33 +49:57:50.0 -- not a known variable star
23:22:41.71 +50:08:48.8 -- not a known variable star
23:22:43.60 +51:19:45.4 -- not a known variable star
23:22:50.20 +51:55:38.5 -- not a known variable star
23:22:55.30 +54:14:50.9 -- not a known variable star
23:22:55.83 +53:23:01.2 -- not a known variable star
23:23:02.09 +51:27:45.7 -- not a known variable star
23:23:04.40 +52:25:37.5 -- a known variable star
23:23:07.34 +49:28:50.7 -- not a known variable star
23:23:09.84 +53:47:00.6 -- not a known variable star
23:23:12.46 +54:50:18.9 -- not a known variable star
23:23:12.70 +56:57:56.7 -- not a known variable star
23:23:13.80 +51:43:35.2 -- not a known variable star
23:23:17.36 +55:37:43.3 -- not a known variable star
23:23:22.45 +51:40:47.7 -- not a known variable star
23:23:31.78 +55:24:15.3 -- not a known variable star
23:23:34.50 +52:08:32.1 -- not a known variable star
23:23:36.32 +52:43:39.9 -- not a known variable star
23:23:37.36 +52:10:37.1 -- not a known variable star
23:23:47.22 +52:32:55.6 -- a known variable star
23:23:47.98 +53:18:18.4 -- not a known variable star
23:24:02.23 +55:45:42.7 -- not a known variable star
23:24:06.72 +51:31:34.1 -- not a known variable star
23:24:13.25 +57:04:21.3 -- not a known variable star
23:24:18.43 +51:34:22.7 -- not a known variable star
23:24:25.61 +53:57:00.3 -- not a known variable star
23:24:33.15 +53:38:51.1 -- not a known variable star
23:24:52.09 +54:41:49.4 -- not a known variable star
23:24:52.23 +53:53:18.9 -- not a known variable star
23:24:52.56 +55:09:33.4 -- not a known variable star
23:24:54.00 +51:36:31.5 -- not a known variable star
23:25:03.71 +57:01:59.5 -- a known variable star
23:25:12.62 +54:01:38.1 -- not a known variable star
23:25:13.81 +51:29:54.3 -- not a known variable star
23:25:14.02 +55:36:09.2 -- a known variable star
23:25:35.82 +57:55:06.6 -- not a known variable star
23:25:37.16 +51:45:06.5 -- not a known variable star
23:25:40.16 +54:34:40.4 -- not a known variable star
23:25:50.46 +54:19:34.7 -- not a known variable star
23:26:02.05 +54:34:25.4 -- not a known variable star
23:26:02.96 +53:45:44.1 -- not a known variable star
23:26:05.54 +54:30:20.9 -- not a known variable star
23:26:17.36 +55:31:52.1 -- not a known variable star
23:26:19.28 +53:47:48.6 -- not a known variable star
23:26:30.09 +51:45:22.5 -- not a known variable star
23:26:38.84 +55:07:00.1 -- not a known variable star
23:26:47.97 +57:24:35.9 -- a known variable star
23:27:04.72 +55:04:53.5 -- not a known variable star
23:27:25.43 +56:44:45.4 -- not a known variable star
23:27:27.22 +52:12:45.3 -- a known variable star
23:27:34.88 +57:18:22.3 -- not a known variable star
23:27:41.36 +54:21:24.4 -- not a known variable star
23:27:52.16 +57:08:13.7 -- not a known variable star
23:27:53.79 +50:38:36.4 -- not a known variable star
23:28:01.21 +55:38:38.0 -- not a known variable star
23:28:08.91 +50:26:16.2 -- not a known variable star
23:28:15.89 +50:18:04.2 -- not a known variable star
23:28:24.32 +51:59:26.8 -- not a known variable star
23:28:37.29 +56:49:15.5 -- not a known variable star
23:28:38.20 +51:01:20.5 -- not a known variable star
23:28:43.61 +56:40:16.9 -- not a known variable star
23:28:53.48 +49:44:55.5 -- not a known variable star
23:29:01.56 +50:30:26.5 -- not a known variable star
23:29:02.05 +50:39:49.2 -- not a known variable star
23:29:05.04 +55:58:56.1 -- not a known variable star
23:29:27.14 +50:48:42.5 -- not a known variable star
23:29:29.10 +51:00:39.4 -- not a known variable star
23:29:56.83 +51:09:25.5 -- not a known variable star
23:29:57.38 +55:09:17.0 -- not a known variable star
23:30:06.64 +55:31:12.4 -- not a known variable star
23:30:10.24 +49:54:50.3 -- a known variable star
23:30:11.92 +56:22:07.2 -- not a known variable star
23:30:13.36 +55:17:29.0 -- not a known variable star
23:30:21.39 +50:22:09.6 -- not a known variable star
23:30:29.85 +54:34:21.0 -- not a known variable star
23:30:32.15 +54:54:01.6 -- not a known variable star
23:30:33.53 +51:17:36.4 -- not a known variable star
23:30:35.12 +53:14:45.6 -- not a known variable star
23:30:36.18 +54:38:27.4 -- not a known variable star
23:30:36.43 +50:51:22.0 -- a known variable star
23:30:38.22 +55:00:24.1 -- not a known variable star
23:30:40.30 +54:19:13.7 -- not a known variable star
23:30:41.60 +51:38:08.5 -- not a known variable star
23:30:43.51 +55:32:50.3 -- not a known variable star
23:30:52.31 +54:23:23.5 -- not a known variable star
23:31:12.32 +50:01:53.6 -- not a known variable star
23:31:14.34 +51:34:01.0 -- not a known variable star
23:31:16.51 +51:15:13.0 -- not a known variable star
23:31:17.80 +54:01:18.7 -- not a known variable star
23:31:20.91 +52:54:38.0 -- not a known variable star
23:31:25.50 +52:51:49.0 -- not a known variable star
23:31:39.33 +56:24:27.2 -- not a known variable star
23:31:42.78 +55:31:56.5 -- a known variable star
23:31:48.80 +49:59:03.6 -- not a known variable star
23:31:49.97 +56:40:30.7 -- not a known variable star
23:31:54.45 +55:25:34.1 -- not a known variable star
23:32:12.56 +57:11:42.1 -- not a known variable star
23:32:19.47 +55:17:56.4 -- not a known variable star
23:32:25.39 +57:31:51.7 -- not a known variable star
23:32:44.57 +53:36:12.5 -- not a known variable star
23:32:51.32 +54:47:13.9 -- not a known variable star
23:32:52.30 +53:44:57.6 -- not a known variable star
23:32:54.99 +53:38:40.9 -- not a known variable star
23:33:09.14 +52:28:51.3 -- not a known variable star
23:33:12.21 +50:10:29.9 -- not a known variable star
23:33:16.96 +55:43:28.3 -- not a known variable star
23:33:21.87 +54:04:28.5 -- not a known variable star
23:33:42.34 +53:53:39.6 -- not a known variable star
23:33:45.37 +54:02:56.4 -- not a known variable star
23:33:46.42 +50:32:46.8 -- not a known variable star
23:33:53.29 +55:45:09.2 -- not a known variable star
23:34:04.31 +55:18:58.3 -- not a known variable star
23:34:13.54 +56:18:02.1 -- not a known variable star
23:34:13.73 +55:20:19.5 -- not a known variable star
23:34:14.03 +52:18:18.2 -- not a known variable star
23:34:22.88 +52:49:51.6 -- not a known variable star
23:34:23.08 +50:30:41.4 -- not a known variable star
23:34:27.35 +56:45:26.0 -- not a known variable star
23:34:32.46 +54:30:26.4 -- not a known variable star
23:34:34.54 +50:32:21.8 -- not a known variable star
23:34:38.18 +52:09:25.3 -- not a known variable star
23:34:48.44 +54:22:16.9 -- not a known variable star
23:34:54.38 +52:08:13.6 -- not a known variable star
23:34:55.94 +51:11:11.8 -- not a known variable star
23:35:07.39 +50:23:49.7 -- not a known variable star
23:35:09.83 +51:10:28.4 -- not a known variable star
23:35:12.04 +54:13:18.5 -- not a known variable star
23:35:14.99 +52:50:25.3 -- not a known variable star
23:35:16.90 +50:04:40.1 -- not a known variable star
23:35:28.82 +56:19:45.8 -- not a known variable star
23:35:42.50 +52:19:08.8 -- not a known variable star
23:35:43.98 +55:35:51.8 -- not a known variable star
23:35:50.44 +54:56:06.3 -- not a known variable star
23:35:59.42 +51:23:05.6 -- not a known variable star
23:36:05.96 +54:46:13.3 -- not a known variable star
23:36:06.52 +55:53:51.7 -- not a known variable star
23:36:13.21 +51:20:23.4 -- not a known variable star
23:36:25.62 +50:36:51.0 -- not a known variable star
23:36:27.75 +57:32:22.4 -- not a known variable star
23:36:30.79 +50:26:34.8 -- not a known variable star
23:36:52.38 +55:44:54.7 -- not a known variable star
23:36:56.18 +53:26:38.5 -- a known variable star
23:37:04.13 +54:30:54.1 -- not a known variable star
23:37:16.30 +51:29:54.6 -- a known variable star
23:37:26.45 +50:09:49.4 -- not a known variable star
23:37:28.30 +55:09:05.4 -- not a known variable star
23:37:31.07 +54:37:57.2 -- not a known variable star
23:37:39.47 +51:21:05.3 -- not a known variable star
23:37:43.66 +50:45:05.0 -- a known variable star
23:37:52.25 +50:23:10.1 -- not a known variable star
23:37:56.65 +56:26:03.7 -- not a known variable star
23:38:01.96 +57:01:56.2 -- a known variable star
23:38:06.02 +51:03:58.2 -- not a known variable star
23:38:09.64 +50:41:37.0 -- not a known variable star
23:38:10.01 +50:55:36.5 -- not a known variable star
23:38:11.37 +52:05:02.3 -- not a known variable star
23:38:14.48 +50:25:54.0 -- not a known variable star
23:38:16.32 +56:01:28.1 -- not a known variable star
23:38:18.43 +54:09:41.6 -- not a known variable star
23:38:26.80 +56:58:36.3 -- not a known variable star
23:38:40.09 +56:54:44.7 -- not a known variable star
23:39:10.80 +52:38:27.8 -- not a known variable star
23:39:11.14 +57:04:18.8 -- not a known variable star
23:39:28.46 +51:28:27.3 -- not a known variable star
23:39:36.07 +51:31:08.8 -- not a known variable star
23:39:43.83 +50:34:48.1 -- not a known variable star
23:39:45.96 +51:11:03.9 -- not a known variable star
23:39:48.32 +51:17:42.2 -- not a known variable star
23:40:03.08 +50:31:06.4 -- not a known variable star
23:40:12.45 +51:49:27.7 -- not a known variable star
23:40:12.92 +55:26:29.3 -- not a known variable star
23:40:20.54 +54:40:25.9 -- not a known variable star
23:40:24.59 +51:36:30.4 -- not a known variable star
23:40:46.84 +50:21:18.3 -- not a known variable star
23:40:53.24 +53:47:05.7 -- not a known variable star
23:41:40.88 +51:46:14.0 -- not a known variable star
23:41:48.03 +51:06:34.3 -- not a known variable star
23:41:50.24 +55:02:54.1 -- not a known variable star
23:41:59.95 +54:41:41.0 -- not a known variable star
23:42:01.24 +52:33:44.2 -- not a known variable star
23:42:03.14 +51:28:48.3 -- not a known variable star
23:42:07.04 +54:29:32.0 -- not a known variable star
23:42:24.64 +53:39:51.6 -- not a known variable star
23:42:33.85 +53:51:34.2 -- not a known variable star
23:42:42.37 +53:38:55.8 -- not a known variable star
23:42:43.39 +53:34:06.0 -- not a known variable star
23:43:28.60 +51:58:13.4 -- not a known variable star
23:43:35.35 +55:18:49.6 -- not a known variable star
23:43:52.25 +51:14:12.9 -- not a known variable star
23:43:54.73 +53:29:50.5 -- not a known variable star
23:43:56.31 +50:48:29.6 -- not a known variable star
23:43:57.22 +51:35:21.9 -- not a known variable star
23:44:12.54 +51:12:02.8 -- not a known variable star
23:44:26.65 +52:35:34.9 -- not a known variable star
23:44:37.70 +51:40:35.6 -- not a known variable star
23:44:40.46 +54:40:58.5 -- not a known variable star
23:45:01.22 +55:19:04.4 -- not a known variable star
23:45:18.59 +50:50:13.5 -- not a known variable star
23:45:23.37 +50:21:07.2 -- not a known variable star
23:45:24.96 +54:18:51.5 -- not a known variable star
23:45:27.28 +54:31:03.7 -- not a known variable star
23:45:28.49 +54:37:56.6 -- not a known variable star
23:45:40.78 +51:00:36.0 -- not a known variable star
23:46:00.08 +52:44:54.5 -- not a known variable star
23:46:19.77 +51:19:58.5 -- not a known variable star
23:46:39.65 +50:07:15.9 -- not a known variable star
23:46:45.03 +50:07:53.8 -- not a known variable star
23:47:45.19 +49:57:10.9 -- not a known variable star
23:48:22.59 +53:58:07.2 -- a known variable star
23:48:36.95 +50:34:52.5 -- not a known variable star
23:48:55.40 +52:57:31.1 -- not a known variable star
23:49:17.93 +50:14:11.3 -- a known variable star
23:49:21.12 +50:23:22.7 -- not a known variable star
23:49:27.48 +51:58:31.5 -- not a known variable star
23:49:43.32 +50:42:41.7 -- not a known variable star
23:50:33.67 +50:47:47.1 -- not a known variable star
23:51:27.72 +54:14:05.2 -- not a known variable star
23:52:18.62 +50:33:10.0 -- not a known variable star
23:52:19.18 +54:21:38.8 -- not a known variable star
23:52:25.64 +52:52:42.7 -- not a known variable star
23:52:37.11 +53:51:53.0 -- not a known variable star
23:52:55.59 +53:55:19.6 -- not a known variable star
23:53:22.44 +53:30:17.8 -- not a known variable star
23:53:59.45 +50:05:18.9 -- not a known variable star
23:54:00.82 +50:12:59.3 -- not a known variable star
23:54:20.86 +51:29:40.6 -- not a known variable star
23:54:30.23 +54:01:29.4 -- not a known variable star
23:54:34.26 +51:57:43.2 -- not a known variable star
23:55:18.97 +53:33:58.1 -- a known variable star
23:55:31.73 +51:24:35.3 -- not a known variable star
23:55:59.18 +52:04:34.3 -- not a known variable star
23:56:48.43 +50:59:50.3 -- not a known variable star
23:57:03.64 +52:12:14.7 -- not a known variable star
23:57:13.66 +51:50:40.9 -- not a known variable star
23:58:27.86 +52:16:14.1 -- not a known variable star
23:58:37.65 +53:26:04.7 -- not a known variable star
23:58:42.03 +52:17:51.8 -- not a known variable star
23:59:22.19 +50:46:57.6 -- not a known variable star
23:59:31.46 +54:09:40.4 -- not a known variable star
23:59:42.82 +53:21:57.0 -- not a known variable star
23:59:59.89 +53:02:02.6 -- not a known variable star
Found 411 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
441 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 441 (excluding asteroids and hot pixels, 411 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461280.70551288 -observatory V36
10:30:05.72 +11:16:29.9 Mercury (-1.9mag)
13:08:11.24 -10:23:38.1 Venus (-4.6mag)
06:46:17.31 +23:29:15.6 Mars (1.3mag)
09:00:33.65 +17:32:44.2 Jupiter (-1.8mag)
00:53:49.89 +02:53:55.3 Saturn (0.5mag)
04:13:22.79 +21:01:11.8 Uranus (5.7mag)
00:14:39.32 +00:02:57.8 Neptune (7.7mag)
20:26:21.17 -23:36:59.4 Pluto (14.5mag)
22:27:44.07 -09:52:29.8 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 363 Aug 28 00:10 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461280.70551288:
09:00:28.75 +17:33:08.3 Io (6.1mag)
09:00:24.96 +17:33:26.4 Europa (6.3mag)
09:00:35.88 +17:32:36.8 Ganymede (5.7mag)
09:01:01.92 +17:30:32.8 Callisto (6.9mag)
08:58:05.35 +17:44:08.2 Himalia (15.7mag)
09:00:38.04 +17:32:24.9 Thebe (16.6mag)
08:57:45.47 +17:39:05.9 Elara (17.7mag)
09:04:38.02 +17:03:43.1 Pasiphae (17.9mag)
09:02:22.09 +17:47:48.8 Carme (19.0mag)
00:53:41.80 +02:53:29.6 Titan (8.4mag)
00:53:46.64 +02:54:01.9 Rhea (9.7mag)
00:54:23.99 +02:56:23.2 Iapetus (11.1mag)
00:53:34.55 +02:54:01.3 Hyperion (14.4mag)
00:52:47.78 +02:44:41.0 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 28 00:10 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461280.70551288:
20:50:10.97 -09:04:14.9 JWST
18:34:48.43 +20:27:48.4 Chandra
09:44:17.80 -54:38:08.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 28 00:10 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461280.70551288 -observatory V36
03:33:18.19 +18:48:27.0 17.5mag P/1996 R2 (Lagerkvist)
18:00:24.17 -34:23:14.0 14.2mag P/2010 H2 (Vales)
07:11:27.22 -69:46:16.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:14:14.28 +33:26:49.0 17.7mag C/2017 K2 (PANSTARRS)
04:33:48.54 +43:43:26.8 17.7mag P/2021 N1 (ZTF)
22:21:47.00 +29:48:28.2 17.4mag C/2022 E2 (ATLAS)
07:02:01.80 +26:10:17.2 16.8mag C/2022 N2 (PANSTARRS)
10:40:08.94 +27:36:41.9 17.0mag C/2022 QE78 (ATLAS)
09:42:09.23 +05:16:51.8 18.0mag C/2022 R6 (PANSTARRS)
20:47:25.22 +63:03:17.3 18.0mag C/2023 H5 (Lemmon)
15:33:17.88 -14:45:25.9 14.7mag C/2023 R1 (PANSTARRS)
08:29:03.93 +32:18:53.2 15.6mag C/2024 E1 (Wierzchos)
15:05:46.00 +15:26:27.4 17.8mag C/2024 G6 (ATLAS)
18:41:17.49 +43:26:59.1 13.7mag C/2024 J3 (ATLAS)
20:40:37.96 +49:39:20.5 17.5mag C/2024 R4 (PANSTARRS)
05:29:39.90 -12:55:26.8 15.2mag C/2024 T5 (ATLAS)
07:07:30.82 +20:30:34.1 17.9mag C/2025 J1 (Borisov)
11:02:07.31 +19:32:05.5 17.0mag C/2025 V2 (Rankin)
13:11:40.56 +00:54:42.5 16.9mag C/2025 Y1 (ATLAS)
16:19:17.09 +75:32:05.1 16.3mag C/2026 A2 (Bok)
03:09:15.35 +46:19:44.8 17.3mag C/2026 B2 (Sun-Gao)
12:04:03.52 +10:26:26.6 17.5mag A/2026 E1
22:17:33.71 -33:41:26.2 7.3mag 10P/Tempel
11:41:29.93 -04:43:47.7 16.3mag 29P/Schwassmann-Wachmann
11:48:13.66 -01:52:08.8 17.5mag 63P/Wild
00:49:31.65 -06:26:19.3 15.4mag 65P/Gunn
06:19:05.18 +19:55:57.6 13.7mag 78P/Gehrels
20:21:44.04 -25:28:55.7 17.3mag 84P/Giclas
03:14:54.05 +14:45:56.2 17.0mag 88P/Howell
08:43:51.76 +24:38:57.6 16.5mag 93P/Lovas
05:05:37.44 +24:42:47.1 17.1mag 112P/Urata-Niijima
07:01:01.77 +27:09:37.2 16.0mag 114P/Wiseman-Skiff
10:05:05.42 +22:56:51.5 14.9mag 123P/West-Hartley
12:24:48.35 -17:44:50.6 17.3mag 124P/Mrkos
06:04:37.25 +20:54:38.0 16.0mag 128P/Shoemaker-Holt
07:01:06.74 +17:42:19.9 17.9mag 131P/Mueller
23:57:15.55 +02:52:23.7 17.4mag 139P/Vaisala-Oterma
03:00:17.73 -18:22:14.5 12.4mag 161P/Hartley-IRAS
08:22:11.70 +38:01:42.5 16.2mag 162P/Siding Spring
10:15:21.49 +22:26:47.6 12.5mag 169P/NEAT
03:13:56.05 +09:08:54.1 17.6mag 220P/McNaught
04:20:01.45 +32:57:22.7 15.3mag 260P/McNaught
08:04:02.26 +36:39:10.4 17.3mag 295P/LINEAR
15:19:12.43 +00:53:29.6 17.8mag 391P/Kowalski
09:18:56.29 +17:22:06.4 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.2K Aug 28 00:10 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
-rw-r--r-- 1 apache apache 190K Aug 28 00:10 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:00:02.823 +12:57:02.46 AT 2026xsp 2026-02-13.59 21.18
13:18:25.859 +25:17:53.19 AT 2026xso 2026-02-17.52 21.43
14:46:41.619 +11:38:04.02 AT 2026xsn 2026-02-17.55 20.37
14:12:17.965 +35:36:02.21 AT 2026xsm 2026-02-17.60 20.93
00:28:22.210 -09:16:55.88 AT 2026xsl 2026-08-06.67 20.38
13:40:02.666 +27:45:49.66 AT 2026xsk 2026-02-17.50 21.05
13:18:58.760 +35:13:29.33 AT 2026xsj 2026-02-17.49 21.16
14:58:55.200 +08:49:53.06 AT 2026xsi 2026-02-13.58 21.13
12:22:18.795 +12:08:10.55 AT 2026xsh 2026-02-16.62 20.67
11:46:22.552 +13:15:39.41 AT 2026xsg 2026-02-16.57 20.7
08:55:07.272 +15:47:59.14 AT 2026xsf 2026-02-13.30 20.98
07:34:01.728 +10:29:15.79 AT 2026xse 2026-02-14.26 20.11
07:29:49.030 +19:09:23.06 AT 2026xsd 2026-02-13.26 20.62
07:42:52.595 +22:58:08.19 AT 2026xsc 2026-02-13.26 20.93
04:42:06.854 +06:56:13.00 AT 2026xsb 2026-02-06.24 21.16
05:10:23.116 -06:04:42.26 AT 2026xsa 2026-02-05.30 20.59
05:17:11.087 -07:32:29.20 AT 2026xrz 2026-02-02.30 20.34
08:18:15.789 -07:48:37.88 AT 2026xry 2026-01-28.38 20.53
10:52:02.742 +09:20:43.23 AT 2026xrx 2026-01-28.44 21.19
10:51:22.547 +09:35:56.77 AT 2026xrw 2026-01-28.44 20.5
-rw-r--r-- 1 apache apache 88K Aug 28 00:10 tns_transients_list.txt
