This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg
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 09 09.2599 2461292.7599 12.21 23:43:47.21 +58:01:11.0
114.05019 -3.68067 galactic Cas Second-epoch detections are separated by 0.9" 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 | 23:43:47.21 +58:01:11.0 (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 23:43:47.21 +58:01:11.0: 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 23:43:47.21 +58:01:11.0: 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 09 09.2599* 23 43 47.21 +58 01 11.0 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,2461292.7599,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 12.21 23:31:14.93 +54:16:11.9
111.30189 -6.78108 galactic Cas Second-epoch detections are separated by 8.7" 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 | 23:31:14.93 +54:16:11.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:14.93 +54:16:11.9: 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 23:31:14.93 +54:16:11.9: 14.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 31 14.93 +54 16 11.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 11.95 23:23:47.40 +54:32:06.3
110.35277 -6.18192 galactic Cas Second-epoch detections are separated by 6.4" 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 | 23:23:47.40 +54:32:06.3 (user input) | T | P | (position from user input) J-Ks=0.757+/-0.160 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:47.40 +54:32:06.3: 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 23:23:47.40 +54:32:06.3: 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 09 09.2599* 23 23 47.40 +54 32 06.3 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 11.89 23:39:43.59 +57:07:19.3
113.28395 -4.40033 galactic Cas Second-epoch detections are separated by 8.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J354.9153+57.1171 | 23:39:43.59 +57:07:19.3 (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 23:39:43.59 +57:07:19.3: 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 23:39:43.59 +57:07:19.3: 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 09 09.2599* 23 39 43.59 +57 07 19.3 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.9153+57.1171,2461292.7599,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.9153+57.1171 20260909.2599 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 11.97 00:26:43.55 +50:38:16.8
118.93006 -12.04163 galactic Cas Second-epoch detections are separated by 0.8" 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 | ATO J006.6731+50.6581 | 00:26:41.32 +50:38:51.4 (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 00:26:43.55 +50:38:16.8: 14.35 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:26:43.55 +50:38:16.8: 14.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.35 +/- 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 09 09.2599* 00 26 43.55 +50 38 16.8 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J006.6731+50.6581,2461292.7599,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J006.6731+50.6581 20260909.2599 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 11.53 23:23:26.83 +55:05:04.9
110.49081 -5.64745 galactic Cas Second-epoch detections are separated by 8.7" 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 | 23:23:26.83 +55:05:04.9 (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 23:23:26.83 +55:05:04.9: 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 23:23:26.83 +55:05:04.9: 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 09 09.2599* 23 23 26.83 +55 05 04.9 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,2461292.7599,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 11.87 23:48:15.65 +57:52:36.7
114.59006 -3.96802 galactic Cas Second-epoch detections are separated by 1.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J357.0701+57.8983 | 23:48:15.89 +57:53:15.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 1947AnDea...5....1L DO 43645
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:15.65 +57:52:36.7: 13.22 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:15.65 +57:52:36.7: 13.29 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 48 15.65 +57 52 36.7 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.0701+57.8983,2461292.7599,11.87,0.05,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 J357.0701+57.8983 20260909.2599 11.87CV 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 09 09.2599 2461292.7599 11.88 23:44:13.98 +57:45:24.9
114.03947 -3.94987 galactic Cas Second-epoch detections are separated by 4.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J356.0552+57.7556 | 23:44:13.98 +57:45:24.9 (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 23:44:13.98 +57:45:24.9: 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 23:44:13.98 +57:45:24.9: 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 09 09.2599* 23 44 13.98 +57 45 24.9 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.0552+57.7556,2461292.7599,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.0552+57.7556 20260909.2599 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 12.11 23:28:42.59 +57:11:03.1
111.87130 -3.90029 galactic Cas Second-epoch detections are separated by 1.1" 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 | 23:28:42.59 +57:11:03.1 (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 23:28:42.59 +57:11:03.1: 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 23:28:42.59 +57:11:03.1: 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 09 09.2599* 23 28 42.59 +57 11 03.1 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,12.11,0.05,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 20260909.2599 12.11CV 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 09 09.2599 2461292.7599 12.16 23:34:42.99 +57:22:12.9
112.70314 -3.96992 galactic Cas Second-epoch detections are separated by 0.7" 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 | 23:34:42.99 +57:22:12.9 (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 23:34:42.99 +57:22:12.9: 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 23:34:42.99 +57:22:12.9: 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 09 09.2599* 23 34 42.99 +57 22 12.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 12.29 23:39:42.20 +55:51:27.0
112.93171 -5.61520 galactic Cas Second-epoch detections are separated by 5.8" 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 | ATO J354.9101+55.8654 | 23:39:39.82 +55:51:52.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.305+/-0.259 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:42.20 +55:51:27.0: 13.61 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:42.20 +55:51:27.0: 14.01 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 09 09.2599* 23 39 42.20 +55 51 27.0 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.9101+55.8654,2461292.7599,12.29,0.05,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 J354.9101+55.8654 20260909.2599 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 09 09.2599 2461292.7599 12.27 23:13:58.82 +53:19:37.0
108.56471 -6.80437 galactic Cas Second-epoch detections are separated by 5.2" 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 | 23:13:58.82 +53:19:37.0 (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 23:13:58.82 +53:19:37.0: 13.75 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:13:58.82 +53:19:37.0: 14.30 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 13 58.82 +53 19 37.0 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,2461292.7599,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 14.30 23:16:39.91 +56:29:27.8
110.08287 -3.99789 galactic Cas Second-epoch detections are separated by 7.2" 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 | 23:16:39.91 +56:29:27.8 (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 23:16:39.91 +56:29:27.8: 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 23:16:39.91 +56:29:27.8: 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 09 09.2599* 23 16 39.91 +56 29 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,2461292.7599,14.30,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.35 23:16:01.56 +55:36:22.2
109.68001 -4.79140 galactic Cas Second-epoch detections are separated by 4.7" 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 | 23:16:01.56 +55:36:22.2 (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 23:16:01.56 +55:36:22.2: 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 23:16:01.56 +55:36:22.2: 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 09 09.2599* 23 16 01.56 +55 36 22.2 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,2461292.7599,14.35,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:15:47.76 +54:58:14.9
109.41862 -5.37189 galactic Cas Second-epoch detections are separated by 7.8" 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 | 23:15:47.76 +54:58:14.9 (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 23:15:47.76 +54:58:14.9: 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 23:15:47.76 +54:58:14.9: 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 09 09.2599* 23 15 47.76 +54 58 14.9 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,2461292.7599,14.38,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.29 23:25:15.17 +56:00:10.4
111.03846 -4.86584 galactic Cas Second-epoch detections are separated by 1.8" 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 | ATO J351.3137+56.0135 | 23:25:15.17 +56:00:10.4 (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 23:25:15.17 +56:00:10.4: 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 23:25:15.17 +56:00:10.4: 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 09 09.2599* 23 25 15.17 +56 00 10.4 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 J351.3137+56.0135,2461292.7599,14.29,0.05,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 J351.3137+56.0135 20260909.2599 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 09 09.2599 2461292.7599 14.47 23:32:31.21 +55:27:33.1
111.84153 -5.70407 galactic Cas Second-epoch detections are separated by 3.4" 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 | 23:32:31.21 +55:27:33.1 (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 23:32:31.21 +55:27:33.1: 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 23:32:31.21 +55:27:33.1: 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 09 09.2599* 23 32 31.21 +55 27 33.1 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
target,2461292.7599,14.47,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.34 23:45:44.54 +57:58:28.6
114.28963 -3.79056 galactic Cas Second-epoch detections are separated by 8.6" 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 | 23:45:44.54 +57:58:28.6 (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 23:45:44.54 +57:58:28.6: 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 23:45:44.54 +57:58:28.6: 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 09 09.2599* 23 45 44.54 +57 58 28.6 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,2461292.7599,14.34,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.36 23:17:28.43 +53:27:01.5
109.09862 -6.87871 galactic Cas Second-epoch detections are separated by 2.7" 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 | 23:17:28.43 +53:27:01.5 (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 23:17:28.43 +53:27:01.5: 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 23:17:28.43 +53:27:01.5: 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 09 09.2599* 23 17 28.43 +53 27 01.5 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,2461292.7599,14.36,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.39 23:27:32.52 +54:43:03.7
110.92899 -6.18707 galactic Cas Second-epoch detections are separated by 2.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:27:32.52 +54:43:03.7 (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 23:27:32.52 +54:43:03.7: 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 23:27:32.52 +54:43:03.7: 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 09 09.2599* 23 27 32.52 +54 43 03.7 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,2461292.7599,14.39,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:18:23.18 +52:39:51.7
108.94568 -7.66207 galactic And Second-epoch detections are separated by 1.3" 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 | ATO J349.5925+52.6543 | 23:18:23.18 +52:39:51.7 (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 23:18:23.18 +52:39:51.7: 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 23:18:23.18 +52:39:51.7: 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 09 09.2599* 23 18 23.18 +52 39 51.7 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
ATO J349.5925+52.6543,2461292.7599,14.38,0.05,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 J349.5925+52.6543 20260909.2599 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 09 09.2599 2461292.7599 14.40 23:15:38.74 +53:18:33.4
108.79122 -6.91203 galactic Cas Second-epoch detections are separated by 5.0" and 7.0 pix
The object was found in VSX15" Gaia DR3 1995357903546008192
Type: ROT
# Max. Min./Amp. JD0 Period
15.230 G 15.260 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 23:15:38.74 +53:18:33.4: 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 23:15:38.74 +53:18:33.4: 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 09 09.2599* 23 15 38.74 +53 18 33.4 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 1995357903546008192,2461292.7599,14.40,0.05,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 1995357903546008192 20260909.2599 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 09 09.2599 2461292.7599 14.35 23:17:34.14 +53:34:44.7
109.15820 -6.76358 galactic Cas Second-epoch detections are separated by 1.8" 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 | 23:17:34.14 +53:34:44.7 (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 23:17:34.14 +53:34:44.7: 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 23:17:34.14 +53:34:44.7: 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 09 09.2599* 23 17 34.14 +53 34 44.7 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,2461292.7599,14.35,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:23:51.71 +56:20:24.8
110.96698 -4.48349 galactic Cas Second-epoch detections are separated by 2.1" 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 | 23:23:51.71 +56:20:24.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:51.71 +56:20:24.8: 15.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:51.71 +56:20:24.8: 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 09 09.2599* 23 23 51.71 +56 20 24.8 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,2461292.7599,14.38,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.24 23:16:19.40 +54:47:52.9
109.42692 -5.56039 galactic Cas Second-epoch detections are separated by 3.2" 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 | 23:16:19.40 +54:47:52.9 (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 23:16:19.40 +54:47:52.9: 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 23:16:19.40 +54:47:52.9: 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 09 09.2599* 23 16 19.40 +54 47 52.9 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,2461292.7599,14.24,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.39 23:29:25.81 +54:56:43.2
111.26090 -6.05734 galactic Cas Second-epoch detections are separated by 3.6" 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 | 23:29:25.81 +54:56:43.2 (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 23:29:25.81 +54:56:43.2: 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 23:29:25.81 +54:56:43.2: 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 09 09.2599* 23 29 25.81 +54 56 43.2 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,2461292.7599,14.39,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.35 23:15:00.68 +55:27:37.5
109.49267 -4.87509 galactic Cas Second-epoch detections are separated by 4.0" 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 | 23:15:00.68 +55:27:37.5 (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 23:15:00.68 +55:27:37.5: 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 23:15:00.68 +55:27:37.5: 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 09 09.2599* 23 15 00.68 +55 27 37.5 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,2461292.7599,14.35,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:44:03.56 +57:40:10.8
113.99443 -4.02817 galactic Cas Second-epoch detections are separated by 2.9" 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 | 23:44:03.56 +57:40:10.8 (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 23:44:03.56 +57:40:10.8: 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 23:44:03.56 +57:40:10.8: 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 09 09.2599* 23 44 03.56 +57 40 10.8 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,2461292.7599,14.38,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.40 23:32:13.05 +54:36:49.8
111.54261 -6.49664 galactic Cas Second-epoch detections are separated by 4.7" 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 | 23:32:13.05 +54:36:49.8 (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 23:32:13.05 +54:36:49.8: 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 23:32:13.05 +54:36:49.8: 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 09 09.2599* 23 32 13.05 +54 36 49.8 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,2461292.7599,14.40,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:22:25.15 +55:31:37.9
110.50212 -5.18153 galactic Cas Second-epoch detections are separated by 8.0" 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 | 23:22:25.15 +55:31:37.9 (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 23:22:25.15 +55:31:37.9: 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 23:22:25.15 +55:31:37.9: 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 09 09.2599* 23 22 25.15 +55 31 37.9 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,2461292.7599,14.38,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:32:03.93 +56:47:02.7
112.18320 -4.42207 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 | 23:32:03.93 +56:47:02.7 (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 23:32:03.93 +56:47:02.7: 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 23:32:03.93 +56:47:02.7: 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 09 09.2599* 23 32 03.93 +56 47 02.7 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,2461292.7599,14.38,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.50 23:23:32.97 +54:29:59.7
110.30785 -6.20338 galactic Cas Second-epoch detections are separated by 7.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:23:32.97 +54:29:59.7 (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 23:23:32.97 +54:29:59.7: 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 23:23:32.97 +54:29:59.7: 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 09 09.2599* 23 23 32.97 +54 29 59.7 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,2461292.7599,14.50,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.26 23:21:26.83 +54:07:11.5
109.88803 -6.45705 galactic Cas Second-epoch detections are separated by 6.7" 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 | 23:21:26.83 +54:07:11.5 (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 23:21:26.83 +54:07:11.5: 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 23:21:26.83 +54:07:11.5: 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 09 09.2599* 23 21 26.83 +54 07 11.5 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,2461292.7599,14.26,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.32 23:34:49.87 +54:52:42.5
111.98435 -6.35672 galactic Cas Second-epoch detections are separated by 2.4" 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 | ATO J353.7144+54.8900 | 23:34:51.46 +54:53:24.0 (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 23:34:49.87 +54:52:42.5: 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 23:34:49.87 +54:52:42.5: 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 09 09.2599* 23 34 49.87 +54 52 42.5 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
ATO J353.7144+54.8900,2461292.7599,14.32,0.05,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
ATO J353.7144+54.8900 20260909.2599 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 09 09.2599 2461292.7599 14.13 23:37:22.76 +57:07:09.6
112.97642 -4.31401 galactic Cas Second-epoch detections are separated by 4.0" 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 | 23:37:22.76 +57:07:09.6 (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 23:37:22.76 +57:07:09.6: 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 23:37:22.76 +57:07:09.6: 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 09 09.2599* 23 37 22.76 +57 07 09.6 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,2461292.7599,14.13,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.35 23:19:56.60 +56:53:58.7
110.64933 -3.77423 galactic Cas Second-epoch detections are separated by 7.1" 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 | 23:19:56.60 +56:53:58.7 (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 23:19:56.60 +56:53:58.7: 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 23:19:56.60 +56:53:58.7: 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 09 09.2599* 23 19 56.60 +56 53 58.7 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,2461292.7599,14.35,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.33 23:24:50.08 +57:00:22.7
111.31448 -3.89918 galactic Cas Second-epoch detections are separated by 8.8" 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 | Gaia DR3 1997332248471101184 | 23:24:51.69 +57:00:55.2 (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 23:24:50.08 +57:00:22.7: 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 23:24:50.08 +57:00:22.7: 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 09 09.2599* 23 24 50.08 +57 00 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
Gaia DR3 1997332248471101184,2461292.7599,14.33,0.05,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
Gaia DR3 1997332248471101184 20260909.2599 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 09 09.2599 2461292.7599 14.20 23:14:54.27 +55:00:57.8
109.31555 -5.28322 galactic Cas Second-epoch detections are separated by 5.5" 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 J348.7395+55.0104 | 23:14:54.27 +55:00:57.8 (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 23:14:54.27 +55:00:57.8: 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 23:14:54.27 +55:00:57.8: 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 09 09.2599* 23 14 54.27 +55 00 57.8 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 J348.7395+55.0104,2461292.7599,14.20,0.05,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 J348.7395+55.0104 20260909.2599 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 09 09.2599 2461292.7599 14.36 23:36:45.10 +57:01:41.5
112.86840 -4.37710 galactic Cas Second-epoch detections are separated by 8.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:36:45.10 +57:01:41.5 (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 23:36:45.10 +57:01:41.5: 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 23:36:45.10 +57:01:41.5: 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 09 09.2599* 23 36 45.10 +57 01 41.5 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,2461292.7599,14.36,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.24 23:14:30.31 +55:30:20.3
109.44229 -4.80678 galactic Cas Second-epoch detections are separated by 2.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.6288+55.4945 | 23:14:30.31 +55:30:20.3 (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 23:14:30.31 +55:30:20.3: 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 23:14:30.31 +55:30:20.3: 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 09 09.2599* 23 14 30.31 +55 30 20.3 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 J348.6288+55.4945,2461292.7599,14.24,0.05,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 J348.6288+55.4945 20260909.2599 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 09 09.2599 2461292.7599 14.36 23:33:48.63 +55:44:18.1
112.10026 -5.49231 galactic Cas Second-epoch detections are separated by 3.1" 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 | 23:33:48.63 +55:44:18.1 (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 23:33:48.63 +55:44:18.1: 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 23:33:48.63 +55:44:18.1: 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 09 09.2599* 23 33 48.63 +55 44 18.1 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,2461292.7599,14.36,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.41 23:23:09.89 +52:36:00.7
109.60986 -7.97326 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 | 23:23:09.89 +52:36:00.7 (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 23:23:09.89 +52:36:00.7: 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 23:23:09.89 +52:36:00.7: 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 09 09.2599* 23 23 09.89 +52 36 00.7 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,2461292.7599,14.41,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.26 23:19:54.88 +54:33:51.7
109.83159 -5.96278 galactic Cas Second-epoch detections are separated by 4.8" 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 | 23:19:54.88 +54:33:51.7 (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 23:19:54.88 +54:33:51.7: 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 23:19:54.88 +54:33:51.7: 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 09 09.2599* 23 19 54.88 +54 33 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,2461292.7599,14.26,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.24 23:27:51.82 +57:07:05.0
111.74121 -3.92670 galactic Cas Second-epoch detections are separated by 8.3" 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 | 23:27:51.82 +57:07:05.0 (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 23:27:51.82 +57:07:05.0: 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 23:27:51.82 +57:07:05.0: 14.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 27 51.82 +57 07 05.0 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,2461292.7599,14.24,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.26 23:19:25.45 +56:55:07.4
110.58940 -3.73170 galactic Cas Second-epoch detections are separated by 2.3" 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 J349.8385+56.9126 | 23:19:25.45 +56:55:07.4 (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 23:19:25.45 +56:55:07.4: 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 23:19:25.45 +56:55:07.4: 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 09 09.2599* 23 19 25.45 +56 55 07.4 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 J349.8385+56.9126,2461292.7599,14.26,0.05,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 J349.8385+56.9126 20260909.2599 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 09 09.2599 2461292.7599 14.18 23:18:08.89 +56:55:36.0
110.42881 -3.66319 galactic Cas Second-epoch detections are separated by 5.3" 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 | 23:18:08.89 +56:55:36.0 (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 23:18:08.89 +56:55:36.0: 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 23:18:08.89 +56:55:36.0: 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 09 09.2599* 23 18 08.89 +56 55 36.0 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,2461292.7599,14.18,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.23 23:33:46.97 +56:23:25.9
112.29104 -4.86842 galactic Cas Second-epoch detections are separated by 1.6" 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 | 23:33:46.97 +56:23:25.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:33:46.97 +56:23:25.9: 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 23:33:46.97 +56:23:25.9: 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 09 09.2599* 23 33 46.97 +56 23 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
target,2461292.7599,14.23,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.16 23:25:09.08 +55:35:12.3
110.88778 -5.25423 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 | 23:25:09.08 +55:35:12.3 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.100 (G)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:25:09.08 +55:35:12.3: 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 23:25:09.08 +55:35:12.3: 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 09 09.2599* 23 25 09.08 +55 35 12.3 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,2461292.7599,14.16,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.24 23:29:44.72 +55:16:19.1
111.40665 -5.76119 galactic Cas Second-epoch detections are separated by 4.7" 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 | 23:29:44.72 +55:16:19.1 (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 23:29:44.72 +55:16:19.1: 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 23:29:44.72 +55:16:19.1: 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 09 09.2599* 23 29 44.72 +55 16 19.1 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,2461292.7599,14.24,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.15 23:14:18.36 +54:02:54.6
108.87773 -6.15150 galactic Cas Second-epoch detections are separated by 4.9" 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 | 23:14:18.36 +54:02:54.6 (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 23:14:18.36 +54:02:54.6: 15.21 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:18.36 +54:02:54.6: 14.73 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.21 +/- 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 09 09.2599* 23 14 18.36 +54 02 54.6 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,2461292.7599,14.15,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.24 23:17:36.98 +52:53:25.7
108.91710 -7.40932 galactic And Second-epoch detections are separated by 6.5" 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 | 23:17:36.98 +52:53:25.7 (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 23:17:36.98 +52:53:25.7: 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 23:17:36.98 +52:53:25.7: 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 09 09.2599* 23 17 36.98 +52 53 25.7 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,2461292.7599,14.24,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.19 23:16:33.42 +56:59:47.7
110.25067 -3.52067 galactic Cas Second-epoch detections are separated by 3.1" 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 | 23:16:33.42 +56:59:47.7 (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 23:16:33.42 +56:59:47.7: 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 23:16:33.42 +56:59:47.7: 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 09 09.2599* 23 16 33.42 +56 59 47.7 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,2461292.7599,14.19,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.19 23:21:45.86 +54:25:14.4
110.03533 -6.19023 galactic Cas Second-epoch detections are separated by 3.0" 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 J350.4525+54.4167 | 23:21:45.86 +54:25:14.4 (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 23:21:45.86 +54:25:14.4: 15.12 +/- 0.25 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:45.86 +54:25:14.4: 14.97 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.12 +/- 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 09 09.2599* 23 21 45.86 +54 25 14.4 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 J350.4525+54.4167,2461292.7599,14.19,0.05,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 J350.4525+54.4167 20260909.2599 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 09 09.2599 2461292.7599 14.32 23:34:25.78 +54:29:17.4
111.81279 -6.71260 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 | 23:34:25.78 +54:29:17.4 (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 23:34:25.78 +54:29:17.4: 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 23:34:25.78 +54:29:17.4: 14.97 +/- 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 09 09.2599* 23 34 25.78 +54 29 17.4 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,2461292.7599,14.32,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.22 23:21:35.97 +52:15:13.3
109.26404 -8.21777 galactic And Second-epoch detections are separated by 4.9" 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 | 23:21:35.97 +52:15:13.3 (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 23:21:35.97 +52:15:13.3: 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 23:21:35.97 +52:15:13.3: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 21 35.97 +52 15 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,2461292.7599,14.22,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.12 23:17:54.28 +55:27:35.5
109.87656 -5.02313 galactic Cas Second-epoch detections are separated by 5.1" 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 | 23:17:54.28 +55:27:35.5 (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 23:17:54.28 +55:27:35.5: 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 23:17:54.28 +55:27:35.5: 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 09 09.2599* 23 17 54.28 +55 27 35.5 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,2461292.7599,14.12,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.40 23:25:12.74 +54:23:17.1
110.49990 -6.38913 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 | 23:25:12.74 +54:23:17.1 (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 23:25:12.74 +54:23:17.1: 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 23:25:12.74 +54:23:17.1: 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 09 09.2599* 23 25 12.74 +54 23 17.1 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,2461292.7599,14.40,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.15 23:18:20.22 +52:39:22.6
108.93573 -7.66698 galactic And Second-epoch detections are separated by 5.4" 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 | ATO J349.5925+52.6543 | 23:18:20.22 +52:39:22.6 (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 23:18:20.22 +52:39:22.6: 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 23:18:20.22 +52:39:22.6: 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 09 09.2599* 23 18 20.22 +52 39 22.6 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
ATO J349.5925+52.6543,2461292.7599,14.15,0.05,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
ATO J349.5925+52.6543 20260909.2599 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 09 09.2599 2461292.7599 14.35 23:14:25.46 +53:35:42.3
108.72614 -6.57952 galactic Cas Second-epoch detections are separated by 5.7" and 7.0 pix
The object was found in VSX19" Gaia DR3 1995566772090189440
Type: ROT
# Max. Min./Amp. JD0 Period
14.850 G 14.880 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 23:14:25.46 +53:35:42.3: 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 23:14:25.46 +53:35:42.3: 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 09 09.2599* 23 14 25.46 +53 35 42.3 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
Gaia DR3 1995566772090189440,2461292.7599,14.35,0.05,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
Gaia DR3 1995566772090189440 20260909.2599 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 09 09.2599 2461292.7599 14.22 23:37:34.22 +55:28:31.4
112.53417 -5.89806 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 | Gaia DR3 1997509746575583360 | 23:37:30.06 +55:28:22.7 (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 23:37:34.22 +55:28:31.4: 15.15 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:34.22 +55:28:31.4: 15.08 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.15 +/- 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 09 09.2599* 23 37 34.22 +55 28 31.4 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
Gaia DR3 1997509746575583360,2461292.7599,14.22,0.05,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
Gaia DR3 1997509746575583360 20260909.2599 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 09 09.2599 2461292.7599 14.18 23:26:55.39 +57:19:49.3
111.68839 -3.68484 galactic Cas Second-epoch detections are separated by 7.4" 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 | 23:26:55.39 +57:19:49.3 (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 23:26:55.39 +57:19:49.3: 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 23:26:55.39 +57:19:49.3: 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 09 09.2599* 23 26 55.39 +57 19 49.3 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,2461292.7599,14.18,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.06 23:13:47.45 +56:30:59.2
109.72183 -3.83005 galactic Cas Second-epoch detections are separated by 6.0" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:13:47.45 +56:30:59.2 (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 23:13:47.45 +56:30:59.2: 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 23:13:47.45 +56:30:59.2: 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 09 09.2599* 23 13 47.45 +56 30 59.2 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,2461292.7599,14.06,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.15 23:21:14.77 +54:14:41.7
109.90340 -6.32950 galactic Cas Second-epoch detections are separated by 7.7" 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 | 23:21:14.77 +54:14:41.7 (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 23:21:14.77 +54:14:41.7: 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 23:21:14.77 +54:14:41.7: 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 09 09.2599* 23 21 14.77 +54 14 41.7 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,2461292.7599,14.15,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.27 23:32:57.84 +55:20:35.9
111.86684 -5.83355 galactic Cas Second-epoch detections are separated by 5.8" 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 | target | 23:32:57.84 +55:20:35.9 (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 23:32:57.84 +55:20:35.9: 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 23:32:57.84 +55:20:35.9: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 32 57.84 +55 20 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
target,2461292.7599,14.27,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.21 23:16:51.96 +54:13:37.3
109.29430 -6.12150 galactic Cas Second-epoch detections are separated by 7.4" 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 | 23:16:51.96 +54:13:37.3 (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 23:16:51.96 +54:13:37.3: 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 23:16:51.96 +54:13:37.3: 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 09 09.2599* 23 16 51.96 +54 13 37.3 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,2461292.7599,14.21,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.22 23:35:58.96 +54:45:35.1
112.10916 -6.51866 galactic Cas Second-epoch detections are separated by 2.6" 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 | ATO J353.9747+54.7618 | 23:35:58.96 +54:45:35.1 (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 23:35:58.96 +54:45:35.1: 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 23:35:58.96 +54:45:35.1: 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 09 09.2599* 23 35 58.96 +54 45 35.1 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 J353.9747+54.7618,2461292.7599,14.22,0.05,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 J353.9747+54.7618 20260909.2599 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 09 09.2599 2461292.7599 14.32 23:26:07.61 +57:14:57.4
111.56012 -3.72684 galactic Cas Second-epoch detections are separated by 8.3" 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 | 23:26:07.61 +57:14:57.4 (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 23:26:07.61 +57:14:57.4: 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 23:26:07.61 +57:14:57.4: 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 09 09.2599* 23 26 07.61 +57 14 57.4 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,2461292.7599,14.32,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.25 23:31:32.30 +54:31:32.9
111.42125 -6.55049 galactic Cas Second-epoch detections are separated by 6.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:31:32.30 +54:31:32.9 (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 23:31:32.30 +54:31:32.9: 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 23:31:32.30 +54:31:32.9: 15.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 31 32.30 +54 31 32.9 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,2461292.7599,14.25,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.14 23:15:19.57 +56:28:53.9
109.90668 -3.93997 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 | 23:15:19.57 +56:28:53.9 (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 23:15:19.57 +56:28:53.9: 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 23:15:19.57 +56:28:53.9: 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 09 09.2599* 23 15 19.57 +56 28 53.9 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,2461292.7599,14.14,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.24 23:13:58.59 +56:31:17.4
109.74755 -3.83479 galactic Cas Second-epoch detections are separated by 0.7" and 7.2 pix
The object was found in VSX13" Gaia DR3 2009243086136077056
Type: ROT
# Max. Min./Amp. JD0 Period
16.040 G 16.090 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 23:13:58.59 +56:31:17.4: 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 23:13:58.59 +56:31:17.4: 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 09 09.2599* 23 13 58.59 +56 31 17.4 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
Gaia DR3 2009243086136077056,2461292.7599,14.24,0.05,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
Gaia DR3 2009243086136077056 20260909.2599 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 09 09.2599 2461292.7599 14.17 23:42:06.81 +57:58:08.8
113.82250 -3.67129 galactic Cas Second-epoch detections are separated by 7.3" 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 | 23:42:06.81 +57:58:08.8 (user input) | T | P | (position from user input) J-Ks=1.064+/-0.306 (M)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:06.81 +57:58:08.8: 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 23:42:06.81 +57:58:08.8: 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 09 09.2599* 23 42 06.81 +57 58 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,2461292.7599,14.17,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.36 23:16:30.27 +53:08:44.7
108.85220 -7.11103 galactic And Second-epoch detections are separated by 2.7" 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 | 23:16:30.27 +53:08:44.7 (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 23:16:30.27 +53:08:44.7: 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 23:16:30.27 +53:08:44.7: 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 09 09.2599* 23 16 30.27 +53 08 44.7 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,2461292.7599,14.36,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.22 23:25:53.49 +55:45:47.2
111.04473 -5.12172 galactic Cas Second-epoch detections are separated by 6.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J351.4867+55.7532 | 23:25:53.49 +55:45:47.2 (user input) | CBF (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 23:25:53.49 +55:45:47.2: 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 23:25:53.49 +55:45:47.2: 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 09 09.2599* 23 25 53.49 +55 45 47.2 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
ATO J351.4867+55.7532,2461292.7599,14.22,0.05,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 J351.4867+55.7532 20260909.2599 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 09 09.2599 2461292.7599 14.15 23:32:21.04 +56:19:24.7
112.08096 -4.87293 galactic Cas Second-epoch detections are separated by 1.1" 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 J353.0924+56.3256 | 23:32:21.04 +56:19:24.7 (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 23:32:21.04 +56:19:24.7: 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 23:32:21.04 +56:19:24.7: 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 09 09.2599* 23 32 21.04 +56 19 24.7 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 J353.0924+56.3256,2461292.7599,14.15,0.05,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
ATO J353.0924+56.3256 20260909.2599 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 09 09.2599 2461292.7599 14.18 23:21:21.42 +56:54:37.7
110.83466 -3.83047 galactic Cas Second-epoch detections are separated by 4.3" 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 | 23:21:21.42 +56:54:37.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:21.42 +56:54:37.7: 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 23:21:21.42 +56:54:37.7: 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 09 09.2599* 23 21 21.42 +56 54 37.7 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,2461292.7599,14.18,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.23 23:45:57.96 +57:31:58.3
114.20705 -4.22559 galactic Cas Second-epoch detections are separated by 7.2" and 6.8 pix
The object was found in VSX15" ZTF J234556.19+573201.3
Type: EW
# Max. Min./Amp. JD0 Period
17.743 r Y 0.194 r 2458437.77940 0.301362200000
ATTENTION: measured mag 14.23 is 3.3 mag brighter than the VSX record maximum brightness 17.55 - 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 23:45:57.96 +57:31:58.3: 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 23:45:57.96 +57:31:58.3: 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 09 09.2599* 23 45 57.96 +57 31 58.3 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
ZTF J234556.19+573201.3,2461292.7599,14.23,0.05,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
ZTF J234556.19+573201.3 20260909.2599 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 09 09.2599 2461292.7599 14.12 23:17:37.23 +51:54:22.0
108.56233 -8.32882 galactic And Second-epoch detections are separated by 8.4" 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 | 23:17:37.23 +51:54:22.0 (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 23:17:37.23 +51:54:22.0: 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 23:17:37.23 +51:54:22.0: 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 09 09.2599* 23 17 37.23 +51 54 22.0 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,2461292.7599,14.12,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.21 23:27:57.66 +55:37:44.4
111.27854 -5.34262 galactic Cas Second-epoch detections are separated by 2.5" 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 J352.0099+55.6264 | 23:27:57.66 +55:37:44.4 (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 23:27:57.66 +55:37:44.4: 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 23:27:57.66 +55:37:44.4: 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 09 09.2599* 23 27 57.66 +55 37 44.4 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 J352.0099+55.6264,2461292.7599,14.21,0.05,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
ATO J352.0099+55.6264 20260909.2599 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 09 09.2599 2461292.7599 14.30 23:15:16.56 +53:02:09.3
108.63881 -7.14637 galactic And Second-epoch detections are separated by 8.3" and 7.0 pix
The object was found in VSX20" Gaia DR3 1995303271560133376
Type: ROT
# Max. Min./Amp. JD0 Period
15.970 G 16.030 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 23:15:16.56 +53:02:09.3: 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 23:15:16.56 +53:02:09.3: 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 09 09.2599* 23 15 16.56 +53 02 09.3 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 1995303271560133376,2461292.7599,14.30,0.05,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 1995303271560133376 20260909.2599 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 09 09.2599 2461292.7599 14.16 23:44:44.22 +57:54:11.1
114.14209 -3.82584 galactic Cas Second-epoch detections are separated by 7.1" 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 | ATO J356.1751+57.8910 | 23:44:44.22 +57:54:11.1 (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 23:44:44.22 +57:54:11.1: 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 23:44:44.22 +57:54:11.1: 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 09 09.2599* 23 44 44.22 +57 54 11.1 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 J356.1751+57.8910,2461292.7599,14.16,0.05,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
ATO J356.1751+57.8910 20260909.2599 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 09 09.2599 2461292.7599 14.34 23:45:58.71 +56:57:42.7
114.06460 -4.77865 galactic Cas Second-epoch detections are separated by 6.3" 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 | 23:45:58.71 +56:57:42.7 (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 23:45:58.71 +56:57:42.7: 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 23:45:58.71 +56:57:42.7: 14.90 +/- 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 09 09.2599* 23 45 58.71 +56 57 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,2461292.7599,14.34,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.22 23:29:41.45 +55:55:24.8
111.60357 -5.13975 galactic Cas 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 | target | 23:29:41.45 +55:55:24.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:41.45 +55:55:24.8: 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 23:29:41.45 +55:55:24.8: 15.00 +/- 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 09 09.2599* 23 29 41.45 +55 55 24.8 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,2461292.7599,14.22,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.18 23:19:39.77 +55:04:10.7
109.97425 -5.47649 galactic Cas Second-epoch detections are separated by 7.0" 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 | 23:19:39.77 +55:04:10.7 (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 23:19:39.77 +55:04:10.7: 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 23:19:39.77 +55:04:10.7: 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 09 09.2599* 23 19 39.77 +55 04 10.7 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,2461292.7599,14.18,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.22 23:19:48.73 +52:55:01.9
109.23901 -7.50131 galactic And Second-epoch detections are separated by 7.2" 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 | 23:19:48.73 +52:55:01.9 (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 23:19:48.73 +52:55:01.9: 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 23:19:48.73 +52:55:01.9: 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 09 09.2599* 23 19 48.73 +52 55 01.9 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,2461292.7599,14.22,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.22 23:18:08.05 +53:41:11.3
109.27552 -6.69303 galactic Cas Second-epoch detections are separated by 0.7" 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 | 23:18:08.05 +53:41:11.3 (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 23:18:08.05 +53:41:11.3: 15.24 +/- 0.33 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:08.05 +53:41:11.3: 14.77 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.24 +/- 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 09 09.2599* 23 18 08.05 +53 41 11.3 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,2461292.7599,14.22,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.20 23:32:36.20 +55:07:12.7
111.75000 -6.03083 galactic Cas Second-epoch detections are separated by 6.1" 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 | 23:32:36.20 +55:07:12.7 (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 23:32:36.20 +55:07:12.7: 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 23:32:36.20 +55:07:12.7: 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 09 09.2599* 23 32 36.20 +55 07 12.7 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,2461292.7599,14.20,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.12 23:22:07.86 +54:45:26.6
110.20089 -5.89174 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 | 23:22:07.86 +54:45:26.6 (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 23:22:07.86 +54:45:26.6: 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 23:22:07.86 +54:45:26.6: 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 09 09.2599* 23 22 07.86 +54 45 26.6 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,2461292.7599,14.12,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.11 23:18:06.95 +55:05:34.2
109.77423 -5.37701 galactic Cas Second-epoch detections are separated by 8.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J349.5108+55.0948 | 23:18:06.95 +55:05:34.2 (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 23:18:06.95 +55:05:34.2: 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 23:18:06.95 +55:05:34.2: 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 09 09.2599* 23 18 06.95 +55 05 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
ATO J349.5108+55.0948,2461292.7599,14.11,0.05,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 J349.5108+55.0948 20260909.2599 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 09 09.2599 2461292.7599 14.09 23:23:10.72 +56:57:08.7
111.08325 -3.87509 galactic Cas Second-epoch detections are separated by 8.7" 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 | 23:23:10.72 +56:57:08.7 (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 23:23:10.72 +56:57:08.7: 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 23:23:10.72 +56:57:08.7: 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 09 09.2599* 23 23 10.72 +56 57 08.7 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,2461292.7599,14.09,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.01 23:16:20.46 +52:05:57.6
108.44705 -8.07763 galactic And Second-epoch detections are separated by 6.1" 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 | 23:16:20.46 +52:05:57.6 (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 23:16:20.46 +52:05:57.6: 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 23:16:20.46 +52:05:57.6: 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 09 09.2599* 23 16 20.46 +52 05 57.6 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,2461292.7599,14.01,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.14 23:35:43.23 +54:55:15.1
112.11984 -6.35353 galactic Cas Second-epoch detections are separated by 4.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:35:43.23 +54:55:15.1 (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 23:35:43.23 +54:55:15.1: 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 23:35:43.23 +54:55:15.1: 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 09 09.2599* 23 35 43.23 +54 55 15.1 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,2461292.7599,14.14,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.20 23:26:02.49 +55:37:17.4
111.01850 -5.26250 galactic Cas Second-epoch detections are separated by 6.5" 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 J351.4984+55.6136 | 23:26:02.49 +55:37:17.4 (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 23:26:02.49 +55:37:17.4: 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 23:26:02.49 +55:37:17.4: 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 09 09.2599* 23 26 02.49 +55 37 17.4 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 J351.4984+55.6136,2461292.7599,14.20,0.05,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 J351.4984+55.6136 20260909.2599 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 09 09.2599 2461292.7599 14.17 23:19:35.83 +54:10:39.1
109.65237 -6.30922 galactic Cas Second-epoch detections are separated by 6.6" 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 | 23:19:35.83 +54:10:39.1 (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 23:19:35.83 +54:10:39.1: 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 23:19:35.83 +54:10:39.1: 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 09 09.2599* 23 19 35.83 +54 10 39.1 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,2461292.7599,14.17,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.08 23:16:25.10 +54:01:09.4
109.15755 -6.29173 galactic Cas Second-epoch detections are separated by 0.6" 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 | 23:16:25.10 +54:01:09.4 (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 23:16:25.10 +54:01:09.4: 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 23:16:25.10 +54:01:09.4: 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 09 09.2599* 23 16 25.10 +54 01 09.4 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,2461292.7599,14.08,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.18 23:17:11.07 +53:36:00.8
109.11216 -6.72343 galactic Cas Second-epoch detections are separated by 1.8" 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 | 23:17:11.07 +53:36:00.8 (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 23:17:11.07 +53:36:00.8: 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 23:17:11.07 +53:36:00.8: 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 09 09.2599* 23 17 11.07 +53 36 00.8 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,2461292.7599,14.18,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.17 23:30:41.40 +55:31:43.5
111.61484 -5.55872 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 | 23:30:41.40 +55:31:43.5 (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 23:30:41.40 +55:31:43.5: 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 23:30:41.40 +55:31:43.5: 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 09 09.2599* 23 30 41.40 +55 31 43.5 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,2461292.7599,14.17,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.11 23:20:27.83 +51:25:08.0
108.80553 -8.94035 galactic And Second-epoch detections are separated by 2.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.1080+51.4135 | 23:20:27.83 +51:25:08.0 (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 23:20:27.83 +51:25:08.0: 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 23:20:27.83 +51:25:08.0: 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 09 09.2599* 23 20 27.83 +51 25 08.0 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 J350.1080+51.4135,2461292.7599,14.11,0.05,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 J350.1080+51.4135 20260909.2599 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 09 09.2599 2461292.7599 14.21 23:17:08.15 +53:54:15.9
109.21509 -6.43685 galactic Cas Second-epoch detections are separated by 2.8" 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 | 23:17:08.15 +53:54:15.9 (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 23:17:08.15 +53:54:15.9: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:08.15 +53:54:15.9: 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 09 09.2599* 23 17 08.15 +53 54 15.9 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,2461292.7599,14.21,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.12 23:14:39.23 +54:17:58.8
109.01813 -5.93660 galactic Cas Second-epoch detections are separated by 3.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.6647+54.3080 | 23:14:39.23 +54:17:58.8 (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 23:14:39.23 +54:17:58.8: 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 23:14:39.23 +54:17:58.8: 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 09 09.2599* 23 14 39.23 +54 17 58.8 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
ATO J348.6647+54.3080,2461292.7599,14.12,0.05,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 J348.6647+54.3080 20260909.2599 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 09 09.2599 2461292.7599 14.01 23:18:33.81 +55:52:09.0
110.10892 -4.67305 galactic Cas Second-epoch detections are separated by 8.8" 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 | target | 23:18:33.81 +55:52:09.0 (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 23:18:33.81 +55:52:09.0: 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 23:18:33.81 +55:52:09.0: 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 09 09.2599* 23 18 33.81 +55 52 09.0 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,2461292.7599,14.01,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.88 23:14:09.14 +56:26:10.1
109.73872 -3.92309 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 | ATO J348.5475+56.4478 | 23:14:09.14 +56:26:10.1 (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 23:14:09.14 +56:26:10.1: 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 23:14:09.14 +56:26:10.1: 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 09 09.2599* 23 14 09.14 +56 26 10.1 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
ATO J348.5475+56.4478,2461292.7599,13.88,0.05,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
ATO J348.5475+56.4478 20260909.2599 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 09 09.2599 2461292.7599 14.02 23:40:01.78 +56:50:24.8
113.24626 -4.68265 galactic Cas Second-epoch detections are separated by 7.5" 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 | target | 23:40:01.78 +56:50:24.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:40:01.78 +56:50:24.8: 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 23:40:01.78 +56:50:24.8: 15.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 40 01.78 +56 50 24.8 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,2461292.7599,14.02,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.02 23:27:25.75 +53:28:43.0
110.51265 -7.35526 galactic Cas Second-epoch detections are separated by 6.0" 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 | Gaia DR3 1992756218512829056 | 23:27:22.77 +53:29:04.5 (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 23:27:25.75 +53:28:43.0: 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 23:27:25.75 +53:28:43.0: 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 09 09.2599* 23 27 25.75 +53 28 43.0 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 1992756218512829056,2461292.7599,14.02,0.05,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
Gaia DR3 1992756218512829056 20260909.2599 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 09 09.2599 2461292.7599 13.97 23:16:22.30 +53:52:52.6
109.10101 -6.41796 galactic Cas Second-epoch detections are separated by 1.1" 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 | 23:16:22.30 +53:52:52.6 (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 23:16:22.30 +53:52:52.6: 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 23:16:22.30 +53:52:52.6: 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 09 09.2599* 23 16 22.30 +53 52 52.6 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,2461292.7599,13.97,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.92 23:27:25.75 +56:43:28.8
111.55906 -4.28063 galactic Cas Second-epoch detections are separated by 6.4" 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 | 23:27:25.75 +56:43:28.8 (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 23:27:25.75 +56:43:28.8: 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 23:27:25.75 +56:43:28.8: 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 09 09.2599* 23 27 25.75 +56 43 28.8 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,2461292.7599,13.92,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.93 23:13:32.11 +54:36:44.4
108.98207 -5.58603 galactic Cas Second-epoch detections are separated by 5.2" 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 | 23:13:32.11 +54:36:44.4 (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 23:13:32.11 +54:36:44.4: 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 23:13:32.11 +54:36:44.4: 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 09 09.2599* 23 13 32.11 +54 36 44.4 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,2461292.7599,13.93,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.93 23:35:55.50 +54:52:45.0
112.13597 -6.40196 galactic Cas Second-epoch detections are separated by 4.3" 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 | ATO J353.9615+54.8758 | 23:35:55.50 +54:52:45.0 (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 23:35:55.50 +54:52:45.0: 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 23:35:55.50 +54:52:45.0: 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 09 09.2599* 23 35 55.50 +54 52 45.0 13.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J353.9615+54.8758,2461292.7599,13.93,0.05,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 J353.9615+54.8758 20260909.2599 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 09 09.2599 2461292.7599 13.91 23:14:34.44 +55:57:47.9
109.61954 -4.38448 galactic Cas Second-epoch detections are separated by 5.0" 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 | 23:14:34.44 +55:57:47.9 (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 23:14:34.44 +55:57:47.9: 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 23:14:34.44 +55:57:47.9: 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 09 09.2599* 23 14 34.44 +55 57 47.9 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,2461292.7599,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 13.95 23:14:15.61 +53:53:54.8
108.81588 -6.28843 galactic Cas Second-epoch detections are separated by 5.3" 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 | 23:14:15.61 +53:53:54.8 (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 23:14:15.61 +53:53:54.8: 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 23:14:15.61 +53:53:54.8: 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 09 09.2599* 23 14 15.61 +53 53 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,2461292.7599,13.95,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.93 23:28:14.02 +57:41:39.9
111.97186 -3.39595 galactic Cas Second-epoch detections are separated by 5.0" 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 | 23:28:14.02 +57:41:39.9 (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 23:28:14.02 +57:41:39.9: 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 23:28:14.02 +57:41:39.9: 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 09 09.2599* 23 28 14.02 +57 41 39.9 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,2461292.7599,13.93,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.03 23:47:29.00 +57:54:32.3
114.49750 -3.91165 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 | 23:47:29.00 +57:54:32.3 (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 23:47:29.00 +57:54:32.3: 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 23:47:29.00 +57:54:32.3: 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 09 09.2599* 23 47 29.00 +57 54 32.3 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,2461292.7599,14.03,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.01 23:38:31.97 +56:57:45.4
113.08319 -4.50854 galactic Cas Second-epoch detections are separated by 4.1" and 6.9 pix
The object was found in VSX20" Gaia DR3 1998623654937915520
Type: RS
# Max. Min./Amp. JD0 Period
15.000 G 15.170 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 23:38:31.97 +56:57:45.4: 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 23:38:31.97 +56:57:45.4: 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 09 09.2599* 23 38 31.97 +56 57 45.4 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
Gaia DR3 1998623654937915520,2461292.7599,14.01,0.05,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
Gaia DR3 1998623654937915520 20260909.2599 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 09 09.2599 2461292.7599 14.06 23:32:02.00 +54:33:58.2
111.50245 -6.53395 galactic Cas Second-epoch detections are separated by 8.5" 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 | 23:32:02.00 +54:33:58.2 (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 23:32:02.00 +54:33:58.2: 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 23:32:02.00 +54:33:58.2: 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 09 09.2599* 23 32 02.00 +54 33 58.2 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,2461292.7599,14.06,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.90 23:17:11.07 +56:03:01.7
109.99236 -4.43511 galactic Cas Second-epoch detections are separated by 5.8" 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 | 23:17:11.07 +56:03:01.7 (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 23:17:11.07 +56:03:01.7: 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 23:17:11.07 +56:03:01.7: 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 09 09.2599* 23 17 11.07 +56 03 01.7 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,2461292.7599,13.90,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.90 23:11:46.64 +55:24:34.7
109.04624 -4.75230 galactic Cas Second-epoch detections are separated by 5.6" 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 | ATO J347.9633+55.4098 | 23:11:46.64 +55:24:34.7 (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 23:11:46.64 +55:24:34.7: 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 23:11:46.64 +55:24:34.7: 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 09 09.2599* 23 11 46.64 +55 24 34.7 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
ATO J347.9633+55.4098,2461292.7599,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J347.9633+55.4098 20260909.2599 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 09 09.2599 2461292.7599 13.87 23:23:03.31 +55:20:04.8
110.52218 -5.39321 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 | 23:23:03.31 +55:20:04.8 (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 23:23:03.31 +55:20:04.8: 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 23:23:03.31 +55:20:04.8: 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 09 09.2599* 23 23 03.31 +55 20 04.8 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,2461292.7599,13.87,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.00 23:13:56.59 +54:17:45.0
108.91979 -5.90201 galactic Cas Second-epoch detections are separated by 7.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:13:56.59 +54:17:45.0 (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 23:13:56.59 +54:17:45.0: 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 23:13:56.59 +54:17:45.0: 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 09 09.2599* 23 13 56.59 +54 17 45.0 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,2461292.7599,14.00,0.05,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
target 20260909.2599 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 09 09.2599 2461292.7599 13.85 23:14:34.19 +57:04:36.0
110.02732 -3.34812 galactic Cas Second-epoch detections are separated by 6.8" 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 | 23:14:34.19 +57:04:36.0 (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 23:14:34.19 +57:04:36.0: 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 23:14:34.19 +57:04:36.0: 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 09 09.2599* 23 14 34.19 +57 04 36.0 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,2461292.7599,13.85,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.92 23:27:59.89 +56:00:06.1
111.40261 -4.99096 galactic Cas Second-epoch detections are separated by 1.7" 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 | 23:27:59.89 +56:00:06.1 (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 23:27:59.89 +56:00:06.1: 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 23:27:59.89 +56:00:06.1: 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 09 09.2599* 23 27 59.89 +56 00 06.1 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,2461292.7599,13.92,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.88 23:16:35.08 +56:46:41.8
110.17574 -3.72580 galactic Cas Second-epoch detections are separated by 8.5" 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 | 23:16:35.08 +56:46:41.8 (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 23:16:35.08 +56:46:41.8: 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 23:16:35.08 +56:46:41.8: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 16 35.08 +56 46 41.8 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,2461292.7599,13.88,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.94 23:26:18.51 +55:19:51.5
110.95960 -5.54955 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 | 23:26:18.51 +55:19:51.5 (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 23:26:18.51 +55:19:51.5: 14.84 +/- 0.20 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:18.51 +55:19:51.5: 14.90 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.84 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 26 18.51 +55 19 51.5 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,2461292.7599,13.94,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.79 23:30:01.22 +55:54:14.2
111.64149 -5.17276 galactic Cas Second-epoch detections are separated by 3.8" 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 | 23:30:01.22 +55:54:14.2 (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 23:30:01.22 +55:54:14.2: 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 23:30:01.22 +55:54:14.2: 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 09 09.2599* 23 30 01.22 +55 54 14.2 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,13.79,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.80 23:30:15.05 +55:35:38.9
111.57585 -5.47733 galactic Cas Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.5770+55.5988 | 23:30:15.05 +55:35:38.9 (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 23:30:15.05 +55:35:38.9: 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 23:30:15.05 +55:35:38.9: 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 09 09.2599* 23 30 15.05 +55 35 38.9 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 J352.5770+55.5988,2461292.7599,13.80,0.05,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
ATO J352.5770+55.5988 20260909.2599 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 09 09.2599 2461292.7599 13.82 23:14:30.40 +53:29:10.0
108.69723 -6.68534 galactic Cas Second-epoch detections are separated by 8.7" 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 | 23:14:30.40 +53:29:10.0 (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 23:14:30.40 +53:29:10.0: 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 23:14:30.40 +53:29:10.0: 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 09 09.2599* 23 14 30.40 +53 29 10.0 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,2461292.7599,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 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 09 09.2599 2461292.7599 13.85 23:37:47.13 +58:01:32.6
113.28543 -3.45993 galactic Cas Second-epoch detections are separated by 2.5" and 7.0 pix
The object was found in VSX12" Gaia DR3 1998927364963638272
Type: VAR
# Max. Min./Amp. JD0 Period
15.220 G 15.380 G 0.018813200000 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 23:37:47.13 +58:01:32.6: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:47.13 +58:01:32.6: 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 09 09.2599* 23 37 47.13 +58 01 32.6 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1998927364963638272,2461292.7599,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1998927364963638272 20260909.2599 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 09 09.2599 2461292.7599 13.80 23:36:17.30 +58:00:14.4
113.08882 -3.42437 galactic Cas Second-epoch detections are separated by 4.9" 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 | 23:36:17.30 +58:00:14.4 (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 23:36:17.30 +58:00:14.4: 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 23:36:17.30 +58:00:14.4: 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 09 09.2599* 23 36 17.30 +58 00 14.4 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,2461292.7599,13.80,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.81 23:43:53.25 +57:35:52.5
113.95354 -4.09152 galactic Cas Second-epoch detections are separated by 6.7" 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 | 23:43:53.25 +57:35:52.5 (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 23:43:53.25 +57:35:52.5: 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 23:43:53.25 +57:35:52.5: 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 09 09.2599* 23 43 53.25 +57 35 52.5 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 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 09 09.2599 2461292.7599 13.79 23:24:48.05 +56:02:35.3
110.99189 -4.80707 galactic Cas Second-epoch detections are separated by 2.1" 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 | 23:24:48.05 +56:02:35.3 (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 23:24:48.05 +56:02:35.3: 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 23:24:48.05 +56:02:35.3: 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 09 09.2599* 23 24 48.05 +56 02 35.3 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,2461292.7599,13.79,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.79 23:26:39.23 +55:39:34.7
111.11299 -5.25444 galactic Cas Second-epoch detections are separated by 0.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J351.6844+55.6552 | 23:26:39.23 +55:39:34.7 (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 23:26:39.23 +55:39:34.7: 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 23:26:39.23 +55:39:34.7: 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 09 09.2599* 23 26 39.23 +55 39 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
ATO J351.6844+55.6552,2461292.7599,13.79,0.05,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 J351.6844+55.6552 20260909.2599 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 09 09.2599 2461292.7599 13.85 23:18:42.39 +54:57:41.2
109.80718 -5.52982 galactic Cas Second-epoch detections are separated by 4.8" and 7.0 pix
The object was found in VSX 5" Gaia DR3 1996825030011876864
Type: ROT
# Max. Min./Amp. JD0 Period
16.380 G 16.440 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 23:18:42.39 +54:57:41.2: 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 23:18:42.39 +54:57:41.2: 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 09 09.2599* 23 18 42.39 +54 57 41.2 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1996825030011876864,2461292.7599,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1996825030011876864 20260909.2599 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 09 09.2599 2461292.7599 13.80 23:20:45.16 +55:50:06.0
110.38596 -4.81203 galactic Cas Second-epoch detections are separated by 7.7" 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 | 23:20:45.16 +55:50:06.0 (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 23:20:45.16 +55:50:06.0: 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 23:20:45.16 +55:50:06.0: 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 09 09.2599* 23 20 45.16 +55 50 06.0 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,2461292.7599,13.80,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.70 23:13:55.38 +55:27:50.3
109.34996 -4.81521 galactic Cas Second-epoch detections are separated by 8.0" 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 | 23:13:55.38 +55:27:50.3 (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 23:13:55.38 +55:27:50.3: 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 23:13:55.38 +55:27:50.3: 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 09 09.2599* 23 13 55.38 +55 27 50.3 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,2461292.7599,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 13.86 00:26:17.02 +49:45:32.0
118.76883 -12.90942 galactic Cas Second-epoch detections are separated by 1.6" 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 | 00:26:17.02 +49:45:32.0 (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 00:26:17.02 +49:45:32.0: 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 00:26:17.02 +49:45:32.0: 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 09 09.2599* 00 26 17.02 +49 45 32.0 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,2461292.7599,13.86,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.72 23:15:13.69 +52:09:41.4
108.30930 -7.95752 galactic And Second-epoch detections are separated by 6.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.7950+52.1634 | 23:15:09.24 +52:10:03.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:13.69 +52:09:41.4: 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 23:15:13.69 +52:09:41.4: 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 09 09.2599* 23 15 13.69 +52 09 41.4 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.7950+52.1634,2461292.7599,13.72,0.05,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 J348.7950+52.1634 20260909.2599 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 09 09.2599 2461292.7599 13.51 23:46:40.40 +57:42:14.9
114.34194 -4.08344 galactic Cas Second-epoch detections are separated by 2.4" 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 | ATO J356.6480+57.7053 | 23:46:38.32 +57:41:43.8 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | 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 23:46:40.40 +57:42:14.9: 15.13 +/- 0.23 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:46:40.40 +57:42:14.9: 14.98 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.13 +/- 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 09 09.2599* 23 46 40.40 +57 42 14.9 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.6480+57.7053,2461292.7599,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.6480+57.7053 20260909.2599 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 09 09.2599 2461292.7599 13.43 23:18:01.30 +54:07:27.0
109.41626 -6.27794 galactic Cas Second-epoch detections are separated by 8.0" 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 | Gaia DR3 1995967337921119232 | 23:18:03.31 +54:06:51.3 (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 23:18:01.30 +54:07:27.0: 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 23:18:01.30 +54:07:27.0: 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 09 09.2599* 23 18 01.30 +54 07 27.0 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995967337921119232,2461292.7599,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995967337921119232 20260909.2599 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 13.45 23:16:09.31 +53:48:25.6
109.04407 -6.47558 galactic Cas Second-epoch detections are separated by 0.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J349.0407+53.7944 | 23:16:09.31 +53:48:25.6 (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 23:16:09.31 +53:48:25.6: 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 23:16:09.31 +53:48:25.6: 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 09 09.2599* 23 16 09.31 +53 48 25.6 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J349.0407+53.7944,2461292.7599,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.0407+53.7944 20260909.2599 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 13.31 23:21:55.39 +54:35:42.1
110.11693 -6.03419 galactic Cas Second-epoch detections are separated by 3.2" 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 | 23:21:55.39 +54:35:42.1 (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 23:21:55.39 +54:35:42.1: 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 23:21:55.39 +54:35:42.1: 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 09 09.2599* 23 21 55.39 +54 35 42.1 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 13.34 23:15:15.23 +53:51:11.9
108.93628 -6.38422 galactic Cas Second-epoch detections are separated by 2.0" and 7.0 pix
The object was found in VSX20" Gaia DR3 1995585639890167040
Type: E
# Max. Min./Amp. JD0 Period
13.860 G 13.940 G 0.462859000000 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 23:15:15.23 +53:51:11.9: 14.41 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:15.23 +53:51:11.9: 14.83 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.41 +/- 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 09 09.2599* 23 15 15.23 +53 51 11.9 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1995585639890167040,2461292.7599,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1995585639890167040 20260909.2599 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 13.27 23:32:32.93 +56:41:23.6
112.21802 -4.53189 galactic Cas Second-epoch detections are separated by 2.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:32:32.93 +56:41:23.6 (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 23:32:32.93 +56:41:23.6: 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 23:32:32.93 +56:41:23.6: 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 09 09.2599* 23 32 32.93 +56 41 23.6 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
target,2461292.7599,13.27,0.05,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 20260909.2599 13.27CV 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 09 09.2599 2461292.7599 13.30 23:14:58.02 +56:01:19.0
109.69233 -4.34998 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 | ATO J348.7398+56.0329 | 23:14:58.02 +56:01:19.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.479+/-0.234 (K)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:14:58.02 +56:01:19.0: 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 23:14:58.02 +56:01:19.0: 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 09 09.2599* 23 14 58.02 +56 01 19.0 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J348.7398+56.0329,2461292.7599,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J348.7398+56.0329 20260909.2599 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 13.05 23:28:13.78 +55:31:06.4
111.27939 -5.45951 galactic Cas Second-epoch detections are separated by 1.9" 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 | 23:28:13.78 +55:31:06.4 (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 23:28:13.78 +55:31:06.4: 15.32 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:13.78 +55:31:06.4: 14.80 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.32 +/- 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 09 09.2599* 23 28 13.78 +55 31 06.4 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 12.67 23:15:45.35 +54:47:50.6
109.35008 -5.53142 galactic Cas Second-epoch detections are separated by 3.1" 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 | 23:15:45.35 +54:47:50.6 (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 23:15:45.35 +54:47:50.6: 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 23:15:45.35 +54:47:50.6: 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 09 09.2599* 23 15 45.35 +54 47 50.6 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,2461292.7599,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 12.59 23:11:24.30 +55:58:54.2
109.21368 -4.20260 galactic Cas Second-epoch detections are separated by 0.7" 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 | 23:11:24.30 +55:58:54.2 (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 23:11:24.30 +55:58:54.2: 15.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:11:24.30 +55:58:54.2: 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 09 09.2599* 23 11 24.30 +55 58 54.2 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 11.78 23:29:17.34 +54:35:12.9
111.12831 -6.39126 galactic Cas Second-epoch detections are separated by 1.8" 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 | 23:29:17.34 +54:35:12.9 (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 23:29:17.34 +54:35:12.9: 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 23:29:17.34 +54:35:12.9: 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 09 09.2599* 23 29 17.34 +54 35 12.9 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 11.76 23:44:16.96 +57:55:31.4
114.08939 -3.78879 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 | 23:44:16.96 +57:55:31.4 (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 23:44:16.96 +57:55:31.4: 14.44 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:44:16.96 +57:55:31.4: 14.96 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.44 +/- 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 09 09.2599* 23 44 16.96 +57 55 31.4 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 10.90 23:16:02.19 +52:58:01.9
108.72100 -7.25204 galactic And Second-epoch detections are separated by 1.9" 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 | 23:16:02.19 +52:58:01.9 (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 23:16:02.19 +52:58:01.9: 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 23:16:02.19 +52:58:01.9: 14.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 16 02.19 +52 58 01.9 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 12.64 23:14:32.70 +54:44:09.1
109.16417 -5.52502 galactic Cas Second-epoch detections are separated by 4.3" 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 | 23:14:32.70 +54:44:09.1 (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 23:14:32.70 +54:44:09.1: 14.25 +/- 0.14 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:32.70 +54:44:09.1: 14.63 +/- 0.33 detection
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 09 09.2599* 23 14 32.70 +54 44 09.1 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 13.12 23:42:31.53 +56:49:09.8
113.57055 -4.79460 galactic Cas Second-epoch detections are separated by 8.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J355.6437+56.8162 | 23:42:31.53 +56:49:09.8 (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 23:42:31.53 +56:49:09.8: 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 23:42:31.53 +56:49:09.8: 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 09 09.2599* 23 42 31.53 +56 49 09.8 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.6437+56.8162,2461292.7599,13.12,0.05,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 J355.6437+56.8162 20260909.2599 13.12CV 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 09 09.2599 2461292.7599 13.53 23:21:31.31 +54:25:20.0
110.00252 -6.17671 galactic Cas Second-epoch detections are separated by 6.4" 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 | 23:21:31.31 +54:25:20.0 (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 23:21:31.31 +54:25:20.0: 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 23:21:31.31 +54:25:20.0: 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 09 09.2599* 23 21 31.31 +54 25 20.0 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,2461292.7599,13.53,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.55 23:33:18.72 +56:16:57.8
112.19630 -4.95191 galactic Cas Second-epoch detections are separated by 2.1" 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 | 23:33:18.72 +56:16:57.8 (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 23:33:18.72 +56:16:57.8: 15.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:33:18.72 +56:16:57.8: 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 09 09.2599* 23 33 18.72 +56 16 57.8 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 13.51 23:13:29.33 +56:55:19.7
109.83329 -3.43771 galactic Cas Second-epoch detections are separated by 7.3" 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 | ASASSN-V J231334.09+565524.5 | 23:13:34.09 +56:55:24.5 (Gaia DR3) | SR (local) | 213.000000000000 (local) | Gaia3var=VARIABLE SpType: C 1989Afz....31..507K NikC 4-121
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:13:29.33 +56:55:19.7: 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 23:13:29.33 +56:55:19.7: 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 09 09.2599* 23 13 29.33 +56 55 19.7 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J231334.09+565524.5,2461292.7599,13.51,0.05,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
ASASSN-V J231334.09+565524.5 20260909.2599 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 09 09.2599 2461292.7599 13.67 23:41:06.84 +56:50:15.3
113.38872 -4.72549 galactic Cas Second-epoch detections are separated by 7.2" 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 | 23:41:06.84 +56:50:15.3 (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 23:41:06.84 +56:50:15.3: 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 23:41:06.84 +56:50:15.3: 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 09 09.2599* 23 41 06.84 +56 50 15.3 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,2461292.7599,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 13.72 23:19:18.64 +55:23:09.6
110.03790 -5.16250 galactic Cas Second-epoch detections are separated by 3.6" and 6.9 pix
The object was found in VSX14" ZTF J231917.36+552317.8
Type: EA
# Max. Min./Amp. JD0 Period
17.551 r Y 0.290 r 2458277.93120 0.467449400000
ATTENTION: measured mag 13.72 is 3.5 mag brighter than the VSX record maximum brightness 17.26 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:19:18.64 +55:23:09.6: 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 23:19:18.64 +55:23:09.6: 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 09 09.2599* 23 19 18.64 +55 23 09.6 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
ZTF J231917.36+552317.8,2461292.7599,13.72,0.05,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
ZTF J231917.36+552317.8 20260909.2599 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 09 09.2599 2461292.7599 13.69 23:13:32.44 +55:15:28.7
109.22291 -4.98658 galactic Cas Second-epoch detections are separated by 3.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:13:32.44 +55:15:28.7 (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 23:13:32.44 +55:15:28.7: 15.21 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:13:32.44 +55:15:28.7: 14.73 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.21 +/- 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 09 09.2599* 23 13 32.44 +55 15 28.7 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,13.69,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.77 23:13:03.08 +55:43:03.2
109.32935 -4.53406 galactic Cas Second-epoch detections are separated by 6.5" 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 | 23:13:03.08 +55:43:03.2 (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 23:13:03.08 +55:43:03.2: 15.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:13:03.08 +55:43:03.2: 14.67 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 13 03.08 +55 43 03.2 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,13.77,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 13.88 23:33:01.40 +54:38:42.6
111.66402 -6.50199 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 | 23:33:01.40 +54:38:42.6 (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 23:33:01.40 +54:38:42.6: 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 23:33:01.40 +54:38:42.6: 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 09 09.2599* 23 33 01.40 +54 38 42.6 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,2461292.7599,13.88,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.00 23:53:22.36 +57:55:41.8
115.26403 -4.07641 galactic Cas Second-epoch detections are separated by 5.8" 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 | 23:53:22.36 +57:55:41.8 (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 23:53:22.36 +57:55:41.8: 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 23:53:22.36 +57:55:41.8: 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 09 09.2599* 23 53 22.36 +57 55 41.8 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,2461292.7599,14.00,0.05,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
target 20260909.2599 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 09 09.2599 2461292.7599 13.87 23:18:01.69 +54:03:48.9
109.39552 -6.33492 galactic Cas Second-epoch detections are separated by 5.2" and 7.0 pix
The object was found in VSX 7" ZTF J231801.85+540342.4
Type: RS
# Max. Min./Amp. JD0 Period
17.055 r Y 0.071 r 2458249.95030 0.202432300000
ATTENTION: measured mag 13.87 is 3.1 mag brighter than the VSX record maximum brightness 16.98 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:01.69 +54:03:48.9: 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 23:18:01.69 +54:03:48.9: 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 09 09.2599* 23 18 01.69 +54 03 48.9 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
ZTF J231801.85+540342.4,2461292.7599,13.87,0.05,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
ZTF J231801.85+540342.4 20260909.2599 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 09 09.2599 2461292.7599 14.02 23:12:34.49 +54:39:40.3
108.87077 -5.48896 galactic Cas Second-epoch detections are separated by 0.2" 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 | 23:12:34.49 +54:39:40.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:34.49 +54:39:40.3: 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 23:12:34.49 +54:39:40.3: 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 09 09.2599* 23 12 34.49 +54 39 40.3 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,2461292.7599,14.02,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.03 23:36:43.70 +57:59:50.0
113.14283 -3.44755 galactic Cas Second-epoch detections are separated by 0.6" 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 J354.2016+57.9917 | 23:36:43.70 +57:59:50.0 (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 23:36:43.70 +57:59:50.0: 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 23:36:43.70 +57:59:50.0: 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 09 09.2599* 23 36 43.70 +57 59 50.0 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
ATO J354.2016+57.9917,2461292.7599,14.03,0.05,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 J354.2016+57.9917 20260909.2599 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 09 09.2599 2461292.7599 14.09 23:15:12.47 +52:13:25.3
108.32937 -7.89851 galactic And Second-epoch detections are separated by 5.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.7915+52.2203 | 23:15:12.47 +52:13:25.3 (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 23:15:12.47 +52:13:25.3: 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 23:15:12.47 +52:13:25.3: 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 09 09.2599* 23 15 12.47 +52 13 25.3 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 J348.7915+52.2203,2461292.7599,14.09,0.05,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
ATO J348.7915+52.2203 20260909.2599 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 09 09.2599 2461292.7599 14.04 23:41:09.50 +56:50:24.5
113.39527 -4.72466 galactic Cas Second-epoch detections are separated by 7.5" 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 | 23:41:09.50 +56:50:24.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:41:09.50 +56:50:24.5: 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 23:41:09.50 +56:50:24.5: 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 09 09.2599* 23 41 09.50 +56 50 24.5 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,2461292.7599,14.04,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.03 23:14:50.04 +55:24:50.9
109.45221 -4.90899 galactic Cas Second-epoch detections are separated by 3.7" 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 | 23:14:50.04 +55:24:50.9 (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 23:14:50.04 +55:24:50.9: 15.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:14:50.04 +55:24:50.9: 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 09 09.2599* 23 14 50.04 +55 24 50.9 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,2461292.7599,14.03,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.04 23:20:07.23 +55:43:22.5
110.26340 -4.88652 galactic Cas Second-epoch detections are separated by 7.4" 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 | 23:20:07.23 +55:43:22.5 (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 23:20:07.23 +55:43:22.5: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:20:07.23 +55:43:22.5: 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 09 09.2599* 23 20 07.23 +55 43 22.5 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,2461292.7599,14.04,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.04 23:14:23.65 +52:58:53.0
108.49428 -7.14842 galactic And Second-epoch detections are separated by 7.2" and 7.0 pix
The object was found in VSX11" Gaia DR3 1995343949189563392
Type: E
# Max. Min./Amp. JD0 Period
18.030 G 18.190 G 0.277137000000
ATTENTION: measured mag 14.04 is 4.0 mag brighter than the VSX record maximum brightness 18.03 - 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 23:14:23.65 +52:58:53.0: 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 23:14:23.65 +52:58:53.0: 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 09 09.2599* 23 14 23.65 +52 58 53.0 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 1995343949189563392,2461292.7599,14.04,0.05,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 1995343949189563392 20260909.2599 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 09 09.2599 2461292.7599 14.12 23:21:58.57 +54:52:10.1
110.21813 -5.77876 galactic Cas Second-epoch detections are separated by 4.4" 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 | 23:21:58.57 +54:52:10.1 (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 23:21:58.57 +54:52:10.1: 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 23:21:58.57 +54:52:10.1: 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 09 09.2599* 23 21 58.57 +54 52 10.1 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,2461292.7599,14.12,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.04 23:19:10.89 +54:25:33.4
109.68268 -6.05529 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 | Gaia DR3 1996045441909588608 | 23:19:12.80 +54:26:01.4 (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 23:19:10.89 +54:25:33.4: 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 23:19:10.89 +54:25:33.4: 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 09 09.2599* 23 19 10.89 +54 25 33.4 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
Gaia DR3 1996045441909588608,2461292.7599,14.04,0.05,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 1996045441909588608 20260909.2599 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 09 09.2599 2461292.7599 14.09 23:30:53.67 +55:01:29.5
111.48652 -6.04703 galactic Cas Second-epoch detections are separated by 3.2" 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 J352.7047+55.0257 | 23:30:53.67 +55:01:29.5 (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 23:30:53.67 +55:01:29.5: 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 23:30:53.67 +55:01:29.5: 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 09 09.2599* 23 30 53.67 +55 01 29.5 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 J352.7047+55.0257,2461292.7599,14.09,0.05,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
ATO J352.7047+55.0257 20260909.2599 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 09 09.2599 2461292.7599 14.06 23:19:38.69 +54:49:13.9
109.88455 -5.70907 galactic Cas Second-epoch detections are separated by 5.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J349.9173+54.8237 | 23:19:38.69 +54:49:13.9 (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 23:19:38.69 +54:49:13.9: 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 23:19:38.69 +54:49:13.9: 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 09 09.2599* 23 19 38.69 +54 49 13.9 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 J349.9173+54.8237,2461292.7599,14.06,0.05,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
ATO J349.9173+54.8237 20260909.2599 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 09 09.2599 2461292.7599 14.05 23:27:38.62 +57:03:07.5
111.69175 -3.97972 galactic Cas Second-epoch detections are separated by 7.6" 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 | 23:27:38.62 +57:03:07.5 (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 23:27:38.62 +57:03:07.5: 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 23:27:38.62 +57:03:07.5: 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 09 09.2599* 23 27 38.62 +57 03 07.5 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,2461292.7599,14.05,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.11 23:34:15.18 +54:35:52.2
111.82081 -6.60027 galactic Cas Second-epoch detections are separated by 2.7" and 7.0 pix
The object was found in VSX 9" ZTF J233416.06+543547.9
Type: EW
# Max. Min./Amp. JD0 Period
17.931 r Y 0.128 r 2458472.60670 0.291335600000
ATTENTION: measured mag 14.11 is 3.7 mag brighter than the VSX record maximum brightness 17.80 - 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 23:34:15.18 +54:35:52.2: 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 23:34:15.18 +54:35:52.2: 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 09 09.2599* 23 34 15.18 +54 35 52.2 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
ZTF J233416.06+543547.9,2461292.7599,14.11,0.05,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
ZTF J233416.06+543547.9 20260909.2599 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 09 09.2599 2461292.7599 14.11 23:19:38.83 +54:22:29.4
109.72855 -6.12688 galactic Cas Second-epoch detections are separated by 0.8" 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 | 23:19:38.83 +54:22:29.4 (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 23:19:38.83 +54:22:29.4: 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 23:19:38.83 +54:22:29.4: 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 09 09.2599* 23 19 38.83 +54 22 29.4 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,2461292.7599,14.11,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.20 23:17:54.85 +54:02:55.7
109.37451 -6.34279 galactic Cas Second-epoch detections are separated by 4.0" 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 | ATO J349.4662+54.0392 | 23:17:54.85 +54:02:55.7 (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 23:17:54.85 +54:02:55.7: 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 23:17:54.85 +54:02:55.7: 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 09 09.2599* 23 17 54.85 +54 02 55.7 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 J349.4662+54.0392,2461292.7599,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J349.4662+54.0392 20260909.2599 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 09 09.2599 2461292.7599 14.14 23:10:45.12 +56:08:16.7
109.18836 -4.02348 galactic Cas Second-epoch detections are separated by 7.9" 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 | Gaia DR3 2008861693041687808 | 23:10:49.18 +56:07:59.6 (Gaia DR3) | YSO (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:10:45.12 +56:08:16.7: 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 23:10:45.12 +56:08:16.7: 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 09 09.2599* 23 10 45.12 +56 08 16.7 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
Gaia DR3 2008861693041687808,2461292.7599,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2008861693041687808 20260909.2599 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 09 09.2599 2461292.7599 14.05 23:15:05.48 +52:30:01.7
108.41502 -7.63446 galactic And Second-epoch detections are separated by 1.1" 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 | Gaia DR3 1992269650260416640 | 23:15:07.37 +52:30:45.0 (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 23:15:05.48 +52:30:01.7: 15.11 +/- 0.30 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:05.48 +52:30:01.7: 14.69 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.11 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 15 05.48 +52 30 01.7 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 1992269650260416640,2461292.7599,14.05,0.05,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
Gaia DR3 1992269650260416640 20260909.2599 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 09 09.2599 2461292.7599 14.19 23:14:46.10 +57:01:34.0
110.03399 -3.40504 galactic Cas Second-epoch detections are separated by 2.4" 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 | 23:14:46.10 +57:01:34.0 (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 23:14:46.10 +57:01:34.0: 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 23:14:46.10 +57:01:34.0: 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 09 09.2599* 23 14 46.10 +57 01 34.0 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,2461292.7599,14.19,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.23 23:14:46.63 +52:54:55.4
108.52388 -7.23101 galactic And Second-epoch detections are separated by 6.3" 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 | 23:14:46.63 +52:54:55.4 (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 23:14:46.63 +52:54:55.4: 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 23:14:46.63 +52:54:55.4: 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 09 09.2599* 23 14 46.63 +52 54 55.4 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,2461292.7599,14.23,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.25 23:22:45.33 +52:22:47.1
109.47528 -8.15961 galactic And Second-epoch detections are separated by 1.8" 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 | 23:22:45.33 +52:22:47.1 (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 23:22:45.33 +52:22:47.1: 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 23:22:45.33 +52:22:47.1: 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 09 09.2599* 23 22 45.33 +52 22 47.1 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,2461292.7599,14.25,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.37 23:20:26.01 +52:26:49.9
109.16281 -7.97467 galactic And Second-epoch detections are separated by 7.5" 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 J350.0912+52.4441 | 23:20:26.01 +52:26:49.9 (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 23:20:26.01 +52:26:49.9: 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 23:20:26.01 +52:26:49.9: 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 09 09.2599* 23 20 26.01 +52 26 49.9 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
ATO J350.0912+52.4441,2461292.7599,14.37,0.05,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 J350.0912+52.4441 20260909.2599 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 09 09.2599 2461292.7599 14.22 23:13:36.12 +55:38:46.1
109.37511 -4.62916 galactic Cas Second-epoch detections are separated by 3.1" 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 | ATO J348.4220+55.6507 | 23:13:36.12 +55:38:46.1 (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 23:13:36.12 +55:38:46.1: 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 23:13:36.12 +55:38:46.1: 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 09 09.2599* 23 13 36.12 +55 38 46.1 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 J348.4220+55.6507,2461292.7599,14.22,0.05,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 J348.4220+55.6507 20260909.2599 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 09 09.2599 2461292.7599 14.16 23:26:51.40 +54:14:40.4
110.68094 -6.60301 galactic Cas Second-epoch detections are separated by 4.8" and 7.1 pix
The object was found in VSX21" Gaia DR3 1995851996580563584
Type: ROT
# Max. Min./Amp. JD0 Period
15.360 G 15.400 G M
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 23:26:51.40 +54:14:40.4: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:26:51.40 +54:14:40.4: 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 09 09.2599* 23 26 51.40 +54 14 40.4 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
Gaia DR3 1995851996580563584,2461292.7599,14.16,0.05,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 1995851996580563584 20260909.2599 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 09 09.2599 2461292.7599 14.17 23:15:12.70 +53:15:41.0
108.71278 -6.93297 galactic Cas Second-epoch detections are separated by 7.4" 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 | ATO J348.8014+53.2577 | 23:15:12.70 +53:15:41.0 (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 23:15:12.70 +53:15:41.0: 15.32 +/- 0.31 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:15:12.70 +53:15:41.0: 14.88 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.32 +/- 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 09 09.2599* 23 15 12.70 +53 15 41.0 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 J348.8014+53.2577,2461292.7599,14.17,0.05,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 J348.8014+53.2577 20260909.2599 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 09 09.2599 2461292.7599 14.20 23:15:37.17 +54:22:36.2
109.17815 -5.91624 galactic Cas Second-epoch detections are separated by 8.6" 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 | 23:15:37.17 +54:22:36.2 (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 23:15:37.17 +54:22:36.2: 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 23:15:37.17 +54:22:36.2: 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 09 09.2599* 23 15 37.17 +54 22 36.2 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,2461292.7599,14.20,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.11 23:11:47.56 +55:27:46.1
109.06833 -4.70385 galactic Cas Second-epoch detections are separated by 3.0" 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 | 23:11:47.56 +55:27:46.1 (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 23:11:47.56 +55:27:46.1: 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 23:11:47.56 +55:27:46.1: 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 09 09.2599* 23 11 47.56 +55 27 46.1 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,2461292.7599,14.11,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.16 23:26:53.36 +56:25:56.4
111.39436 -4.53364 galactic Cas Second-epoch detections are separated by 6.2" 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 | 23:26:53.36 +56:25:56.4 (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 23:26:53.36 +56:25:56.4: 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 23:26:53.36 +56:25:56.4: 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 09 09.2599* 23 26 53.36 +56 25 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,2461292.7599,14.16,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.27 23:15:49.23 +52:50:40.9
108.64555 -7.35434 galactic And Second-epoch detections are separated by 1.4" 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 | 23:15:49.23 +52:50:40.9 (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 23:15:49.23 +52:50:40.9: 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 23:15:49.23 +52:50:40.9: 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 09 09.2599* 23 15 49.23 +52 50 40.9 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,14.27,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.28 23:30:06.24 +54:42:16.8
111.27803 -6.31628 galactic Cas Second-epoch detections are separated by 4.0" 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 | 23:30:06.24 +54:42:16.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:30:06.24 +54:42:16.8: 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 23:30:06.24 +54:42:16.8: 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 09 09.2599* 23 30 06.24 +54 42 16.8 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,2461292.7599,14.28,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.17 23:13:04.73 +56:43:23.7
109.70730 -3.60169 galactic Cas Second-epoch detections are separated by 2.5" 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 | 23:13:04.73 +56:43:23.7 (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 23:13:04.73 +56:43:23.7: 15.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:13:04.73 +56:43:23.7: 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 09 09.2599* 23 13 04.73 +56 43 23.7 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,2461292.7599,14.17,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.21 23:15:17.99 +53:29:56.8
108.81255 -6.71647 galactic Cas Second-epoch detections are separated by 4.6" 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 J348.8353+53.4900 | 23:15:17.99 +53:29:56.8 (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 23:15:17.99 +53:29:56.8: 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 23:15:17.99 +53:29:56.8: 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 09 09.2599* 23 15 17.99 +53 29 56.8 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 J348.8353+53.4900,2461292.7599,14.21,0.05,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
ATO J348.8353+53.4900 20260909.2599 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 09 09.2599 2461292.7599 14.26 23:43:25.89 +57:58:09.1
113.99147 -3.71721 galactic Cas Second-epoch detections are separated by 6.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J355.8647+57.9806 | 23:43:25.89 +57:58:09.1 (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 23:43:25.89 +57:58:09.1: 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 23:43:25.89 +57:58:09.1: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 43 25.89 +57 58 09.1 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 J355.8647+57.9806,2461292.7599,14.26,0.05,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 J355.8647+57.9806 20260909.2599 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 09 09.2599 2461292.7599 14.20 23:19:31.01 +53:07:24.0
109.26978 -7.29266 galactic And 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 | 23:19:31.01 +53:07:24.0 (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 23:19:31.01 +53:07:24.0: 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 23:19:31.01 +53:07:24.0: 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 09 09.2599* 23 19 31.01 +53 07 24.0 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,2461292.7599,14.20,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.23 23:12:47.55 +54:41:56.4
108.91427 -5.46564 galactic Cas Second-epoch detections are separated by 6.0" 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 | 23:12:47.55 +54:41:56.4 (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 23:12:47.55 +54:41:56.4: 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 23:12:47.55 +54:41:56.4: 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 09 09.2599* 23 12 47.55 +54 41 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,2461292.7599,14.23,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.31 23:21:29.40 +56:15:30.1
110.62861 -4.44963 galactic Cas Second-epoch detections are separated by 8.5" 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 | ATO J350.3872+56.2529 | 23:21:29.40 +56:15:30.1 (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 23:21:29.40 +56:15:30.1: 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 23:21:29.40 +56:15:30.1: 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 09 09.2599* 23 21 29.40 +56 15 30.1 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 J350.3872+56.2529,2461292.7599,14.31,0.05,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 J350.3872+56.2529 20260909.2599 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 09 09.2599 2461292.7599 14.41 23:18:01.81 +53:42:03.7
109.26624 -6.67396 galactic Cas Second-epoch detections are separated by 3.2" 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 | 23:18:01.81 +53:42:03.7 (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 23:18:01.81 +53:42:03.7: 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 23:18:01.81 +53:42:03.7: 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 09 09.2599* 23 18 01.81 +53 42 03.7 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,2461292.7599,14.41,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.35 23:36:08.16 +54:50:06.8
112.15242 -6.45281 galactic Cas Second-epoch detections are separated by 3.9" 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 | 23:36:08.16 +54:50:06.8 (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 23:36:08.16 +54:50:06.8: 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 23:36:08.16 +54:50:06.8: 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 09 09.2599* 23 36 08.16 +54 50 06.8 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,2461292.7599,14.35,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.41 23:36:58.43 +54:29:57.6
112.17198 -6.80934 galactic Cas Second-epoch detections are separated by 6.0" 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 J354.2442+54.4923 | 23:36:59.46 +54:29:30.2 (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 23:36:58.43 +54:29:57.6: 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 23:36:58.43 +54:29:57.6: 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 09 09.2599* 23 36 58.43 +54 29 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 J354.2442+54.4923,2461292.7599,14.41,0.05,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 J354.2442+54.4923 20260909.2599 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 09 09.2599 2461292.7599 14.39 23:25:04.57 +55:52:06.1
110.97067 -4.98479 galactic Cas Second-epoch detections are separated by 4.6" 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 | 23:25:04.57 +55:52:06.1 (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 23:25:04.57 +55:52:06.1: 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 23:25:04.57 +55:52:06.1: 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 09 09.2599* 23 25 04.57 +55 52 06.1 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,2461292.7599,14.39,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.34 23:15:41.21 +53:21:41.6
108.81614 -6.86557 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 | 23:15:41.21 +53:21:41.6 (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 23:15:41.21 +53:21:41.6: 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 23:15:41.21 +53:21:41.6: 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 09 09.2599* 23 15 41.21 +53 21 41.6 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,2461292.7599,14.34,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.29 23:14:43.64 +54:44:02.1
109.18805 -5.53648 galactic Cas Second-epoch detections are separated by 7.2" 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 | ATO J348.6945+54.7379 | 23:14:43.64 +54:44:02.1 (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 23:14:43.64 +54:44:02.1: 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 23:14:43.64 +54:44:02.1: 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 09 09.2599* 23 14 43.64 +54 44 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
ATO J348.6945+54.7379,2461292.7599,14.29,0.05,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 J348.6945+54.7379 20260909.2599 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 09 09.2599 2461292.7599 14.37 23:16:21.53 +53:04:54.1
108.80833 -7.16286 galactic And Second-epoch detections are separated by 1.9" 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 | 23:16:21.53 +53:04:54.1 (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 23:16:21.53 +53:04:54.1: 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 23:16:21.53 +53:04:54.1: 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 09 09.2599* 23 16 21.53 +53 04 54.1 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,2461292.7599,14.37,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.22 23:31:52.24 +55:24:25.2
111.73740 -5.72588 galactic Cas Second-epoch detections are separated by 6.0" 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 | ATO J352.9568+55.4153 | 23:31:52.24 +55:24:25.2 (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 23:31:52.24 +55:24:25.2: 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 23:31:52.24 +55:24:25.2: 99.00 +/- 99.00 bad_region
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 31 52.24 +55 24 25.2 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
ATO J352.9568+55.4153,2461292.7599,14.22,0.05,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 J352.9568+55.4153 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:42:19.27 +56:52:00.2
113.55610 -4.74155 galactic Cas Second-epoch detections are separated by 4.7" 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 | 23:42:19.27 +56:52:00.2 (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 23:42:19.27 +56:52:00.2: 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 23:42:19.27 +56:52:00.2: 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 09 09.2599* 23 42 19.27 +56 52 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,2461292.7599,14.38,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.41 23:27:13.16 +54:36:25.8
110.84884 -6.27677 galactic Cas Second-epoch detections are separated by 6.0" 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 | 23:27:13.16 +54:36:25.8 (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 23:27:13.16 +54:36:25.8: 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 23:27:13.16 +54:36:25.8: 14.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 27 13.16 +54 36 25.8 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,2461292.7599,14.41,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.30 23:26:12.98 +55:30:59.2
111.00767 -5.36988 galactic Cas Second-epoch detections are separated by 2.8" 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 | 23:26:12.98 +55:30:59.2 (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 23:26:12.98 +55:30:59.2: 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 23:26:12.98 +55:30:59.2: 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 09 09.2599* 23 26 12.98 +55 30 59.2 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,2461292.7599,14.30,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:31:02.76 +54:13:33.3
111.25985 -6.81388 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 | 23:31:02.76 +54:13:33.3 (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 23:31:02.76 +54:13:33.3: 15.30 +/- 0.32 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:02.76 +54:13:33.3: 14.90 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.30 +/- 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 09 09.2599* 23 31 02.76 +54 13 33.3 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,2461292.7599,14.38,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:30:42.74 +54:58:05.5
111.44396 -6.09288 galactic Cas Second-epoch detections are separated by 1.6" and 6.8 pix
The object was found in VSX16" Gaia DR3 1997423817174327808
Type: ROT
# Max. Min./Amp. JD0 Period
15.650 G 15.700 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 23:30:42.74 +54:58:05.5: 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 23:30:42.74 +54:58:05.5: 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 09 09.2599* 23 30 42.74 +54 58 05.5 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 1997423817174327808,2461292.7599,14.38,0.05,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 1997423817174327808 20260909.2599 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 09 09.2599 2461292.7599 14.31 23:17:53.18 +53:53:03.8
109.31184 -6.49502 galactic Cas Second-epoch detections are separated by 6.2" 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 | 23:17:53.18 +53:53:03.8 (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 23:17:53.18 +53:53:03.8: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:53.18 +53:53:03.8: 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 09 09.2599* 23 17 53.18 +53 53 03.8 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,2461292.7599,14.31,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:19:07.36 +55:41:18.2
110.11910 -4.86992 galactic Cas Second-epoch detections are separated by 5.8" 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 | 23:19:07.36 +55:41:18.2 (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 23:19:07.36 +55:41:18.2: 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 23:19:07.36 +55:41:18.2: 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 09 09.2599* 23 19 07.36 +55 41 18.2 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,2461292.7599,14.38,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.32 23:31:38.06 +54:52:04.7
111.53981 -6.22895 galactic Cas Second-epoch detections are separated by 5.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J352.9078+54.8743 | 23:31:38.06 +54:52:04.7 (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 23:31:38.06 +54:52:04.7: 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 23:31:38.06 +54:52:04.7: 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 09 09.2599* 23 31 38.06 +54 52 04.7 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
ATO J352.9078+54.8743,2461292.7599,14.32,0.05,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
ATO J352.9078+54.8743 20260909.2599 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 09 09.2599 2461292.7599 14.37 23:24:23.81 +56:17:15.3
111.01965 -4.55777 galactic Cas Second-epoch detections are separated by 3.8" 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 | target | 23:24:23.81 +56:17:15.3 (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 23:24:23.81 +56:17:15.3: 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 23:24:23.81 +56:17:15.3: 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 09 09.2599* 23 24 23.81 +56 17 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,2461292.7599,14.37,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.38 23:17:35.25 +54:40:53.9
109.55617 -5.73443 galactic Cas Second-epoch detections are separated by 5.7" 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 | 23:17:35.25 +54:40:53.9 (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 23:17:35.25 +54:40:53.9: 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 23:17:35.25 +54:40:53.9: 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 09 09.2599* 23 17 35.25 +54 40 53.9 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,2461292.7599,14.38,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.32 23:22:05.30 +52:39:33.0
109.47495 -7.86233 galactic And Second-epoch detections are separated by 1.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:22:05.30 +52:39:33.0 (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 23:22:05.30 +52:39:33.0: 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 23:22:05.30 +52:39:33.0: 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 09 09.2599* 23 22 05.30 +52 39 33.0 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,2461292.7599,14.32,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.32 23:26:37.11 +55:28:49.0
111.05001 -5.42255 galactic Cas Second-epoch detections are separated by 0.5" 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 | target | 23:26:37.11 +55:28:49.0 (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 23:26:37.11 +55:28:49.0: 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 23:26:37.11 +55:28:49.0: 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 09 09.2599* 23 26 37.11 +55 28 49.0 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,2461292.7599,14.32,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.36 23:27:34.12 +54:33:50.7
110.88315 -6.33382 galactic Cas Second-epoch detections are separated by 5.9" 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 | 23:27:34.12 +54:33:50.7 (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 23:27:34.12 +54:33:50.7: 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 23:27:34.12 +54:33:50.7: 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 09 09.2599* 23 27 34.12 +54 33 50.7 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,2461292.7599,14.36,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.46 23:15:17.13 +54:04:35.0
109.02251 -6.17821 galactic Cas Second-epoch detections are separated by 3.1" 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 | 23:15:17.13 +54:04:35.0 (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 23:15:17.13 +54:04:35.0: 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 23:15:17.13 +54:04:35.0: 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 09 09.2599* 23 15 17.13 +54 04 35.0 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,2461292.7599,14.46,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.32 23:17:56.25 +55:25:42.4
109.86975 -5.05416 galactic Cas Second-epoch detections are separated by 4.9" 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 | 23:17:56.25 +55:25:42.4 (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 23:17:56.25 +55:25:42.4: 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 23:17:56.25 +55:25:42.4: 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 09 09.2599* 23 17 56.25 +55 25 42.4 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,2461292.7599,14.32,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.22 23:24:51.30 +56:17:42.2
111.08232 -4.57170 galactic Cas Second-epoch detections are separated by 6.3" 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 | 23:24:51.30 +56:17:42.2 (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 23:24:51.30 +56:17:42.2: 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 23:24:51.30 +56:17:42.2: 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 09 09.2599* 23 24 51.30 +56 17 42.2 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,2461292.7599,14.22,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.37 23:35:23.98 +56:20:57.3
112.49363 -4.97368 galactic Cas Second-epoch detections are separated by 7.4" 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 | 23:35:23.98 +56:20:57.3 (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 23:35:23.98 +56:20:57.3: 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 23:35:23.98 +56:20:57.3: 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 09 09.2599* 23 35 23.98 +56 20 57.3 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,2461292.7599,14.37,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.39 23:43:35.21 +57:49:28.1
113.97365 -3.86232 galactic Cas Second-epoch detections are separated by 3.9" 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 | 23:43:35.21 +57:49:28.1 (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 23:43:35.21 +57:49:28.1: 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 23:43:35.21 +57:49:28.1: 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 09 09.2599* 23 43 35.21 +57 49 28.1 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,2461292.7599,14.39,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.46 23:45:32.20 +57:23:44.0
114.11629 -4.34388 galactic Cas Second-epoch detections are separated by 3.5" 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 | 23:45:32.20 +57:23:44.0 (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 23:45:32.20 +57:23:44.0: 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 23:45:32.20 +57:23:44.0: 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 09 09.2599* 23 45 32.20 +57 23 44.0 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,2461292.7599,14.46,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.49 23:44:20.54 +56:48:40.2
113.80923 -4.86746 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 | ATO J356.0755+56.8200 | 23:44:20.54 +56:48:40.2 (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 23:44:20.54 +56:48:40.2: 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 23:44:20.54 +56:48:40.2: 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 09 09.2599* 23 44 20.54 +56 48 40.2 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
ATO J356.0755+56.8200,2461292.7599,14.49,0.05,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 J356.0755+56.8200 20260909.2599 14.49CV 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 09 09.2599 2461292.7599 14.37 23:20:38.48 +52:15:03.9
109.12409 -8.16959 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 | ATO J350.1425+52.2485 | 23:20:38.48 +52:15:03.9 (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 23:20:38.48 +52:15:03.9: 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 23:20:38.48 +52:15:03.9: 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 09 09.2599* 23 20 38.48 +52 15 03.9 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
ATO J350.1425+52.2485,2461292.7599,14.37,0.05,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 J350.1425+52.2485 20260909.2599 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 09 09.2599 2461292.7599 14.46 23:36:00.61 +54:33:04.0
112.05216 -6.71951 galactic Cas Second-epoch detections are separated by 1.7" 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 | 23:36:00.61 +54:33:04.0 (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 23:36:00.61 +54:33:04.0: 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 23:36:00.61 +54:33:04.0: 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 09 09.2599* 23 36 00.61 +54 33 04.0 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,2461292.7599,14.46,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.33 23:27:08.57 +57:56:28.7
111.91273 -3.11566 galactic Cas Second-epoch detections are separated by 2.0" 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 | 23:27:08.57 +57:56:28.7 (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 23:27:08.57 +57:56:28.7: 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 23:27:08.57 +57:56:28.7: 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 09 09.2599* 23 27 08.57 +57 56 28.7 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,2461292.7599,14.33,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.26 23:19:16.70 +55:34:13.3
110.09830 -4.98818 galactic Cas Second-epoch detections are separated by 5.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 23:19:16.70 +55:34:13.3 (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 23:19:16.70 +55:34:13.3: 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 23:19:16.70 +55:34:13.3: 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 09 09.2599* 23 19 16.70 +55 34 13.3 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,2461292.7599,14.26,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.46 23:30:06.03 +54:28:15.6
111.20436 -6.53818 galactic Cas Second-epoch detections are separated by 6.5" 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 J352.5251+54.4628 | 23:30:06.03 +54:28:15.6 (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 23:30:06.03 +54:28:15.6: 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 23:30:06.03 +54:28:15.6: 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 09 09.2599* 23 30 06.03 +54 28 15.6 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
ATO J352.5251+54.4628,2461292.7599,14.46,0.05,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 J352.5251+54.4628 20260909.2599 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 09 09.2599 2461292.7599 14.43 23:15:12.87 +54:11:50.9
109.05719 -6.06167 galactic Cas Second-epoch detections are separated by 3.4" and 7.0 pix
The object was found in VSX18" ZTF J231513.70+541206.9
Type: EW
# Max. Min./Amp. JD0 Period
18.151 r Y 0.254 r 2458258.95230 0.417192200000
ATTENTION: measured mag 14.43 is 3.5 mag brighter than the VSX record maximum brightness 17.90 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:15:12.87 +54:11:50.9: 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 23:15:12.87 +54:11:50.9: 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 09 09.2599* 23 15 12.87 +54 11 50.9 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
ZTF J231513.70+541206.9,2461292.7599,14.43,0.05,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
ZTF J231513.70+541206.9 20260909.2599 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 09 09.2599 2461292.7599 14.40 23:17:55.05 +54:18:14.4
109.46617 -6.10442 galactic Cas Second-epoch detections are separated by 5.2" 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 | 23:17:55.05 +54:18:14.4 (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 23:17:55.05 +54:18:14.4: 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 23:17:55.05 +54:18:14.4: 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 09 09.2599* 23 17 55.05 +54 18 14.4 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,2461292.7599,14.40,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.47 23:13:56.50 +55:25:37.8
109.33881 -4.85040 galactic Cas Second-epoch detections are separated by 1.3" and 7.0 pix
The object was found in VSX12" ZTF J231357.37+552528.5
Type: EA
# Max. Min./Amp. JD0 Period
18.482 r Y 0.466 r 2458244.98400 0.644970000000
ATTENTION: measured mag 14.47 is 3.5 mag brighter than the VSX record maximum brightness 18.02 - 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 23:13:56.50 +55:25:37.8: 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 23:13:56.50 +55:25:37.8: 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 09 09.2599* 23 13 56.50 +55 25 37.8 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
ZTF J231357.37+552528.5,2461292.7599,14.47,0.05,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
ZTF J231357.37+552528.5 20260909.2599 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 09 09.2599 2461292.7599 14.50 23:30:17.98 +54:25:55.5
111.21988 -6.58417 galactic Cas Second-epoch detections are separated by 7.0" 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 | 23:30:17.98 +54:25:55.5 (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 23:30:17.98 +54:25:55.5: 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 23:30:17.98 +54:25:55.5: 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 09 09.2599* 23 30 17.98 +54 25 55.5 14.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,14.50,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.39 23:12:34.34 +54:40:14.3
108.87398 -5.48007 galactic Cas Second-epoch detections are separated by 0.8" 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 | target | 23:12:34.34 +54:40:14.3 (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 23:12:34.34 +54:40:14.3: 15.30 +/- 0.34 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:12:34.34 +54:40:14.3: 14.81 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.30 +/- 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 09 09.2599* 23 12 34.34 +54 40 14.3 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,2461292.7599,14.39,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.47 23:21:26.77 +51:25:56.2
108.95565 -8.98086 galactic And Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J350.3596+51.4281 | 23:21:26.77 +51:25:56.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:26.77 +51:25:56.2: 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 23:21:26.77 +51:25:56.2: 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 09 09.2599* 23 21 26.77 +51 25 56.2 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
ATO J350.3596+51.4281,2461292.7599,14.47,0.05,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
ATO J350.3596+51.4281 20260909.2599 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 09 09.2599 2461292.7599 14.30 23:19:56.24 +54:56:35.5
109.96709 -5.60873 galactic Cas Second-epoch detections are separated by 3.8" 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 | 23:19:56.24 +54:56:35.5 (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 23:19:56.24 +54:56:35.5: 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 23:19:56.24 +54:56:35.5: 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 09 09.2599* 23 19 56.24 +54 56 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,2461292.7599,14.30,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.52 23:15:39.76 +54:30:28.8
109.23195 -5.79620 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 | 23:15:39.76 +54:30:28.8 (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 23:15:39.76 +54:30:28.8: 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 23:15:39.76 +54:30:28.8: 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 09 09.2599* 23 15 39.76 +54 30 28.8 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,2461292.7599,14.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 14.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 14.24 23:15:58.54 +54:10:16.7
109.15195 -6.12653 galactic Cas Second-epoch detections are separated by 3.0" 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 | 23:15:58.54 +54:10:16.7 (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 23:15:58.54 +54:10:16.7: 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 23:15:58.54 +54:10:16.7: 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 09 09.2599* 23 15 58.54 +54 10 16.7 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,2461292.7599,14.24,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.52 23:15:53.87 +57:02:25.2
110.18259 -3.44757 galactic Cas Second-epoch detections are separated by 2.4" 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 | Gaia DR3 2009297542017190016 | 23:15:52.86 +57:03:05.8 (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 23:15:53.87 +57:02:25.2: 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 23:15:53.87 +57:02:25.2: 14.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 09.2599* 23 15 53.87 +57 02 25.2 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 2009297542017190016,2461292.7599,14.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2009297542017190016 20260909.2599 14.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 14.35 23:29:11.22 +55:12:46.5
111.31211 -5.79236 galactic Cas Second-epoch detections are separated by 2.2" 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 | 23:29:11.22 +55:12:46.5 (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 23:29:11.22 +55:12:46.5: 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 23:29:11.22 +55:12:46.5: 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 09 09.2599* 23 29 11.22 +55 12 46.5 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,2461292.7599,14.35,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.30 23:15:49.17 +54:42:21.6
109.32540 -5.61992 galactic Cas Second-epoch detections are separated by 4.3" and 7.3 pix
The object was found in VSX18" Gaia DR3 1996804517247346304
Type: RS
# Max. Min./Amp. JD0 Period
17.000 G 17.110 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 23:15:49.17 +54:42:21.6: 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 23:15:49.17 +54:42:21.6: 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 09 09.2599* 23 15 49.17 +54 42 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
Gaia DR3 1996804517247346304,2461292.7599,14.30,0.05,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 1996804517247346304 20260909.2599 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 09 09.2599 2461292.7599 14.35 23:17:45.41 +56:54:51.5
110.37438 -3.65586 galactic Cas Second-epoch detections are separated by 1.7" 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 | ATO J349.4596+56.9121 | 23:17:45.41 +56:54:51.5 (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 23:17:45.41 +56:54:51.5: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:17:45.41 +56:54:51.5: 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 09 09.2599* 23 17 45.41 +56 54 51.5 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
ATO J349.4596+56.9121,2461292.7599,14.35,0.05,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
ATO J349.4596+56.9121 20260909.2599 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 09 09.2599 2461292.7599 14.30 23:19:25.33 +55:38:48.2
110.14419 -4.92372 galactic Cas Second-epoch detections are separated by 5.5" and 7.1 pix
The object was found in VSX14" Gaia DR3 1996920137769170432
Type: ROT
# Max. Min./Amp. JD0 Period
15.800 G 15.840 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 23:19:25.33 +55:38:48.2: 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 23:19:25.33 +55:38:48.2: 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 09 09.2599* 23 19 25.33 +55 38 48.2 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 1996920137769170432,2461292.7599,14.30,0.05,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 1996920137769170432 20260909.2599 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 09 09.2599 2461292.7599 14.47 23:15:35.46 +52:09:47.5
108.36222 -7.97629 galactic And Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J348.8805+52.1649 | 23:15:35.46 +52:09:47.5 (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 23:15:35.46 +52:09:47.5: 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 23:15:35.46 +52:09:47.5: 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 09 09.2599* 23 15 35.46 +52 09 47.5 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
ATO J348.8805+52.1649,2461292.7599,14.47,0.05,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
ATO J348.8805+52.1649 20260909.2599 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 09 09.2599 2461292.7599 14.52 23:14:31.80 +53:50:27.8
108.83181 -6.35653 galactic Cas Second-epoch detections are separated by 5.5" 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 | target | 23:14:31.80 +53:50:27.8 (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 23:14:31.80 +53:50:27.8: 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 23:14:31.80 +53:50:27.8: 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 09 09.2599* 23 14 31.80 +53 50 27.8 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,2461292.7599,14.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 14.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.2599 2461292.7599 14.32 23:27:37.01 +56:15:56.3
111.43651 -4.72385 galactic Cas Second-epoch detections are separated by 8.0" 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 | 23:27:37.01 +56:15:56.3 (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 23:27:37.01 +56:15:56.3: 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 23:27:37.01 +56:15:56.3: 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 09 09.2599* 23 27 37.01 +56 15 56.3 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,2461292.7599,14.32,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.44 23:18:41.56 +54:46:21.0
109.73847 -5.70596 galactic Cas Second-epoch detections are separated by 3.6" 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 | 23:18:41.56 +54:46:21.0 (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 23:18:41.56 +54:46:21.0: 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 23:18:41.56 +54:46:21.0: 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 09 09.2599* 23 18 41.56 +54 46 21.0 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,2461292.7599,14.44,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.46 23:22:21.61 +56:29:36.7
110.82238 -4.26939 galactic Cas Second-epoch detections are separated by 8.3" 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 | 23:22:21.61 +56:29:36.7 (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 23:22:21.61 +56:29:36.7: 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 23:22:21.61 +56:29:36.7: 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 09 09.2599* 23 22 21.61 +56 29 36.7 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,2461292.7599,14.46,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.50 23:12:59.22 +55:34:38.1
109.26857 -4.66094 galactic Cas Second-epoch detections are separated by 3.4" 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 | 23:12:59.22 +55:34:38.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=1.279+/- (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:12:59.22 +55:34:38.1: 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 23:12:59.22 +55:34:38.1: 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 09 09.2599* 23 12 59.22 +55 34 38.1 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
target,2461292.7599,14.50,0.05,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 20260909.2599 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 09 09.2599 2461292.7599 14.29 23:12:18.99 +55:16:00.9
109.06379 -4.91336 galactic Cas Second-epoch detections are separated by 5.7" and 7.0 pix
The object was found in VSX23" Gaia DR3 1996708958516347776
Type:
# Max. Min./Amp. JD0 Period
17.340 G 18.100 G
ATTENTION: measured mag 14.29 is 3.1 mag brighter than the VSX record maximum brightness 17.34 - 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 23:12:18.99 +55:16:00.9: 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 23:12:18.99 +55:16:00.9: 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 09 09.2599* 23 12 18.99 +55 16 00.9 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 1996708958516347776,2461292.7599,14.29,0.05,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 1996708958516347776 20260909.2599 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 09 09.2599 2461292.7599 12.41 23:33:57.82 +55:18:00.7
111.99032 -5.91715 galactic Cas Second-epoch detections are separated by 2.8" 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 | 23:33:57.82 +55:18:00.7 (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 23:33:57.82 +55:18:00.7: 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 23:33:57.82 +55:18:00.7: 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 09 09.2599* 23 33 57.82 +55 18 00.7 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461292.7599,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260909.2599 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461292.76022664 09.09.2026 06:14:33.582 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 123
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: 15 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): 25803
Objects passed selection criteria: 25790
Measurements per detected object (mean, median, min, max): 3.3 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 3.0 2 4
Average stars detected per image: 22512.5
Average stars matched: 21713.5 (96.4509 %)
Memory usage VmPeak: 253484 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Sep 9 01:34:37 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: 2461292.76022664 09.09.2026 06:14:33.582 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2409
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: 390 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): 177336
Objects passed selection criteria: 176971
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 157962
Average stars matched: 139929 (88.5841 %)
Memory usage VmPeak: 583716 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Sep 9 01:45:30 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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.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: 2461292.75967416
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_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.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_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
Image size: 941.3'x623.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.85"/pix along the Y axis
Image center: 00:00:00.385 +53:59:56.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.062 +54:00:02.05
Second-epoch image center 00:00:00.385 +53:59:56.89
Angular distance between the image centers 0.0022 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
Image size: 941.3'x622.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.85"/pix along the Y axis
Image center: 00:00:00.629 +54:00:38.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.062 +54:00:02.05
Second-epoch image center 00:00:00.629 +54:00:38.07
Angular distance between the image centers 0.0101 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:00.385 +53:59:56.89
Second-epoch second image center 00:00:00.629 +54:00:38.07
Angular distance between the image centers 0.01145 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.OOmjJUAlHg
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.Cq9W2UH3VI
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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits &> /tmp/tmp.ZCxfpnOgtW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits &> /tmp/tmp.LRIW5EEW69
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.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 99 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
2.2 pix fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
2.2 pix fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.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
15.1 mag. fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
15.1 mag. fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
cp: cannot create regular file 'local_wcs_cache/': Not a directory
All-image limiting magnitude estimate: 15.1 (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
############ /tmp/tmp.OOmjJUAlHg (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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/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.Cq9W2UH3VI (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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/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.ZCxfpnOgtW (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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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=3476, bad_region=7300, passed=33051
Got 33051 stars (including 22801 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat
util/solve_plate_with_UCAC5 got 33051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0969 through 0 to 14.9116, gap 14.9116 to 345.0969
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 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 4452 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3828 matched stars entering correct_measured_positions(), 3954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.13"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3751 matched stars entering correct_measured_positions(), 27243 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.80"
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 345.0858 through 0 to 14.9161, gap 14.9161 to 345.0858
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 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 4580 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4028 matched stars entering correct_measured_positions(), 27243 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.67"
Accuracy estimation diagnostic: 4002 matched stars entering correct_measured_positions(), 27240 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.38"
Excluding outliers - 4002 stars left (next iteration limit 4126)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4002 robust_rms=4.937 arcsec worst_quadrant_rms=99.540 arcsec
SIP_REFIT: SIP order 3 trial: matched=4002 robust_rms=0.524 arcsec worst_quadrant_rms=73.796 arcsec
SIP_REFIT: SIP order 5 trial: matched=4002 robust_rms=0.448 arcsec worst_quadrant_rms=66.468 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4002 robust_rms_before=26.156 arcsec robust_rms_before_corrected=2.228 arcsec robust_rms_after=0.448 arcsec worst_quadrant_rms_before=19.023 worst_quadrant_rms_after=66.468
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 19.023 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits N_match=4002 sigma_overall_arcsec=2.041 sigma_q1_arcsec=1.641 sigma_q2_arcsec=1.236 sigma_q3_arcsec=11.077 sigma_q4_arcsec=1.117 n_q1=1355 n_q2=840 n_q3=845 n_q4=962 worst_quadrant_to_overall_ratio=5.426
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits -region wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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.LRIW5EEW69 (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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3431, bad_region=7295, passed=33040
Got 33040 stars (including 22839 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat
util/solve_plate_with_UCAC5 got 33040 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0973 through 0 to 14.9904, gap 14.9904 to 345.0973
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 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4437 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3799 matched stars entering correct_measured_positions(), 3930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.16"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3731 matched stars entering correct_measured_positions(), 27245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.84"
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 345.0867 through 0 to 14.9947, gap 14.9947 to 345.0867
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 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4542 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4036 matched stars entering correct_measured_positions(), 27245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.71"
Accuracy estimation diagnostic: 4017 matched stars entering correct_measured_positions(), 27243 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.43"
Excluding outliers - 4017 stars left (next iteration limit 4104)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4017 robust_rms=5.044 arcsec worst_quadrant_rms=105.305 arcsec
SIP_REFIT: SIP order 3 trial: matched=4017 robust_rms=0.517 arcsec worst_quadrant_rms=76.636 arcsec
SIP_REFIT: SIP order 5 trial: matched=4017 robust_rms=0.453 arcsec worst_quadrant_rms=70.351 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4017 robust_rms_before=25.973 arcsec robust_rms_before_corrected=2.042 arcsec robust_rms_after=0.453 arcsec worst_quadrant_rms_before=19.425 worst_quadrant_rms_after=70.351
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 19.425 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits N_match=4017 sigma_overall_arcsec=1.955 sigma_q1_arcsec=1.531 sigma_q2_arcsec=1.185 sigma_q3_arcsec=12.126 sigma_q4_arcsec=1.149 n_q1=1341 n_q2=849 n_q3=870 n_q4=957 worst_quadrant_to_overall_ratio=6.202
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits -region wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits'
Saving the final (post-refit) wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.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_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits sigma_overall=2.041 worst_q_ratio=5.426
new2=fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits sigma_overall=1.955 worst_q_ratio=6.202
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_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits) flagged: sigma=2.041 (ref avg 0.463), ratio=5.426 (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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/lib/make_outxyls_for_astrometric_calibration found 31962 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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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: "out1059099.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1059099.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 22.5308 (6.09549e+09), 7 match, 0 conflict, 20 distractors, 26 index.
RA,Dec = (359.987,54.0136), pixel scale 5.93008 arcsec/pix.
Hit/miss: Hit/miss: ----+--+---+--+-+---+-----+(best)-----+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1059099.solved to indicate this.
Field: out1059099.xyls
Field center: (RA,Dec) = (359.987914, 54.014453) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:57.099, +54:00:52.030).
Field size: 15.6029 x 10.4303 degrees
Field rotation angle: up is 4.37603 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits' -> 'fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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 Sep 9 01:37 fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
-rw-r--r-- 1 apache apache 8.5K Sep 9 01:37 out1059099.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits (fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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: "out1059099.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1059099.axy"...
Only searching for solutions within 15.4417 degrees of RA,Dec (359.989,54.0153)
log-odds ratio 22.5308 (6.09549e+09), 7 match, 0 conflict, 20 distractors, 26 index.
RA,Dec = (359.987,54.0136), pixel scale 5.93008 arcsec/pix.
Hit/miss: Hit/miss: ----+--+---+--+-+---+-----+(best)-----+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1059099.solved to indicate this.
Field: out1059099.xyls
Field center: (RA,Dec) = (359.987914, 54.014453) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:57.099, +54:00:52.030).
Field size: 15.6029 x 10.4303 degrees
Field rotation angle: up is 4.37603 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 Sep 9 01:37 fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
-rw-r--r-- 1 apache apache 8.5K Sep 9 01:37 out1059099.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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
WARNING: the local solve-field solution for fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits carries no SIP distortion terms while --tweak-order 2 was requested: the tweak silently failed on a marginal quad match and the TAN-only solution is unreliable away from the matched quad. Discarding it and retrying with a remote plate-solve server.
Local astrometry not available or failed, trying remote servers...
Setting up remote astrometry servers...
Checking if we can reach any plate solve servers... tau.kirx.net scan.sai.msu.ru scan.sai.msu.ru
The reachable servers are:
scan.sai.msu.ru
Updated list of available servers: scan.sai.msu.ru
We choose the plate solve server scan.sai.msu.ru
Using the remote server with Astrometry.net code
Plate solve server: scan.sai.msu.ru
Submitting the plates solving job to the server [01;34m scan.sai.msu.ru [00m
This may take [01;31mup to a few minutes[00m...
Plate solving parameters: -F fov=605 -F width=9576 -F hight=6388 http://scan.sai.msu.ru/cgi-bin/process_file/process_sextractor_list.py
% Total % Received % Xferd Average Speed Time Time Time Current
Dload Upload Total Spent Left Speed
0 0 0 0 0 0 0 0 0
100 124.3k 0 0 100 124.3k 0 91808 00:01 00:01 91823
100 124.3k 0 0 100 124.3k 0 42409 00:03 00:03 42412
100 124.3k 0 0 100 124.3k 0 31805 00:04 00:04 31807
100 124.3k 0 0 100 124.3k 0 25444 00:05 00:05 25445
100 124.3k 0 0 100 124.3k 0 21203 00:06 00:06 21204
100 124.3k 0 0 100 124.3k 0 18175 00:07 00:07 0
100 124.3k 0 0 100 124.3k 0 15903 00:08 00:08 0
100 124.3k 0 0 100 124.3k 0 14135 00:09 00:09 0
100 124.3k 0 0 100 124.3k 0 12722 00:10 00:10 0
100 128.8k 0 4579 100 124.3k 455 12657 00:10 00:10 905
100 128.8k 0 4579 100 124.3k 455 12656 00:10 00:10 905
100 128.8k 0 4579 100 124.3k 455 12656 00:10 00:10 905
'out1059099.xyls' -> 'test.xyls'
#### Plate solution log ####
% Total % Received % Xferd Average Speed Time Time Time Current
Dload Upload Total Spent Left Speed
0 0 0 0 0 0 0 0 0
35 3436 35 1204 0 0 1180 0 00:02 00:01 00:01 1180
100 3436 100 3436 0 0 3367 0 00:01 00:01 1180
100 3436 100 3436 0 0 3366 0 00:01 00:01 1180
100 3436 100 3436 0 0 3366 0 00:01 00:01 1180
-rw-r--r-- 1 apache apache 124K Sep 9 06:37 files/4040aWfiPBua/out1059099.xyls
export PATH=/var/www/cgi-venv/bin/:/var/www/scan.sai.msu.ru/venv_astrometrynet/bin/:/usr/local/astrometry/bin/:/bin:/sbin:/bin:/sbin:/usr/bin:/usr/sbin:/usr/bin:/usr/sbin:/usr/local/bin:/usr/local/sbin:/opt/bin:/usr/lib/llvm/19/bin:/usr/lib/llvm/18/bin:/usr/bin/cdsclient; cd files/4040aWfiPBua/ ; timeout 4m solve-field --crpix-center --uniformize 0 --objs 1000 --depth 10,20,30-50 --no-plots --x-column X_IMAGE --y-column Y_IMAGE --sort-column FLUX_APER --width 9576.0 --height 6388.0 --scale-units arcminwidth --scale-low 544.5 --scale-high 3025.0 out1059099.xyls &>> program.log
Reading input file 1 of 1: "out1059099.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1059099.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 22.5308 (6.09549e+09), 7 match, 0 conflict, 20 distractors, 26 index.
RA,Dec = (359.987,54.0136), pixel scale 5.93008 arcsec/pix.
Hit/miss: Hit/miss: ----+--+---+--+-+---+-----+(best)-----+-------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1059099.solved to indicate this.
Field: out1059099.xyls
Field center: (RA,Dec) = (359.987914, 54.014453) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:57.099, +54:00:52.030).
Field size: 15.6029 x 10.4303 degrees
Field rotation angle: up is 4.37603 degrees E of N
Field parity: neg
export PATH=/var/www/cgi-venv/bin/:/var/www/scan.sai.msu.ru/venv_astrometrynet/bin/:/usr/local/astrometry/bin/:/bin:/sbin:/bin:/sbin:/usr/bin:/usr/sbin:/usr/bin:/usr/sbin:/usr/local/bin:/usr/local/sbin:/opt/bin:/usr/lib/llvm/19/bin:/usr/lib/llvm/18/bin:/usr/bin/cdsclient; cd files/4040aWfiPBua/ ; timeout 50 solve-field --overwrite --crpix-center --uniformize 0 --objs 10000 --depth 100 --tweak-order 3 --no-plots --x-column X_IMAGE --y-column Y_IMAGE --sort-column FLUX_APER --width 9576.0 --height 6388.0 --scale-units arcsecperpix --scale-low 5.6336 --scale-high 6.2266 --ra 359.987914 --dec 54.014453 --radius 5 out1059099.xyls &>> program.log
Reading input file 1 of 1: "out1059099.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1059099.axy"...
Only searching for solutions within 5 degrees of RA,Dec (359.988,54.0145)
Field 1 did not solve (index index-4118.fits, field objects 1-100).
Field 1 did not solve (index index-4117.fits, field objects 1-100).
log-odds ratio 50.9357 (1.32163e+22), 9 match, 0 conflict, 21 distractors, 26 index.
RA,Dec = (359.999,53.9975), pixel scale 5.95278 arcsec/pix.
Hit/miss: Hit/miss: +++-------+------+-++-----+--+(best)----------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1059099.solved to indicate this.
Field: out1059099.xyls
Field center: (RA,Dec) = (0.000200, 53.998310) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:00.048, +53:59:53.915).
Field size: 15.7165 x 10.5217 degrees
Field rotation angle: up is 2.23307 degrees E of N
Field parity: neg
############################
Field [01;32mSOLVED[00m =)
Downloading WCS header... done
'/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits' -> 'fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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 Sep 9 01:37 fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
-rw-r--r-- 1 apache apache 8.5K Sep 9 01:37 out1059099.wcs
Inserting WCS header in fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits (remote) ... Opening FITS image file fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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 = 'remote ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'scan.sai.msu.ru' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Sending request to remove job 4040aWfiPBua from the server...
% Total % Received % Xferd Average Speed Time Time Time Current
Dload Upload Total Spent Left Speed
0 0 0 0 0 0 0 0 0
100 324 0 27 100 297 54 596 0
100 324 0 27 100 297 54 596 0
100 324 0 27 100 297 54 596 0
Job 4040aWfiPBua removed.
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat from image00003.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
Image size: 941.3'x623.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.85"/pix along the Y axis
Image center: 00:00:00.385 +53:59:56.89 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 33051 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/correct_sextractor_wcs_catalog_usingxy2sky1108293.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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=3476, bad_region=7300, passed=33051
Got 33051 stars (including 22801 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat
util/solve_plate_with_UCAC5 got 33051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0969 through 0 to 14.9116, gap 14.9116 to 345.0969
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 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 4452 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3828 matched stars entering correct_measured_positions(), 3954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.13"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3751 matched stars entering correct_measured_positions(), 27243 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.80"
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 345.0858 through 0 to 14.9161, gap 14.9161 to 345.0858
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 48.1 to 59.2)
Done reading UCAC5 zone files...
Matched 4580 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4028 matched stars entering correct_measured_positions(), 27243 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.67"
Accuracy estimation diagnostic: 4002 matched stars entering correct_measured_positions(), 27240 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.38"
Excluding outliers - 4002 stars left (next iteration limit 4126)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4002 robust_rms=4.937 arcsec worst_quadrant_rms=99.540 arcsec
SIP_REFIT: SIP order 3 trial: matched=4002 robust_rms=0.524 arcsec worst_quadrant_rms=73.796 arcsec
SIP_REFIT: SIP order 5 trial: matched=4002 robust_rms=0.448 arcsec worst_quadrant_rms=66.468 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4002 robust_rms_before=26.156 arcsec robust_rms_before_corrected=2.228 arcsec robust_rms_after=0.448 arcsec worst_quadrant_rms_before=19.023 worst_quadrant_rms_after=66.468
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 19.023 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits N_match=4002 sigma_overall_arcsec=2.041 sigma_q1_arcsec=1.641 sigma_q2_arcsec=1.236 sigma_q3_arcsec=11.077 sigma_q4_arcsec=1.117 n_q1=1355 n_q2=840 n_q3=845 n_q4=962 worst_quadrant_to_overall_ratio=5.426
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits -region wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.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: the retry reproduced the identical solution for 1st new image (fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits) - the plate solve is deterministic for this image and the tweak order is not the problem (suspect a marginal quad match; see the silently-failed-tweak guard in util/wcs_image_calibration.sh)
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits): sigma 2.041->2.041, ratio 5.426->5.426; reverting to order 3
WCS_QUALITY_RETRY: 2nd new image (fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits) flagged: sigma=1.955 (ref avg 0.463), ratio=6.202 (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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/lib/make_outxyls_for_astrometric_calibration found 31924 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_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out1108578.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1108578.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 22.4684 (5.72642e+09), 7 match, 0 conflict, 20 distractors, 26 index.
RA,Dec = (359.987,54.0249), pixel scale 5.93017 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 ./out1108578.solved to indicate this.
Field: out1108578.xyls
Field center: (RA,Dec) = (359.988760, 54.025759) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:57.302, +54:01:32.732).
Field size: 15.6034 x 10.4307 degrees
Field rotation angle: up is 4.3774 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits' -> 'fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Sep 9 01:37 fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
-rw-r--r-- 1 apache apache 8.5K Sep 9 01:37 out1108578.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits (fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out1108578.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1108578.axy"...
Only searching for solutions within 15.4433 degrees of RA,Dec (359.99,54.0266)
log-odds ratio 22.4684 (5.72642e+09), 7 match, 0 conflict, 20 distractors, 26 index.
RA,Dec = (359.987,54.0249), pixel scale 5.93017 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 ./out1108578.solved to indicate this.
Field: out1108578.xyls
Field center: (RA,Dec) = (359.988760, 54.025759) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:57.302, +54:01:32.732).
Field size: 15.6034 x 10.4307 degrees
Field rotation angle: up is 4.3774 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 Sep 9 01:37 fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
-rw-r--r-- 1 apache apache 8.5K Sep 9 01:37 out1108578.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
WARNING: the local solve-field solution for fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits carries no SIP distortion terms while --tweak-order 2 was requested: the tweak silently failed on a marginal quad match and the TAN-only solution is unreliable away from the matched quad. Discarding it and retrying with a remote plate-solve server.
Local astrometry not available or failed, trying remote servers...
Setting up remote astrometry servers...
Checking if we can reach any plate solve servers... tau.kirx.net scan.sai.msu.ru scan.sai.msu.ru
The reachable servers are:
scan.sai.msu.ru
Updated list of available servers: scan.sai.msu.ru
We choose the plate solve server scan.sai.msu.ru
Using the remote server with Astrometry.net code
Plate solve server: scan.sai.msu.ru
Submitting the plates solving job to the server [01;34m scan.sai.msu.ru [00m
This may take [01;31mup to a few minutes[00m...
Plate solving parameters: -F fov=605 -F width=9576 -F hight=6388 http://scan.sai.msu.ru/cgi-bin/process_file/process_sextractor_list.py
% Total % Received % Xferd Average Speed Time Time Time Current
Dload Upload Total Spent Left Speed
0 0 0 0 0 0 0 0 0
100 124.3k 0 0 100 124.3k 0 78442 00:01 00:01 78452
100 124.3k 0 0 100 124.3k 0 42434 00:03 00:03 42437
100 124.3k 0 0 100 124.3k 0 31819 00:04 00:04 31820
100 124.3k 0 0 100 124.3k 0 25452 00:05 00:05 25454
100 124.3k 0 0 100 124.3k 0 21209 00:06 00:06 21210
100 124.3k 0 0 100 124.3k 0 18179 00:07 00:07 0
100 124.3k 0 0 100 124.3k 0 15906 00:08 00:08 0
100 124.3k 0 0 100 124.3k 0 14138 00:09 00:09 0
100 124.3k 0 0 100 124.3k 0 12724 00:10 00:10 0
100 128.9k 0 4670 100 124.3k 434 11856 00:10 00:10 813
100 128.9k 0 4670 100 124.3k 434 11855 00:10 00:10 813
100 128.9k 0 4670 100 124.3k 434 11855 00:10 00:10 813
'out1108578.xyls' -> 'test.xyls'
#### Plate solution log ####
% Total % Received % Xferd Average Speed Time Time Time Current
Dload Upload Total Spent Left Speed
0 0 0 0 0 0 0 0 0
100 3517 100 3517 0 0 4934 0 0
100 3517 100 3517 0 0 4933 0 0
100 3517 100 3517 0 0 4932 0 0
-rw-r--r-- 1 apache apache 124K Sep 9 06:37 files/4178tDreadrC/out1108578.xyls
export PATH=/var/www/cgi-venv/bin/:/var/www/scan.sai.msu.ru/venv_astrometrynet/bin/:/usr/local/astrometry/bin/:/bin:/sbin:/bin:/sbin:/usr/bin:/usr/sbin:/usr/bin:/usr/sbin:/usr/local/bin:/usr/local/sbin:/opt/bin:/usr/lib/llvm/19/bin:/usr/lib/llvm/18/bin:/usr/bin/cdsclient; cd files/4178tDreadrC/ ; timeout 4m solve-field --crpix-center --uniformize 0 --objs 1000 --depth 10,20,30-50 --no-plots --x-column X_IMAGE --y-column Y_IMAGE --sort-column FLUX_APER --width 9576.0 --height 6388.0 --scale-units arcminwidth --scale-low 544.5 --scale-high 3025.0 out1108578.xyls &>> program.log
Reading input file 1 of 1: "out1108578.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1108578.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 22.4684 (5.72642e+09), 7 match, 0 conflict, 20 distractors, 26 index.
RA,Dec = (359.987,54.0249), pixel scale 5.93017 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 ./out1108578.solved to indicate this.
Field: out1108578.xyls
Field center: (RA,Dec) = (359.988760, 54.025759) deg.
Field center: (RA H:M:S, Dec D:M:S) = (23:59:57.302, +54:01:32.732).
Field size: 15.6034 x 10.4307 degrees
Field rotation angle: up is 4.3774 degrees E of N
Field parity: neg
export PATH=/var/www/cgi-venv/bin/:/var/www/scan.sai.msu.ru/venv_astrometrynet/bin/:/usr/local/astrometry/bin/:/bin:/sbin:/bin:/sbin:/usr/bin:/usr/sbin:/usr/bin:/usr/sbin:/usr/local/bin:/usr/local/sbin:/opt/bin:/usr/lib/llvm/19/bin:/usr/lib/llvm/18/bin:/usr/bin/cdsclient; cd files/4178tDreadrC/ ; timeout 50 solve-field --overwrite --crpix-center --uniformize 0 --objs 10000 --depth 100 --tweak-order 3 --no-plots --x-column X_IMAGE --y-column Y_IMAGE --sort-column FLUX_APER --width 9576.0 --height 6388.0 --scale-units arcsecperpix --scale-low 5.6337 --scale-high 6.2267 --ra 359.988760 --dec 54.025759 --radius 5 out1108578.xyls &>> program.log
Reading input file 1 of 1: "out1108578.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out1108578.axy"...
Only searching for solutions within 5 degrees of RA,Dec (359.989,54.0258)
Field 1 did not solve (index index-4118.fits, field objects 1-100).
Field 1 did not solve (index index-4117.fits, field objects 1-100).
log-odds ratio 51.355 (2.00992e+22), 9 match, 0 conflict, 21 distractors, 26 index.
RA,Dec = (360,54.0089), pixel scale 5.9527 arcsec/pix.
Hit/miss: Hit/miss: +-++----+------+---++-----+--+(best)----------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out1108578.solved to indicate this.
Field: out1108578.xyls
Field center: (RA,Dec) = (0.001216, 54.009748) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:00.292, +54:00:35.093).
Field size: 15.7163 x 10.5215 degrees
Field rotation angle: up is 2.23468 degrees E of N
Field parity: neg
############################
Field [01;32mSOLVED[00m =)
Downloading WCS header... done
'/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits' -> 'fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Sep 9 01:38 fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
-rw-r--r-- 1 apache apache 8.5K Sep 9 01:38 out1108578.wcs
Inserting WCS header in fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits (remote) ... Opening FITS image file fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits for reading... done!
Creating new image file (wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'remote ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'scan.sai.msu.ru' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Sending request to remove job 4178tDreadrC from the server...
% Total % Received % Xferd Average Speed Time Time Time Current
Dload Upload Total Spent Left Speed
0 0 0 0 0 0 0 0 0
100 324 0 27 100 297 29 323 0
100 324 0 27 100 297 29 323 0
100 324 0 27 100 297 29 323 0
Job 4178tDreadrC removed.
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
Generating wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat from image00004.cat
Catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits created.
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
Image size: 941.3'x622.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.85"/pix along the Y axis
Image center: 00:00:00.629 +54:00:38.07 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 33040 stars ###
'wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/correct_sextractor_wcs_catalog_usingxy2sky1109185.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3431, bad_region=7295, passed=33040
Got 33040 stars (including 22839 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat
util/solve_plate_with_UCAC5 got 33040 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.0973 through 0 to 14.9904, gap 14.9904 to 345.0973
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 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4437 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3799 matched stars entering correct_measured_positions(), 3930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.16"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3731 matched stars entering correct_measured_positions(), 27245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.84"
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 345.0867 through 0 to 14.9947, gap 14.9947 to 345.0867
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 48.1 to 59.3)
Done reading UCAC5 zone files...
Matched 4542 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4036 matched stars entering correct_measured_positions(), 27245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.71"
Accuracy estimation diagnostic: 4017 matched stars entering correct_measured_positions(), 27243 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.43"
Excluding outliers - 4017 stars left (next iteration limit 4104)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4017 robust_rms=5.044 arcsec worst_quadrant_rms=105.305 arcsec
SIP_REFIT: SIP order 3 trial: matched=4017 robust_rms=0.517 arcsec worst_quadrant_rms=76.636 arcsec
SIP_REFIT: SIP order 5 trial: matched=4017 robust_rms=0.453 arcsec worst_quadrant_rms=70.351 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4017 robust_rms_before=25.973 arcsec robust_rms_before_corrected=2.042 arcsec robust_rms_after=0.453 arcsec worst_quadrant_rms_before=19.425 worst_quadrant_rms_after=70.351
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 19.425 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits N_match=4017 sigma_overall_arcsec=1.955 sigma_q1_arcsec=1.531 sigma_q2_arcsec=1.185 sigma_q3_arcsec=12.126 sigma_q4_arcsec=1.149 n_q1=1341 n_q2=849 n_q3=870 n_q4=957 worst_quadrant_to_overall_ratio=6.202
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits -region wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
WCS_QUALITY_RETRY: the retry reproduced the identical solution for 2nd new image (fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits) - the plate solve is deterministic for this image and the tweak order is not the problem (suspect a marginal quad match; see the silently-failed-tweak guard in util/wcs_image_calibration.sh)
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 2nd new image (fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits): sigma 1.955->1.955, ratio 6.202->6.202; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=2.041 -- 4.41x the reference average (0.463); plate solution may be of low accuracy
WARNING: 2nd new image has sigma_overall_arcsec=1.955 -- 4.22x the reference average (0.463); plate solution may be of low accuracy
WARNING: 1st new image has worst_quadrant_to_overall_ratio=5.426 -- 4.89x the reference average (1.1085); plate solution may be of low accuracy
WARNING: 2nd new image has worst_quadrant_to_overall_ratio=6.202 -- 5.59x the reference average (1.1085); 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_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095_astrometric_residuals.png (4002 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.91 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096_astrometric_residuals.png (4017 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.94 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-13-45_20.00sec_-0.00C_LIGHT_0095.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cas-04-Q2b1x1_011855_TTUQ2b1x1_2844802_ujvlG8Kg/wcs_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096.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 00:08:37.34 +56:07:36.1: 11.99 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:43:47.21 +58:01:11.0: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:14.93 +54:16:11.9: 15.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:26.57 +51:05:19.5: 11.86 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:20.28 +52:09:11.6: 11.79 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:04:36.44 +57:49:20.5: 12.04 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:48.78 +55:36:07.9: 12.01 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:29:05.12 +49:30:12.3: 11.81 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:24:22.26 +50:32:22.0: 11.87 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:11:49.87 +51:40:43.6: 11.80 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:20.28 +52:09:11.6: 12.08 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:08:37.34 +56:07:36.1: 12.11 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:48.78 +55:36:07.9: 12.22 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:04:36.44 +57:49:20.5: 12.09 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:29:05.12 +49:30:12.3: 11.92 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:26.57 +51:05:19.5: 12.11 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:43:47.21 +58:01:11.0: 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 23:31:14.93 +54:16:11.9: 14.67 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Forced photometry filter REJECTED candidate at 23:36:20.28 +52:09:11.6: ref_mag=11.83 +/- 0.01 new_mean_mag=12.1663 delta=-0.33 (need > 0.90)
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter REJECTED candidate at 00:05:48.78 +55:36:07.9: ref_mag=12.05 +/- 0.01 new_mean_mag=12.3250 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:08:37.34 +56:07:36.1: ref_mag=12.01 +/- 0.01 new_mean_mag=12.2117 delta=-0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:04:36.44 +57:49:20.5: ref_mag=12.05 +/- 0.01 new_mean_mag=12.1669 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:29:05.12 +49:30:12.3: ref_mag=11.83 +/- 0.01 new_mean_mag=12.1506 delta=-0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:23:26.57 +51:05:19.5: ref_mag=11.90 +/- 0.01 new_mean_mag=12.2936 delta=-0.39 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:11:49.87 +51:40:43.6: 12.05 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:24:22.26 +50:32:22.0: 12.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Forced photometry filter REJECTED candidate at 00:11:49.87 +51:40:43.6: ref_mag=11.84 +/- 0.01 new_mean_mag=12.2404 delta=-0.40 (need > 0.90)
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Forced photometry filter REJECTED candidate at 23:24:22.26 +50:32:22.0: ref_mag=11.89 +/- 0.01 new_mean_mag=12.0999 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:21:49.81 +53:49:32.5: 11.96 +/- 0.01 detection
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 +52:59:31.2: 11.73 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:13.94 +56:40:58.2: 11.93 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:40.43 +50:05:34.7: 11.81 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:18:40.98 +51:26:59.1: 11.19 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:38:07.44 +52:23:54.3: 11.81 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:06:21.63 +52:30:14.3: 11.86 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:48.80 +52:59:31.2: 12.02 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:21:49.81 +53:49:32.5: 12.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter REJECTED candidate at 23:31:48.80 +52:59:31.2: ref_mag=11.77 +/- 0.01 new_mean_mag=12.0341 delta=-0.26 (need > 0.90)
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:13.94 +56:40:58.2: 12.05 +/- 0.05 detection
Forced photometry filter REJECTED candidate at 00:21:49.81 +53:49:32.5: ref_mag=11.99 +/- 0.01 new_mean_mag=12.1295 delta=-0.14 (need > 0.90)
Forced photometry reference-image weighted average: 11.98 +/- 0.03
Forced photometry filter REJECTED candidate at 23:57:13.94 +56:40:58.2: ref_mag=11.98 +/- 0.03 new_mean_mag=12.0053 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:18:40.98 +51:26:59.1: 11.58 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:40.43 +50:05:34.7: 12.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.01
Forced photometry filter REJECTED candidate at 23:18:40.98 +51:26:59.1: ref_mag=11.24 +/- 0.01 new_mean_mag=12.0974 delta=-0.85 (need > 0.90)
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Forced photometry filter REJECTED candidate at 23:34:40.43 +50:05:34.7: ref_mag=11.85 +/- 0.01 new_mean_mag=12.0854 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:15:13.65 +57:49:14.8: 11.45 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:38:07.44 +52:23:54.3: 11.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Forced photometry filter REJECTED candidate at 23:38:07.44 +52:23:54.3: ref_mag=11.84 +/- 0.01 new_mean_mag=12.0164 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:06:21.63 +52:30:14.3: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Forced photometry filter REJECTED candidate at 00:06:21.63 +52:30:14.3: ref_mag=11.89 +/- 0.01 new_mean_mag=12.0473 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:15:13.65 +57:49:14.8: 11.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.01
Forced photometry filter REJECTED candidate at 00:15:13.65 +57:49:14.8: ref_mag=11.51 +/- 0.01 new_mean_mag=11.9825 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:39.71 +50:21:42.0: 11.55 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:02:41.35 +52:58:16.6: 11.51 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:47.40 +54:32:06.3: 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 00:12:31.42 +53:39:59.1: 11.52 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:43.59 +57:07:19.3: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:29.88 +52:53:06.0: 11.35 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:39.71 +50:21:42.0: 11.62 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:02:41.35 +52:58:16.6: 11.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Forced photometry filter REJECTED candidate at 23:23:39.71 +50:21:42.0: ref_mag=11.56 +/- 0.01 new_mean_mag=11.9860 delta=-0.42 (need > 0.90)
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Forced photometry filter REJECTED candidate at 00:02:41.35 +52:58:16.6: ref_mag=11.55 +/- 0.01 new_mean_mag=11.9692 delta=-0.41 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:12:31.42 +53:39:59.1: 11.82 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:47.40 +54:32:06.3: 14.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Forced photometry filter REJECTED candidate at 00:12:31.42 +53:39:59.1: ref_mag=11.57 +/- 0.01 new_mean_mag=12.0282 delta=-0.46 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:24.48 +51:46:48.5: 11.77 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:37.26 +51:28:18.1: 11.41 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:43.59 +57:07:19.3: 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 23:37:29.88 +52:53:06.0: 11.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.40 +/- 0.01
Forced photometry filter REJECTED candidate at 23:37:29.88 +52:53:06.0: ref_mag=11.40 +/- 0.01 new_mean_mag=11.9065 delta=-0.51 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:24.48 +51:46:48.5: 11.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Forced photometry filter REJECTED candidate at 23:42:24.48 +51:46:48.5: ref_mag=11.80 +/- 0.01 new_mean_mag=11.8787 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:28:37.26 +51:28:18.1: 11.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Forced photometry filter REJECTED candidate at 23:28:37.26 +51:28:18.1: ref_mag=11.44 +/- 0.01 new_mean_mag=11.8180 delta=-0.37 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:26:43.55 +50:38:16.8: 14.35 +/- 0.13 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:45:18.92 +54:17:58.8: 11.34 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:18:45.32 +54:13:44.5: 11.28 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:26:43.55 +50:38:16.8: 14.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.35 +/- 0.13
Forced photometry filter KEPT candidate at 00:26:43.55 +50:38:16.8: ref_mag=14.35 +/- 0.13 new_mean_mag=11.9698 delta=2.38 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:23:26.83 +55:05:04.9: 15.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:43:38.18 +51:08:51.0: 10.87 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:55:34.85 +51:17:32.1: 10.94 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:45:18.92 +54:17:58.8: 11.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.01
Forced photometry filter REJECTED candidate at 23:45:18.92 +54:17:58.8: ref_mag=11.38 +/- 0.01 new_mean_mag=11.5754 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:18:45.32 +54:13:44.5: 11.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Forced photometry filter REJECTED candidate at 00:18:45.32 +54:13:44.5: ref_mag=11.33 +/- 0.01 new_mean_mag=11.8273 delta=-0.50 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:23:26.83 +55:05:04.9: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:43:38.18 +51:08:51.0: 11.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.00
Forced photometry filter REJECTED candidate at 23:43:38.18 +51:08:51.0: ref_mag=10.91 +/- 0.00 new_mean_mag=11.5249 delta=-0.61 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:55:34.85 +51:17:32.1: 11.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Forced photometry filter REJECTED candidate at 23:55:34.85 +51:17:32.1: ref_mag=10.97 +/- 0.00 new_mean_mag=11.4759 delta=-0.50 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:32:00.74 +56:21:49.6: 11.09 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:30.16 +56:58:31.3: 10.78 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:37:03.91 +52:31:27.2: 10.41 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:31:56.10 +52:52:13.4: 10.58 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:32:00.74 +56:21:49.6: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 11.09 +/- 0.01
Forced photometry filter REJECTED candidate at 00:32:00.74 +56:21:49.6: ref_mag=11.09 +/- 0.01 new_mean_mag=11.4486 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:30.16 +56:58:31.3: 10.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.82 +/- 0.00
Forced photometry filter REJECTED candidate at 00:05:30.16 +56:58:31.3: ref_mag=10.82 +/- 0.00 new_mean_mag=11.3390 delta=-0.52 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:37:03.91 +52:31:27.2: 10.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.45 +/- 0.00
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:31:56.10 +52:52:13.4: 10.69 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 23:37:03.91 +52:31:27.2: ref_mag=10.45 +/- 0.00 new_mean_mag=11.1072 delta=-0.66 (need > 0.90)
Forced photometry reference-image weighted average: 10.60 +/- 0.00
Forced photometry filter REJECTED candidate at 23:31:56.10 +52:52:13.4: ref_mag=10.60 +/- 0.00 new_mean_mag=11.0252 delta=-0.42 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:12:50.43 +57:13:07.2: 11.02 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:54:30.04 +51:55:04.3: 10.89 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:37.54 +52:05:01.5: 10.75 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:12:50.43 +57:13:07.2: 11.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.01
Forced photometry filter REJECTED candidate at 00:12:50.43 +57:13:07.2: ref_mag=11.03 +/- 0.01 new_mean_mag=11.2194 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:41.93 +53:22:33.0: 10.70 +/- 0.00 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:54:30.04 +51:55:04.3: 11.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.92 +/- 0.00
Forced photometry filter REJECTED candidate at 23:54:30.04 +51:55:04.3: ref_mag=10.92 +/- 0.00 new_mean_mag=11.3206 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:34:37.54 +52:05:01.5: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.80 +/- 0.00
Forced photometry filter REJECTED candidate at 23:34:37.54 +52:05:01.5: ref_mag=10.80 +/- 0.00 new_mean_mag=11.4367 delta=-0.63 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:41.93 +53:22:33.0: 11.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.74 +/- 0.00
Forced photometry filter REJECTED candidate at 23:58:41.93 +53:22:33.0: ref_mag=10.74 +/- 0.00 new_mean_mag=11.4667 delta=-0.72 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:00:10.05 +51:17:32.8: 11.26 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:15:09.84 +53:35:02.6: 11.79 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:23:14.80 +51:45:19.1: 11.51 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:00:10.05 +51:17:32.8: 11.50 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:08:57.08 +49:42:59.0: 11.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.01
Forced photometry filter REJECTED candidate at 00:00:10.05 +51:17:32.8: ref_mag=11.30 +/- 0.01 new_mean_mag=11.6520 delta=-0.35 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:15:09.84 +53:35:02.6: 11.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Forced photometry filter REJECTED candidate at 00:15:09.84 +53:35:02.6: ref_mag=11.80 +/- 0.01 new_mean_mag=11.7760 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:23:14.80 +51:45:19.1: 11.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Forced photometry filter REJECTED candidate at 00:23:14.80 +51:45:19.1: ref_mag=11.55 +/- 0.01 new_mean_mag=11.7217 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:08:57.08 +49:42:59.0: 11.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Forced photometry filter REJECTED candidate at 00:08:57.08 +49:42:59.0: ref_mag=11.56 +/- 0.01 new_mean_mag=11.8818 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:15.65 +57:52:36.7: 13.22 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:44:13.98 +57:45:24.9: 15.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:49:42.98 +52:47:17.9: 11.86 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:22.67 +56:41:45.4: 12.17 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:15.65 +57:52:36.7: 13.29 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.04
Forced photometry filter KEPT candidate at 23:48:15.65 +57:52:36.7: ref_mag=13.24 +/- 0.04 new_mean_mag=11.8637 delta=1.38 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:44:13.98 +57:45:24.9: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:49:42.98 +52:47:17.9: 11.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Forced photometry filter REJECTED candidate at 23:49:42.98 +52:47:17.9: ref_mag=11.87 +/- 0.01 new_mean_mag=11.9302 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:22.67 +56:41:45.4: 12.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.04
Forced photometry filter REJECTED candidate at 23:57:22.67 +56:41:45.4: ref_mag=12.12 +/- 0.04 new_mean_mag=11.9394 delta=0.18 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:32:27.39 +53:34:05.6: 12.03 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:27:02.62 +52:20:08.7: 11.75 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:32:27.39 +53:34:05.6: 12.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Forced photometry filter REJECTED candidate at 23:32:27.39 +53:34:05.6: ref_mag=12.03 +/- 0.01 new_mean_mag=12.0061 delta=0.02 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:27:02.62 +52:20:08.7: 11.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry filter REJECTED candidate at 23:27:02.62 +52:20:08.7: ref_mag=11.78 +/- 0.01 new_mean_mag=11.9661 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:51:04.16 +51:20:58.9: 12.05 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:48:20.10 +55:53:29.9: 12.10 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:51:04.16 +51:20:58.9: 12.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter REJECTED candidate at 23:51:04.16 +51:20:58.9: ref_mag=12.06 +/- 0.01 new_mean_mag=12.0728 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:48:20.10 +55:53:29.9: 12.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry filter REJECTED candidate at 23:48:20.10 +55:53:29.9: ref_mag=12.10 +/- 0.01 new_mean_mag=12.0858 delta=0.01 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:26:54.01 +52:55:42.7: 12.10 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:21:40.12 +50:25:09.8: 11.89 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:26:54.01 +52:55:42.7: 12.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter REJECTED candidate at 00:26:54.01 +52:55:42.7: ref_mag=12.13 +/- 0.01 new_mean_mag=12.2004 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:21:40.12 +50:25:09.8: 12.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter REJECTED candidate at 00:21:40.12 +50:25:09.8: ref_mag=11.93 +/- 0.01 new_mean_mag=12.2220 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:18:15.31 +54:06:18.6: 12.12 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:05:40.70 +55:50:56.3: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:18:15.31 +54:06:18.6: 12.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter REJECTED candidate at 00:18:15.31 +54:06:18.6: ref_mag=12.13 +/- 0.01 new_mean_mag=12.2028 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:05:40.70 +55:50:56.3: 12.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter REJECTED candidate at 00:05:40.70 +55:50:56.3: ref_mag=12.25 +/- 0.01 new_mean_mag=12.1681 delta=0.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:02:30.54 +55:50:44.0: 12.17 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:02:30.54 +55:50:44.0: 12.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 00:02:30.54 +55:50:44.0: ref_mag=12.17 +/- 0.01 new_mean_mag=12.1658 delta=0.01 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:28:42.59 +57:11:03.1: 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 23:28:42.59 +57:11:03.1: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:57.99 +50:29:19.8: 12.31 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:57.99 +50:29:19.8: 12.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.02
Forced photometry filter REJECTED candidate at 23:58:57.99 +50:29:19.8: ref_mag=12.30 +/- 0.02 new_mean_mag=12.2773 delta=0.02 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:15:27.82 +50:45:27.1: 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 00:15:27.82 +50:45:27.1: 12.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.02
Forced photometry filter REJECTED candidate at 00:15:27.82 +50:45:27.1: ref_mag=12.31 +/- 0.02 new_mean_mag=12.3055 delta=0.00 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:21:37.53 +49:47:30.0: 12.22 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:21:37.53 +49:47:30.0: 12.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.02
Forced photometry filter REJECTED candidate at 23:21:37.53 +49:47:30.0: ref_mag=12.20 +/- 0.02 new_mean_mag=12.1850 delta=0.02 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:57:28.58 +56:42:23.5: 12.24 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:57:28.58 +56:42:23.5: 12.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.04
Forced photometry filter REJECTED candidate at 23:57:28.58 +56:42:23.5: ref_mag=12.17 +/- 0.04 new_mean_mag=12.2274 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:34:42.99 +57:22:12.9: 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 23:34:42.99 +57:22:12.9: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:13:32.64 +54:59:49.8: 12.30 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:13:32.64 +54:59:49.8: 12.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.02
Forced photometry filter REJECTED candidate at 00:13:32.64 +54:59:49.8: ref_mag=12.32 +/- 0.02 new_mean_mag=12.2938 delta=0.02 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:19:23.95 +55:37:01.7: 12.32 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:58:10.78 +50:30:02.1: 12.24 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:19:23.95 +55:37:01.7: 12.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.02
Forced photometry filter REJECTED candidate at 00:19:23.95 +55:37:01.7: ref_mag=12.31 +/- 0.02 new_mean_mag=12.2614 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:58:10.78 +50:30:02.1: 12.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.02
Forced photometry filter REJECTED candidate at 23:58:10.78 +50:30:02.1: ref_mag=12.27 +/- 0.02 new_mean_mag=12.2931 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:55:04.22 +50:18:19.0: 12.19 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:43:35.92 +51:23:15.5: 12.26 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:44:45.54 +52:00:54.0: 12.29 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:36:22.34 +53:47:59.8: 12.28 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:55:04.22 +50:18:19.0: 12.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter REJECTED candidate at 23:55:04.22 +50:18:19.0: ref_mag=12.20 +/- 0.01 new_mean_mag=12.2833 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:43:35.92 +51:23:15.5: 12.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry filter REJECTED candidate at 23:43:35.92 +51:23:15.5: ref_mag=12.25 +/- 0.02 new_mean_mag=12.2675 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:44:45.54 +52:00:54.0: 12.33 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:36:22.34 +53:47:59.8: 12.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.02
Forced photometry filter REJECTED candidate at 23:44:45.54 +52:00:54.0: ref_mag=12.30 +/- 0.02 new_mean_mag=12.2771 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Forced photometry filter REJECTED candidate at 23:36:22.34 +53:47:59.8: ref_mag=12.27 +/- 0.01 new_mean_mag=12.2406 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:00.39 +53:50:16.7: 12.22 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:42:05.79 +50:43:45.7: 12.21 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 00:09:59.46 +55:28:17.3: 12.25 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:53:17.82 +53:51:32.0: 12.32 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:00.39 +53:50:16.7: 12.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter REJECTED candidate at 23:42:00.39 +53:50:16.7: ref_mag=12.22 +/- 0.01 new_mean_mag=12.2514 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:42:05.79 +50:43:45.7: 12.25 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:51:16.33 +55:40:27.1: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter REJECTED candidate at 23:42:05.79 +50:43:45.7: ref_mag=12.22 +/- 0.01 new_mean_mag=12.2826 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 00:09:59.46 +55:28:17.3: 12.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter REJECTED candidate at 00:09:59.46 +55:28:17.3: ref_mag=12.25 +/- 0.01 new_mean_mag=12.2834 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:39:42.20 +55:51:27.0: 13.61 +/- 0.07 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:53:17.82 +53:51:32.0: 12.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.02
Forced photometry filter REJECTED candidate at 23:53:17.82 +53:51:32.0: ref_mag=12.32 +/- 0.02 new_mean_mag=12.2757 delta=0.04 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-18_02-46-42_20.00sec_-0.00C_LIGHTs_0246.fits at 23:13:58.82 +53:19:37.0: 13.75 +/- 0.09 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:51:16.33 +55:40:27.1: 12.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry filter REJECTED candidate at 23:51:16.33 +55:40:27.1: ref_mag=12.25 +/- 0.02 new_mean_mag=12.2910 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:39:42.20 +55:51:27.0: 14.01 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.06
Forced photometry filter KEPT candidate at 23:39:42.20 +55:51:27.0: ref_mag=13.66 +/- 0.06 new_mean_mag=12.2958 delta=1.36 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-07-21_23-21-38_20.00sec_5.00C_LIGHT_0111.fits at 23:13:58.82 +53:19:37.0: 14.30 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.08
Forced photometry filter KEPT candidate at 23:13:58.82 +53:19:37.0: ref_mag=13.82 +/- 0.08 new_mean_mag=12.2687 delta=1.55 (need > 0.90)
Adding exclusion_list_local.txt__out50565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50993.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 31s
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: 10s
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Considering the candidate 50557_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50557_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50560_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50560_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 50564_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50564_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50565_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 50565_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 50571_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50571_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 50574_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 50574_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 50575_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50575_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50579_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50579_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50581_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50581_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50583_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50583_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50585_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50585_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50587_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50587_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50589_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50589_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50593_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50593_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:43:42.19 +52:46:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50594_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50594_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50595_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50595_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50597_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50597_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50601_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50601_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50602_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50602_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:57:28.13 +56:41:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50604_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50604_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50605_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50605_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50606_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50606_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50607_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50607_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50609_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50609_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 50610_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 50610_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 50611_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50611_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50612_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50612_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50614_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50614_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:50:16.41 +52:52:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50615_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 50615_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 50618_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50618_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50620_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50620_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50621_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50621_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50623_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50623_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:05:40.45 +54:22:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50625_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 50625_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 50630_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50630_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:57:06.01 +56:45:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50631_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50631_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50637_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50637_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 50638_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50638_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50639_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 50639_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 50641_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50641_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50642_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50642_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50646_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50646_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50648_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50648_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50649_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50649_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50650_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50650_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50651_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50651_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:54:23.22 +53:19:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50660_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50660_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:21:11.77 +50:00:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50668_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50668_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:15:50.58 +57:32:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50672_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50672_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50673_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50673_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50674_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50674_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:18:59.68 +53:18:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50676_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50676_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50679_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50679_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50686_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50686_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:28:56.12 +57:11:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50688_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50688_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50692_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50692_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50699_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50699_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50711_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50711_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50713_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50713_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:17:41.62 +51:27:11.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 50728_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50728_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:49:24.09 +55:38:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50732_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50732_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:10:46.78 +49:57:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50742_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50742_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:25:21.20 +56:10:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50747_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 50747_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 50749_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 50749_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50761_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50761_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50773_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50773_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50795_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50795_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50797_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50797_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50810_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50810_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50819_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50819_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50823_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50823_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50832_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50832_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50840_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50840_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50848_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50848_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50851_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50851_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50852_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50852_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 50858_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 50858_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50862_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50862_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 50870_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50870_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50873_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50873_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50874_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50874_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50876_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50876_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50881_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 50881_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50889_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50889_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50890_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50890_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50891_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50891_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50895_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50895_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 50897_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50897_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50906_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50906_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50909_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50909_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50912_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50912_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50919_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50919_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50920_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50920_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50922_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50922_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50936_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50936_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 50940_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50940_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 50961_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 50961_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195209_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195209_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195222_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195222_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195355_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195355_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195367_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195367_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195370_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195370_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195389_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195389_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195399_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195399_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195420_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195420_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195433_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195433_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195445_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195445_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195447_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195447_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195453_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195453_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:24:56.87 +55:23:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 4.567 1996184014734179968 351.23917382686 +55.39097794884 15.1095 14.2779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195469_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195469_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195483_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195483_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195497_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195497_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195501_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195501_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195502_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195502_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195512_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195512_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195514_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195514_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195517_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195517_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195519_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195519_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195522_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195522_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195523_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195523_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195527_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195527_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195537_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195537_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195538_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195538_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195539_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195539_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195549_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195549_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195556_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195556_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195561_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195561_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195563_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195563_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195585_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195585_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195592_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195592_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195595_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195595_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195596_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195596_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195598_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195598_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195604_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195604_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195607_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195607_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195613_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195613_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195614_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195614_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195616_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195616_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195642_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195642_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195647_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195647_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195665_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195665_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195668_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195668_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195680_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195680_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195681_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195681_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195684_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195684_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195687_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195687_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195688_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195688_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195692_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195692_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195695_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195695_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195696_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195696_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195701_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195701_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195704_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195704_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195706_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195706_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195707_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195707_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195710_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195710_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195714_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195714_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195715_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195715_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195717_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195717_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 195720_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195720_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195721_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195721_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195725_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195725_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195726_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195726_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195728_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195728_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195733_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195733_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195734_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195734_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195736_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195736_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195744_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195744_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195745_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195745_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195746_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195746_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 195748_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195748_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 195752_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195752_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195766_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195766_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195770_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195770_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195772_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195772_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195773_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195773_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195778_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195778_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195781_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195781_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195782_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195782_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195784_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195784_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195793_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195793_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195796_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195796_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195797_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195797_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 195807_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195807_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195812_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195812_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195817_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195817_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195822_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195822_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195824_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195824_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195831_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195831_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:19:41.13 +56:10:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.773 1997134611254788352 349.92183527074 +56.17135705887 14.7537 13.9445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195834_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195834_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195835_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195835_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:48:08.06 +53:38:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195839_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195839_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195840_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195840_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195841_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195841_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195845_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195845_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195846_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195846_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195848_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195848_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195851_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195851_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 195854_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195854_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195856_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195856_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195857_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195857_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195858_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195858_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195860_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195860_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195861_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195861_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195863_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195863_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195871_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195871_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195872_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195872_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195873_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195873_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195877_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195877_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195888_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195888_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195889_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195889_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195890_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195890_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195891_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195891_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195892_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195892_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195893_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195893_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195897_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195897_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 195900_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195900_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195905_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195905_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195907_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195907_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195909_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195909_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195910_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195910_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195912_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195912_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195921_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195921_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195925_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195925_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195926_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195926_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195928_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195928_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195929_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195929_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195930_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195930_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195932_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195932_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195936_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195936_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195939_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195939_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195942_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 195942_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 195947_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195947_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195962_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195962_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195964_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195964_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195970_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195970_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (31.7") between the two second-epoch detections
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Considering the candidate 195971_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195971_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195974_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195974_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195975_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195975_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195976_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195976_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195978_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195978_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195979_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195979_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195980_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195980_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195982_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195982_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195985_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195985_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195987_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195987_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195988_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195988_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 195994_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195994_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 195997_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 195997_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196000_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196000_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196001_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196001_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196002_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196002_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196003_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196003_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196004_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196004_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196007_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196007_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196009_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196009_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196012_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196012_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196013_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196013_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196014_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196014_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196017_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196017_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196018_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196018_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196020_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196020_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196025_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196025_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196026_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196026_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196028_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196028_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196029_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196029_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196030_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196030_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196031_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196031_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196033_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196033_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196034_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196034_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196035_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196035_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196036_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196036_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196037_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196037_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196040_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196040_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196042_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196042_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196045_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196045_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196046_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196046_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196047_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196047_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196049_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196049_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196053_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196053_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196054_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196054_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196055_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196055_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196058_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196058_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196059_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196059_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196063_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196063_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196064_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196064_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196065_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196065_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196066_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196066_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196075_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196075_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196076_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196076_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196077_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196077_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 196081_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196081_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196082_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196082_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196083_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196083_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196085_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196085_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196087_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196087_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196090_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196090_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196091_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196091_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196094_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196094_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196102_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196102_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196103_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196103_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 196105_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196105_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (41.6") between the two second-epoch detections
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Considering the candidate 196108_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196108_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196109_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196109_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196112_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196112_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196117_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196117_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196119_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196119_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196121_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196121_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (25.2") between the two second-epoch detections
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Considering the candidate 196123_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196123_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196124_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196124_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196128_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196128_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196129_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196129_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196131_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196131_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196134_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196134_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196141_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196141_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196144_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196144_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196145_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196145_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196146_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196146_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196148_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196148_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196149_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196149_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196151_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196151_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196153_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196153_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196154_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196154_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196155_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196155_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196156_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196156_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196159_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196159_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196160_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196160_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196161_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196161_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196162_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196162_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196164_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196164_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196165_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196165_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196167_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196167_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196168_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196168_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196169_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196169_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196170_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196170_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196172_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196172_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196173_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196173_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196176_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196176_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196177_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196177_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196179_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196179_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196180_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196180_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196183_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196183_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196184_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196184_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196185_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196185_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196186_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196186_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196187_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196187_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196189_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196189_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196192_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196192_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196193_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196193_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196194_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196194_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196195_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196195_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196197_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196197_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196198_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196198_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196202_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196202_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196203_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196203_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196204_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196204_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196206_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196206_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196207_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196207_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196208_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196208_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196214_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196214_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196215_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196215_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196216_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196216_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196217_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196217_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196218_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196218_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196219_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196219_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196220_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196220_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196222_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196222_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196224_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196224_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196226_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196226_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196228_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196228_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196229_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196229_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196230_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196230_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196234_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196234_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196235_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196235_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196236_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196236_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196238_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196238_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196239_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196239_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196243_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196243_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196244_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196244_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196245_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196245_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196248_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196248_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196249_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196249_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196253_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196253_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196254_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196254_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196256_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196256_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 196257_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196257_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196259_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196259_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196263_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196263_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196264_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196264_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196266_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196266_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196267_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196267_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196268_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196268_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196269_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196269_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196273_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196273_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 196274_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196274_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196275_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196275_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196277_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196277_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196278_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196278_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196279_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196279_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196282_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196282_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196284_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196284_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196286_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196286_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196287_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196287_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196289_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196289_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196291_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196291_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196292_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196292_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196293_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196293_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196297_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196297_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196299_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196299_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:16:07.09 +51:04:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196301_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196301_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196303_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196303_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196304_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196304_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196306_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196306_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196307_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196307_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196308_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196308_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196310_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196310_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196311_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196311_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196314_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196314_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196315_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196315_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196316_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196316_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196319_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196319_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196320_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196320_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196321_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196321_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196324_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196324_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196326_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196326_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196327_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196327_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196331_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196331_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196335_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196335_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196338_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196338_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196340_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196340_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196341_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196341_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196342_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196342_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196347_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196347_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196349_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196349_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196350_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196350_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196352_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196352_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196355_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196355_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196360_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196360_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196363_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196363_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196364_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196364_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196367_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196367_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196369_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196369_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196371_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196371_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196376_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196376_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196378_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196378_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196383_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196383_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196385_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196385_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196388_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196388_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196389_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196389_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196390_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196390_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196391_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196391_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196392_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196392_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196394_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196394_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 196396_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196396_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196397_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196397_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196402_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196402_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196403_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196403_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196408_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196408_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196409_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196409_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196411_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196411_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196413_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196413_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196414_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196414_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196415_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196415_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196416_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196416_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196417_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196417_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (35.0") between the two second-epoch detections
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Considering the candidate 196420_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196420_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (33.4") between the two second-epoch detections
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Considering the candidate 196421_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196421_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196425_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196425_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196427_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196427_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196428_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196428_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196429_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196429_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196431_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196431_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196433_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196433_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196434_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196434_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196436_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196436_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196438_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196438_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196439_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196439_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196440_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196440_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196441_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196441_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196442_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196442_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196444_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196444_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196446_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196446_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196447_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196447_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196448_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196448_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196450_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196450_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196451_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196451_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196452_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196452_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196453_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196453_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196455_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196455_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196456_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196456_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196457_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196457_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196461_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196461_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196463_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196463_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196464_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196464_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196465_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196465_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196466_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196466_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196467_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196467_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196470_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196470_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196471_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196471_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196472_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196472_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196473_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196473_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196474_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196474_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196475_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196475_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196476_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196476_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (40.2") between the two second-epoch detections
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Considering the candidate 196477_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196477_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196479_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196479_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196480_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196480_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196481_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196481_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196482_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196482_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196483_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196483_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196484_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196484_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196486_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196486_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196487_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196487_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196488_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196488_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196492_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196492_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196493_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196493_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196495_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196495_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196496_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196496_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196497_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196497_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196499_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196499_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196501_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196501_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196502_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196502_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196503_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196503_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196504_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196504_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196506_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196506_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196507_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196507_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196508_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196508_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196510_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196510_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196513_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196513_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196515_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196515_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196516_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196516_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196517_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196517_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196518_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196518_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196519_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196519_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196521_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196521_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196522_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196522_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196524_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196524_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196525_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196525_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196528_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196528_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:56:03.79 +56:52:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196531_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196531_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196532_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196532_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196533_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196533_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196535_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196535_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196536_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196536_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196537_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196537_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196538_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196538_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196539_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196539_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196540_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196540_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196541_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196541_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196543_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196543_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196548_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196548_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196553_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196553_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (40.3") between the two second-epoch detections
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Considering the candidate 196554_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196554_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196555_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196555_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196558_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196558_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196559_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196559_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196561_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196561_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:48:09.80 +55:32:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196562_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196562_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196563_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196563_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196564_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196564_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196566_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196566_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196567_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196567_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196568_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196568_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196569_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196569_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196570_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196570_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196571_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196571_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196572_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196572_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196573_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196573_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196575_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196575_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196576_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196576_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 196577_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196577_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196578_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196578_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196584_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196584_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196587_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196587_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196588_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196588_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196589_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196589_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196590_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196590_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196591_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196591_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196593_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196593_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196596_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196596_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196597_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196597_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196598_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196598_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:44:28.44 +55:14:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196599_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196599_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196600_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196600_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196604_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196604_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196606_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196606_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196608_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196608_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196610_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196610_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196612_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196612_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196613_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196613_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196615_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196615_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196620_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196620_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196621_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196621_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196623_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196623_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196625_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196625_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196626_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196626_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196627_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196627_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196628_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196628_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196630_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196630_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196631_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196631_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196632_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196632_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196633_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196633_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196635_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196635_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196637_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196637_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196638_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196638_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196640_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196640_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196642_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196642_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196643_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196643_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196644_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196644_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196647_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196647_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196648_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196648_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196649_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196649_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196650_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196650_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196653_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196653_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196656_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196656_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196657_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196657_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196658_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196658_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196659_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196659_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196661_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196661_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196662_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196662_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196663_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196663_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:13:59.80 +57:05:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196664_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196664_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196665_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196665_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196667_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196667_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196668_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196668_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196670_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196670_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196673_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196673_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196677_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196677_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196679_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196679_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196680_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196680_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196682_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196682_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196683_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196683_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196686_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196686_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196687_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196687_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196688_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196688_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196689_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196689_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 196690_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196690_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196692_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196692_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196693_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196693_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196694_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196694_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196696_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196696_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196697_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196697_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196699_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196699_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (47.7") between the two second-epoch detections
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Considering the candidate 196701_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196701_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196702_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196702_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196703_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196703_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196705_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196705_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196706_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196706_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196708_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196708_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196709_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196709_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196710_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196710_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196711_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196711_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196712_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196712_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196713_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196713_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196716_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196716_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196719_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196719_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196721_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196721_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196726_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196726_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196730_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196730_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196731_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196731_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196733_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196733_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196736_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196736_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196737_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196737_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196738_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196738_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196740_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196740_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196744_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196744_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196747_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196747_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:19:16.41 +58:04:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196750_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196750_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196752_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196752_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 196753_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196753_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196754_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196754_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196756_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196756_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196757_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196757_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196759_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196759_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196760_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196760_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196761_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196761_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196762_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196762_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196766_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196766_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196768_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196768_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196770_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196770_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196772_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196772_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196773_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196773_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196774_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196774_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196775_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196775_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196776_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196776_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196778_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196778_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196779_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196779_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196780_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196780_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196782_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196782_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196786_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196786_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196787_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196787_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196789_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196789_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196791_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196791_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196792_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196792_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196793_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196793_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196794_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196794_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196795_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196795_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196796_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196796_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196798_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196798_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196799_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196799_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196800_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196800_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196801_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196801_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196804_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196804_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196805_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196805_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196806_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196806_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196807_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196807_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196808_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196808_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196809_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196809_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196811_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196811_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196813_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196813_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196815_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196815_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196819_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196819_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196822_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196822_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196824_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196824_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196825_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196825_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196826_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196826_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 196828_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196828_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196832_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196832_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196835_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196835_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196838_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196838_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196843_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196843_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196844_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196844_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:53:56.28 +56:03:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196846_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196846_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196849_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196849_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196856_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196856_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196857_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196857_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196858_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196858_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196859_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196859_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196860_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196860_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:09:03.38 +51:49:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196861_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196861_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196862_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196862_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196863_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196863_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196864_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196864_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196865_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196865_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:04:35.26 +52:41:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196866_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196866_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196868_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196868_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196869_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196869_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196871_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196871_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196872_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196872_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196873_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196873_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196874_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196874_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196875_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196875_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196877_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196877_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196878_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196878_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196879_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196879_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196881_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196881_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196883_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196883_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 196884_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196884_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196885_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196885_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196886_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196886_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196887_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196887_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196889_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196889_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196890_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196890_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196892_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196892_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196893_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196893_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196894_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196894_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196896_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196896_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196901_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196901_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196902_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196902_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196904_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196904_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196906_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196906_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196908_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196908_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196909_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196909_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196910_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196910_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196911_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196911_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196912_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196912_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196915_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196915_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196917_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196917_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196918_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196918_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196920_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196920_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196922_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196922_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196924_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196924_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196925_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196925_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196926_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196926_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196929_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196929_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196930_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196930_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196931_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196931_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196932_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196932_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196933_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196933_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196934_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196934_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196935_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196935_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196937_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196937_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196938_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196938_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196939_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196939_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196942_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196942_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196943_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196943_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196948_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196948_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196949_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196949_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196950_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196950_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196952_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196952_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196953_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196953_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196955_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196955_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196957_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196957_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196958_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196958_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196961_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196961_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 196963_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196963_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196966_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196966_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196967_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196967_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196968_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196968_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196969_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196969_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196970_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196970_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 196972_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196972_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 196973_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196973_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196974_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196974_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196976_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 196976_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196978_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196978_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196980_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196980_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196981_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196981_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196983_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196983_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196988_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196988_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196990_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196990_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196992_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196992_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196993_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196993_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:23:48.19 +52:23:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196995_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196995_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196998_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 196998_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197001_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197001_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197002_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197002_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197003_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197003_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197004_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197004_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197005_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197005_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197006_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197006_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197008_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197008_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 197014_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197014_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197017_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197017_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197018_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197018_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197020_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197020_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197022_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197022_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197023_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197023_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197025_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197025_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197026_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197026_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197027_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197027_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197028_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197028_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197031_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197031_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197033_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197033_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197034_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197034_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197037_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197037_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197038_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197038_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197040_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197040_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197041_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197041_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197043_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197043_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197046_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197046_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197048_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197048_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197049_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197049_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197051_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197051_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197053_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197053_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:12:56.07 +53:57:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197054_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197054_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197055_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197055_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197056_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197056_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:02:22.89 +54:16:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197057_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197057_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197060_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197060_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197061_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197061_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197063_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197063_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197064_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197064_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197065_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197065_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197067_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197067_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197070_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197070_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:50:05.46 +51:44:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197071_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197071_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197074_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197074_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197076_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197076_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197078_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197078_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197080_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197080_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197081_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197081_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197084_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197084_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197086_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197086_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197088_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197088_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197090_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197090_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197094_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197094_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197096_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197096_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197098_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197098_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197102_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197102_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197104_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197104_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197105_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197105_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197106_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197106_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197108_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197108_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197109_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197109_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197110_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197110_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197111_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197111_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197112_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197112_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197115_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197115_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197116_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197116_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197117_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197117_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197118_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197118_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197121_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197121_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197123_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197123_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197125_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197125_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197126_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197126_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197129_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197129_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197134_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197134_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197137_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197137_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197140_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197140_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197141_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197141_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:00:49.16 +56:12:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197144_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197144_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197145_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197145_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197146_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197146_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197149_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197149_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197151_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197151_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197153_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197153_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197157_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197157_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197159_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197159_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:00:32.64 +54:57:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197160_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197160_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197165_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197165_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197167_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197167_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197168_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197168_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197169_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197169_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197171_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197171_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197180_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197180_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197183_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197183_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197184_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197184_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197185_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197185_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197186_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197186_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197189_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197189_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197190_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197190_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197195_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197195_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197197_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197197_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197198_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197198_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197202_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197202_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197203_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197203_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197207_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197207_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197208_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197208_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197209_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197209_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197211_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197211_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197214_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197214_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197215_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197215_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197217_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197217_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197219_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197219_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197221_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197221_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197223_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197223_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197224_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197224_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197228_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197228_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197229_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197229_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197231_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197231_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197240_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197240_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197242_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197242_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197243_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197243_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197244_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197244_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197246_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197246_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197248_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197248_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197252_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197252_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:09:10.04 +53:31:17.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197255_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197255_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197257_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197257_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197258_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197258_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197262_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197262_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197265_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197265_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197266_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197266_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197268_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197268_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197270_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197270_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197272_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197272_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197273_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197273_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197274_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197274_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197275_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197275_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (25.2") between the two second-epoch detections
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Considering the candidate 197278_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197278_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197279_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197279_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197280_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197280_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197281_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197281_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197282_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197282_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197283_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197283_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197286_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197286_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197288_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197288_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197289_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197289_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197290_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197290_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197291_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197291_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (27.2") between the two second-epoch detections
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Considering the candidate 197295_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197295_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197296_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197296_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197297_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197297_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:30:59.89 +57:25:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197299_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197299_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197302_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197302_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197303_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197303_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197304_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197304_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197305_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197305_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197306_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197306_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197307_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197307_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197308_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197308_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197312_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197312_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197313_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197313_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197315_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197315_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197316_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197316_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197317_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197317_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197318_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197318_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197319_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197319_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:23:16.63 +56:00:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197320_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197320_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197322_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197322_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197325_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197325_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197326_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197326_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197327_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197327_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:07:59.39 +53:43:32.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197328_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197328_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197331_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197331_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197334_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197334_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197340_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197340_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197343_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197343_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197345_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197345_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197346_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197346_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197354_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197354_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197359_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197359_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197360_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197360_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197361_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197361_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197362_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197362_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197364_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197364_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197365_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197365_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197366_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197366_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197367_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197367_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:54:22.32 +51:36:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197368_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197368_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197369_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197369_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197373_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197373_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197374_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197374_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197377_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197377_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197378_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197378_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197381_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197381_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197382_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197382_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197386_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197386_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:27:45.32 +55:38:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197387_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197387_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197389_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197389_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197390_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197390_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197393_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197393_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:21:13.14 +51:19:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197395_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197395_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197399_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197399_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197401_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197401_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:46:21.71 +52:57:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197402_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197402_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197406_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197406_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197409_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197409_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197411_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197411_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197412_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197412_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197413_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197413_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197417_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197417_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197419_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197419_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197422_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197422_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197423_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197423_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:19:08.26 +56:05:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197425_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197425_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197433_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197433_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197435_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197435_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197438_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197438_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:55:04.11 +54:11:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197439_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197439_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (33.8") between the two second-epoch detections
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Considering the candidate 197440_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197440_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:17:29.16 +52:59:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197441_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197441_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197442_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197442_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197447_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197447_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:26:29.21 +57:34:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197449_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197449_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197452_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197452_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197454_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197454_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:47:25.24 +52:34:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197455_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197455_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197458_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197458_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197459_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197459_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197461_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197461_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197463_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197463_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197466_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197466_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197468_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197468_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:23:06.23 +53:52:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197469_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197469_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (37.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197470_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197470_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197472_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197472_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197473_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197473_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197476_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197476_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:46:28.48 +55:13:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197477_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197477_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197482_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197482_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197483_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197483_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197484_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197484_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197487_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197487_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:23:29.18 +54:55:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197497_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197497_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:07:22.96 +50:57:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197499_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197499_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197500_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197500_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197501_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197501_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:02:52.69 +55:52:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197502_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197502_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197503_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197503_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197505_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197505_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197506_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197506_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:02:02.16 +55:09:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197510_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197510_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197511_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197511_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197514_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197514_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (52.0") between the two second-epoch detections
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Considering the candidate 197516_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197516_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197518_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197518_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:04:00.85 +53:21:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197521_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197521_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197523_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197523_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197526_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197526_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197529_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197529_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197530_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197530_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197531_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197531_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197534_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197534_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:56:37.37 +54:36:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197536_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197536_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197537_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197537_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:59:19.60 +53:52:11.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 197560_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197560_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197564_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197564_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197568_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197568_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197573_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197573_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:10:46.89 +49:57:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197592_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197592_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197594_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197594_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197596_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197596_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197598_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197598_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197599_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197599_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197612_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197612_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197619_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197619_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:22:50.94 +52:21:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197624_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197624_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197632_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197632_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 197633_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197633_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:04:13.16 +51:32:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197637_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197637_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:19:09.72 +53:54:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197640_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197640_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:17:35.00 +49:43:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197644_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197644_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:08:38.03 +51:24:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197645_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197645_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:08:06.22 +51:28:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197647_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197647_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197655_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197655_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:19:52.92 +52:11:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197656_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197656_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197663_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197663_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:17:25.04 +52:04:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197664_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197664_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:24:52.83 +53:56:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197666_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197666_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197671_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197671_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197672_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197672_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197683_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197683_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197688_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197688_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197690_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197690_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197692_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197692_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:00:35.92 +53:44:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197701_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197701_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197704_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197704_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197714_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197714_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197715_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197715_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197726_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197726_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197743_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197743_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197747_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197747_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:29:36.99 +53:56:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197750_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197750_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197751_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197751_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197752_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197752_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197759_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197759_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197763_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197763_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197764_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197764_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:31:00.22 +55:18:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197768_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197768_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197773_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197773_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:25:01.50 +53:42:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197780_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197780_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197784_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197784_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197788_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197788_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197791_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197791_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (31.6") between the two second-epoch detections
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Considering the candidate 197792_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197792_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197793_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197793_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197802_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197802_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197803_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197803_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:05:14.94 +52:06:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197806_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197806_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197807_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197807_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197809_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197809_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:23:59.74 +53:11:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197814_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197814_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197818_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197818_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197823_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197823_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197828_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197828_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197829_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197829_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197832_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197832_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197834_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197834_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197836_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197836_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197837_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197837_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:57:04.52 +52:10:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197846_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197846_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:14:31.03 +53:08:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197851_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197851_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197854_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197854_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:18:40.10 +54:23:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197865_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197865_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197866_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197866_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197875_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197875_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:54:37.45 +54:37:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197879_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197879_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:16:52.52 +54:00:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197882_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197882_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197883_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197883_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197888_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197888_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197889_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197889_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197892_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197892_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197894_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197894_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197897_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197897_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197899_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197899_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197905_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197905_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197908_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197908_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197910_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197910_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197913_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197913_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197915_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197915_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197928_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 197928_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 197933_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197933_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:06:09.86 +55:15:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197936_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197936_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197941_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197941_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197943_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197943_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197944_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197944_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197948_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197948_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197952_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197952_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197954_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197954_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197957_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197957_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197958_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197958_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:57:42.99 +53:44:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197960_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197960_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197964_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197964_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 197966_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197966_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197967_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197967_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197968_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197968_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197970_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197970_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197978_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197978_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197982_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197982_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197984_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197984_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 197986_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197986_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197987_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197987_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197989_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197989_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197991_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197991_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197993_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197993_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197999_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 197999_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198002_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198002_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198007_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198007_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198008_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198008_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:12:48.60 +53:14:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198009_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198009_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 198011_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198011_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198021_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198021_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198026_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198026_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:09:23.88 +58:04:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198027_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198027_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198030_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198030_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198032_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198032_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:25:46.78 +52:37:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198036_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198036_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:07:11.69 +56:33:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198040_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198040_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198041_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198041_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198042_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198042_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198043_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198043_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198047_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198047_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198049_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198049_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198052_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198052_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198068_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198068_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:11:58.05 +57:59:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198070_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198070_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198075_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198075_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198088_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198088_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198089_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198089_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198091_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198091_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198092_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198092_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198094_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198094_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198095_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198095_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198096_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198096_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198098_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198098_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:14:57.08 +55:15:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198100_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198100_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:56:59.77 +56:42:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198101_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198101_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198107_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198107_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198110_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198110_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198114_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198114_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198121_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198121_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198123_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198123_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198127_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198127_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:46:13.91 +51:16:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198129_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198129_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (27.0") between the two second-epoch detections
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Considering the candidate 198139_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198139_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198140_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198140_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198141_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198141_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198143_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198143_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198146_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198146_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198147_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198147_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198151_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198151_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198152_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198152_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198154_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198154_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198155_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198155_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198156_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198156_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198157_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198157_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198159_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198159_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198164_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198164_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198178_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198178_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198179_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198179_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 198183_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198183_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198187_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198187_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198188_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198188_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198190_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198190_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198191_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198191_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198196_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198196_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198198_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198198_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198202_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198202_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198204_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198204_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198206_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198206_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198210_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198210_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198218_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198218_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198219_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198219_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198220_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198220_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198235_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198235_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198237_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198237_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198238_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198238_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198239_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198239_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198240_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198240_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198242_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198242_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198250_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198250_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198253_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198253_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198260_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198260_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198266_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198266_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198268_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198268_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (40.4") between the two second-epoch detections
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Considering the candidate 198271_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198271_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198278_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198278_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198279_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198279_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198281_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198281_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198283_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198283_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198286_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198286_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198287_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198287_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198289_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198289_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198290_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198290_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198295_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198295_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198296_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198296_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198298_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198298_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198304_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198304_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198306_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198306_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198308_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198308_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198313_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198313_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:42:05.35 +53:06:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198317_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198317_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198319_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198319_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198323_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198323_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198324_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198324_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198329_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198329_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198331_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198331_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198333_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198333_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198334_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198334_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198335_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198335_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198339_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198339_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198340_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198340_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198341_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198341_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198344_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198344_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198345_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198345_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198347_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198347_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198348_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198348_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198349_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198349_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198352_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198352_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198358_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198358_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198361_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198361_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (31.5") between the two second-epoch detections
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Considering the candidate 198362_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198362_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198363_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198363_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198367_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198367_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198368_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198368_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198370_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198370_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198373_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198373_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198375_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198375_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198376_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198376_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198377_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198377_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198382_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198382_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198386_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198386_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198387_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198387_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:13:58.30 +54:31:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 5.259 1996426457048514432 348.49045835252 +54.53018478149 15.0192 14.3197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198389_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198389_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198391_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198391_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198393_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198393_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198395_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198395_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198397_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198397_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198399_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198399_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198400_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198400_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198402_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198402_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198403_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198403_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198404_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198404_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198408_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198408_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198410_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198410_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198411_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198411_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198413_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198413_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198415_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198415_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198417_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198417_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198418_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198418_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198420_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198420_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198421_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198421_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198423_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198423_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198425_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198425_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198426_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198426_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198428_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198428_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198430_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198430_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198431_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198431_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198433_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198433_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198434_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198434_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198435_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198435_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198436_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198436_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198438_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198438_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198439_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198439_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198440_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198440_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198441_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198441_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198446_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198446_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198448_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198448_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198456_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198456_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:13:19.01 +52:50:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198457_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198457_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198462_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198462_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198467_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198467_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198468_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198468_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198470_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198470_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198471_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198471_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198472_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198472_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198473_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198473_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198474_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198474_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198476_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198476_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198478_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198478_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198487_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198487_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198497_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198497_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198498_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198498_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198500_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198500_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198501_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198501_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:55:39.15 +51:16:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198502_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198502_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198509_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198509_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198510_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198510_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:20:10.45 +55:06:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198512_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198512_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198513_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198513_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198514_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198514_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198516_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198516_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198518_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198518_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (33.2") between the two second-epoch detections
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Considering the candidate 198519_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198519_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198521_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198521_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198522_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198522_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198525_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198525_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198526_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198526_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198527_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198527_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198532_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198532_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198533_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198533_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198536_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198536_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198539_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198539_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198547_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198547_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198550_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198550_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198556_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198556_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198559_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198559_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198561_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198561_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198564_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198564_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198565_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198565_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198566_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198566_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198572_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198572_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198573_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198573_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198574_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198574_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198575_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198575_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198580_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198580_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198581_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198581_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198589_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198589_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198590_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198590_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198592_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198592_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198596_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198596_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198599_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198599_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198605_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198605_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198611_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198611_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198612_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198612_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198613_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198613_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198615_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198615_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198616_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198616_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198618_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198618_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198620_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198620_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198622_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198622_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198623_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198623_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198629_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198629_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198630_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198630_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198631_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198631_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198634_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198634_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198635_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198635_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:01:17.25 +52:54:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198637_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198637_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198642_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198642_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198644_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198644_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198646_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198646_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198649_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198649_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198656_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198656_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198657_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198657_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198658_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198658_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198661_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198661_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198662_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198662_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198663_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198663_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198664_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198664_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198668_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198668_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198670_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198670_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198671_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198671_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198675_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198675_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198676_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198676_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198679_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198679_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198682_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198682_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:24:23.47 +52:00:37.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 198686_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198686_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198691_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198691_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198692_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198692_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:25:06.07 +54:14:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198695_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198695_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198700_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198700_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198701_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198701_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198707_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198707_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198709_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198709_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198710_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198710_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198711_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198711_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198713_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198713_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198715_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198715_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198718_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198718_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198719_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198719_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198720_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198720_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198721_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198721_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198722_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198722_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198724_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198724_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198732_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198732_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198736_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198736_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198741_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198741_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198745_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198745_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198748_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198748_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198751_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198751_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198752_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198752_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198753_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198753_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198755_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198755_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198762_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198762_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198764_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198764_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198767_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198767_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198768_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198768_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198769_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198769_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198770_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198770_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198773_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198773_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198777_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198777_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198778_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198778_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198783_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198783_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198791_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198791_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198792_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198792_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198796_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198796_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198799_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198799_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198801_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198801_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198803_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198803_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198804_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198804_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198805_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198805_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198812_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198812_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198813_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198813_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198814_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198814_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198815_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198815_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198818_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198818_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198820_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198820_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198821_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198821_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198822_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198822_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198823_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198823_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198827_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198827_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198828_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198828_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198829_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198829_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198830_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198830_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198832_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198832_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198834_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198834_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198835_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198835_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198836_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198836_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198837_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198837_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198840_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198840_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198842_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198842_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198846_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198846_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198847_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198847_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198848_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198848_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198849_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198849_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198859_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198859_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198861_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198861_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198862_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198862_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198864_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198864_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198865_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198865_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198866_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198866_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198869_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198869_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 198875_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198875_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198877_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198877_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198880_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198880_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198881_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198881_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198883_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198883_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198884_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198884_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198888_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198888_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198890_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198890_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198894_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198894_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198895_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198895_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198896_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198896_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198897_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198897_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198899_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198899_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198903_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198903_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198904_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198904_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198905_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198905_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198911_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198911_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198913_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198913_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198918_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198918_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 198928_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198928_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198931_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198931_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198932_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198932_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198935_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198935_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198937_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198937_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198941_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198941_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198942_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198942_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198943_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198943_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198945_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198945_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198954_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198954_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198959_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198959_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198960_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198960_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198962_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198962_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198963_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198963_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198970_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198970_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198972_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198972_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198975_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198975_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198984_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198984_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198990_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 198990_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198991_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198991_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198992_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198992_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 198997_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 198997_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199000_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199000_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199003_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199003_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199004_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199004_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199005_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199005_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199008_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199008_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199014_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199014_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199017_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199017_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199023_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199023_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199025_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199025_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199026_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199026_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199028_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199028_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199031_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199031_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199033_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199033_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199036_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199036_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199038_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199038_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199039_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199039_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199058_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199058_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199061_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199061_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199065_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199065_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199069_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199069_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199071_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199071_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
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Considering the candidate 199075_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199075_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199081_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199081_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199093_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199093_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199094_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199094_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199095_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199095_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199101_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199101_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199102_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199102_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199104_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199104_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (28.1") between the two second-epoch detections
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Considering the candidate 199105_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199105_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199111_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199111_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199113_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199113_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199116_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199116_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199125_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199125_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199127_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199127_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199129_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199129_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199131_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199131_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199134_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199134_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199140_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199140_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199152_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199152_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199156_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199156_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199157_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199157_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199158_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199158_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199159_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199159_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199160_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199160_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199162_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199162_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199164_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199164_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199166_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199166_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199168_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199168_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199169_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199169_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199176_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199176_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199177_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199177_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199181_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199181_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199182_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199182_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199184_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199184_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199185_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199185_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199187_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199187_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199191_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199191_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199197_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199197_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199220_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199220_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199228_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199228_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199244_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199244_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199247_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199247_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199250_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199250_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199252_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199252_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199268_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199268_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199270_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199270_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199271_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199271_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199272_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199272_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199274_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199274_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199275_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199275_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199278_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199278_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199284_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199284_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199286_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199286_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199292_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199292_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199293_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199293_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199297_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199297_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199305_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199305_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199311_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199311_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199316_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199316_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199324_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199324_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199327_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199327_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199330_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199330_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199356_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199356_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199361_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199361_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199364_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199364_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199366_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199366_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199372_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199372_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199374_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199374_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199375_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199375_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199379_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199379_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199393_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199393_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199396_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199396_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199397_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199397_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199411_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199411_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199416_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199416_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199420_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199420_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199425_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199425_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199426_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199426_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199427_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199427_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199428_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199428_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199434_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199434_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199438_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199438_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199444_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199444_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199448_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199448_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199454_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199454_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (31.6") between the two second-epoch detections
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Considering the candidate 199455_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199455_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199456_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199456_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199464_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199464_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199467_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199467_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:57:36.26 +56:44:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199472_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199472_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199473_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199473_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199477_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199477_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199483_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199483_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199489_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199489_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199498_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199498_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 199504_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199504_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199507_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199507_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199518_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199518_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199520_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199520_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199523_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199523_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199524_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199524_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199531_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199531_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199533_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199533_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199546_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199546_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199553_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199553_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199561_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199561_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199569_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199569_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199580_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199580_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199583_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199583_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199590_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199590_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199598_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199598_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199603_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199603_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199606_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199606_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199607_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199607_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199609_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199609_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199611_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199611_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199617_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199617_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199627_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199627_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199629_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199629_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199631_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199631_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199632_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199632_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 199633_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199633_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199634_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199634_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199651_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199651_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199660_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199660_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199661_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199661_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199671_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199671_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199673_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199673_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199675_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199675_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (25.9") between the two second-epoch detections
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Considering the candidate 199697_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199697_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199700_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199700_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199701_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199701_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199703_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199703_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199707_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199707_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199711_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199711_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199721_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199721_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 199726_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199726_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199747_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199747_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199758_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199758_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199759_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199759_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199760_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199760_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199762_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199762_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199767_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199767_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199772_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199772_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199779_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199779_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199795_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199795_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199799_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199799_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199800_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199800_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199812_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199812_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199831_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199831_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199836_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199836_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199837_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199837_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199852_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199852_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199860_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199860_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199863_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199863_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199874_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199874_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199875_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199875_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199878_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199878_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199889_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199889_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199894_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199894_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (40.9") between the two second-epoch detections
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Considering the candidate 199899_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199899_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199904_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199904_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199912_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199912_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199919_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199919_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199920_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199920_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199930_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199930_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199935_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199935_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199942_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199942_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199950_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199950_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199960_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199960_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199969_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 199969_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199970_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199970_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 199977_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199977_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 199993_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 199993_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200000_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200000_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 200005_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200005_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200015_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200015_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200020_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200020_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200042_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200042_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 200056_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200056_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200067_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200067_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200074_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200074_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 200077_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200077_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200098_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200098_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200099_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200099_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200106_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200106_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200107_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200107_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200109_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200109_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200129_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200129_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200148_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200148_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200149_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200149_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200152_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200152_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200162_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200162_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200177_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200177_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 200194_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200194_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 200202_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200202_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200218_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200218_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 200233_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200233_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 200263_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200263_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200280_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200280_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200286_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200286_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 200290_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200290_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200298_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200298_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200353_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200353_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200356_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200356_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200360_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200360_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200378_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200378_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200387_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200387_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200438_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200438_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200440_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200440_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200453_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200453_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 200461_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200461_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200531_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200531_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200595_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200595_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200633_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200633_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200666_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200666_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200725_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200725_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200761_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200761_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200772_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200772_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200881_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 200881_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 200896_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200896_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200920_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200920_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200928_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200928_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 200953_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200953_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
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Considering the candidate 200982_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 200982_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 201071_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 201071_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 201191_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 201191_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 201270_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 201270_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 201486_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 201486_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 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 102558_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
Preparing report for the candidate 102558_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
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Considering the candidate 170697_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 170697_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:15:50.48 +57:32:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93929_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 93929_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:49:13.31 +54:54:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140319_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 140319_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 00:19:59.20 +56:35:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16337_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096
The candidate 16337_fd_Cas-04-Q2b1x1_2026-09-09_01-14-33_20.00sec_0.00C_LIGHT_0096 did not pass the final checks
**** FOUND 23:21:11.60 +50:00:11.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 27s
make_report_in_HTML.sh TOTAL: 647s
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 ####
23:43:47.21 +58:01:11.0
23:31:14.93 +54:16:11.9
23:23:47.40 +54:32:06.3
23:39:43.59 +57:07:19.3
00:26:43.55 +50:38:16.8
23:23:26.83 +55:05:04.9
23:48:15.65 +57:52:36.7
23:44:13.98 +57:45:24.9
23:28:42.59 +57:11:03.1
23:34:42.99 +57:22:12.9
23:39:42.20 +55:51:27.0
23:13:58.82 +53:19:37.0
23:33:57.82 +55:18:00.7
23:16:39.91 +56:29:27.8
23:16:01.56 +55:36:22.2
23:15:47.76 +54:58:14.9
23:25:15.17 +56:00:10.4
23:32:31.21 +55:27:33.1
23:45:44.54 +57:58:28.6
23:17:28.43 +53:27:01.5
23:27:32.52 +54:43:03.7
23:18:23.18 +52:39:51.7
23:15:38.74 +53:18:33.4
23:17:34.14 +53:34:44.7
23:23:51.71 +56:20:24.8
23:16:19.40 +54:47:52.9
23:29:25.81 +54:56:43.2
23:15:00.68 +55:27:37.5
23:44:03.56 +57:40:10.8
23:32:13.05 +54:36:49.8
23:22:25.15 +55:31:37.9
23:32:03.93 +56:47:02.7
23:23:32.97 +54:29:59.7
23:21:26.83 +54:07:11.5
23:34:49.87 +54:52:42.5
23:37:22.76 +57:07:09.6
23:19:56.60 +56:53:58.7
23:24:50.08 +57:00:22.7
23:14:54.27 +55:00:57.8
23:36:45.10 +57:01:41.5
23:14:30.31 +55:30:20.3
23:33:48.63 +55:44:18.1
23:23:09.89 +52:36:00.7
23:19:54.88 +54:33:51.7
23:27:51.82 +57:07:05.0
23:19:25.45 +56:55:07.4
23:18:08.89 +56:55:36.0
23:33:46.97 +56:23:25.9
23:25:09.08 +55:35:12.3
23:29:44.72 +55:16:19.1
23:14:18.36 +54:02:54.6
23:17:36.98 +52:53:25.7
23:16:33.42 +56:59:47.7
23:21:45.86 +54:25:14.4
23:34:25.78 +54:29:17.4
23:21:35.97 +52:15:13.3
23:17:54.28 +55:27:35.5
23:25:12.74 +54:23:17.1
23:18:20.22 +52:39:22.6
23:14:25.46 +53:35:42.3
23:37:34.22 +55:28:31.4
23:26:55.39 +57:19:49.3
23:13:47.45 +56:30:59.2
23:21:14.77 +54:14:41.7
23:32:57.84 +55:20:35.9
23:16:51.96 +54:13:37.3
23:35:58.96 +54:45:35.1
23:26:07.61 +57:14:57.4
23:31:32.30 +54:31:32.9
23:15:19.57 +56:28:53.9
23:13:58.59 +56:31:17.4
23:42:06.81 +57:58:08.8
23:16:30.27 +53:08:44.7
23:25:53.49 +55:45:47.2
23:32:21.04 +56:19:24.7
23:21:21.42 +56:54:37.7
23:45:57.96 +57:31:58.3
23:17:37.23 +51:54:22.0
23:27:57.66 +55:37:44.4
23:15:16.56 +53:02:09.3
23:44:44.22 +57:54:11.1
23:45:58.71 +56:57:42.7
23:29:41.45 +55:55:24.8
23:19:39.77 +55:04:10.7
23:19:48.73 +52:55:01.9
23:18:08.05 +53:41:11.3
23:32:36.20 +55:07:12.7
23:22:07.86 +54:45:26.6
23:18:06.95 +55:05:34.2
23:23:10.72 +56:57:08.7
23:16:20.46 +52:05:57.6
23:35:43.23 +54:55:15.1
23:26:02.49 +55:37:17.4
23:19:35.83 +54:10:39.1
23:16:25.10 +54:01:09.4
23:17:11.07 +53:36:00.8
23:30:41.40 +55:31:43.5
23:20:27.83 +51:25:08.0
23:17:08.15 +53:54:15.9
23:14:39.23 +54:17:58.8
23:18:33.81 +55:52:09.0
23:14:09.14 +56:26:10.1
23:40:01.78 +56:50:24.8
23:27:25.75 +53:28:43.0
23:16:22.30 +53:52:52.6
23:27:25.75 +56:43:28.8
23:13:32.11 +54:36:44.4
23:35:55.50 +54:52:45.0
23:14:34.44 +55:57:47.9
23:14:15.61 +53:53:54.8
23:28:14.02 +57:41:39.9
23:47:29.00 +57:54:32.3
23:38:31.97 +56:57:45.4
23:32:02.00 +54:33:58.2
23:17:11.07 +56:03:01.7
23:11:46.64 +55:24:34.7
23:23:03.31 +55:20:04.8
23:13:56.59 +54:17:45.0
23:14:34.19 +57:04:36.0
23:27:59.89 +56:00:06.1
23:16:35.08 +56:46:41.8
23:26:18.51 +55:19:51.5
23:30:01.22 +55:54:14.2
23:30:15.05 +55:35:38.9
23:14:30.40 +53:29:10.0
23:37:47.13 +58:01:32.6
23:36:17.30 +58:00:14.4
23:43:53.25 +57:35:52.5
23:24:48.05 +56:02:35.3
23:26:39.23 +55:39:34.7
23:18:42.39 +54:57:41.2
23:20:45.16 +55:50:06.0
23:13:55.38 +55:27:50.3
00:26:17.02 +49:45:32.0
23:15:13.69 +52:09:41.4
23:46:40.40 +57:42:14.9
23:18:01.30 +54:07:27.0
23:16:09.31 +53:48:25.6
23:21:55.39 +54:35:42.1
23:15:15.23 +53:51:11.9
23:32:32.93 +56:41:23.6
23:14:58.02 +56:01:19.0
23:28:13.78 +55:31:06.4
23:15:45.35 +54:47:50.6
23:11:24.30 +55:58:54.2
23:29:17.34 +54:35:12.9
23:44:16.96 +57:55:31.4
23:16:02.19 +52:58:01.9
23:14:32.70 +54:44:09.1
23:42:31.53 +56:49:09.8
23:21:31.31 +54:25:20.0
23:33:18.72 +56:16:57.8
23:13:29.33 +56:55:19.7
23:41:06.84 +56:50:15.3
23:19:18.64 +55:23:09.6
23:13:32.44 +55:15:28.7
23:13:03.08 +55:43:03.2
23:33:01.40 +54:38:42.6
23:53:22.36 +57:55:41.8
23:18:01.69 +54:03:48.9
23:12:34.49 +54:39:40.3
23:36:43.70 +57:59:50.0
23:15:12.47 +52:13:25.3
23:41:09.50 +56:50:24.5
23:14:50.04 +55:24:50.9
23:20:07.23 +55:43:22.5
23:14:23.65 +52:58:53.0
23:21:58.57 +54:52:10.1
23:19:10.89 +54:25:33.4
23:30:53.67 +55:01:29.5
23:19:38.69 +54:49:13.9
23:27:38.62 +57:03:07.5
23:34:15.18 +54:35:52.2
23:19:38.83 +54:22:29.4
23:17:54.85 +54:02:55.7
23:10:45.12 +56:08:16.7
23:15:05.48 +52:30:01.7
23:14:46.10 +57:01:34.0
23:14:46.63 +52:54:55.4
23:22:45.33 +52:22:47.1
23:20:26.01 +52:26:49.9
23:13:36.12 +55:38:46.1
23:26:51.40 +54:14:40.4
23:15:12.70 +53:15:41.0
23:15:37.17 +54:22:36.2
23:11:47.56 +55:27:46.1
23:26:53.36 +56:25:56.4
23:15:49.23 +52:50:40.9
23:30:06.24 +54:42:16.8
23:13:04.73 +56:43:23.7
23:15:17.99 +53:29:56.8
23:43:25.89 +57:58:09.1
23:19:31.01 +53:07:24.0
23:12:47.55 +54:41:56.4
23:21:29.40 +56:15:30.1
23:18:01.81 +53:42:03.7
23:36:08.16 +54:50:06.8
23:36:58.43 +54:29:57.6
23:25:04.57 +55:52:06.1
23:15:41.21 +53:21:41.6
23:14:43.64 +54:44:02.1
23:16:21.53 +53:04:54.1
23:31:52.24 +55:24:25.2
23:42:19.27 +56:52:00.2
23:27:13.16 +54:36:25.8
23:26:12.98 +55:30:59.2
23:31:02.76 +54:13:33.3
23:30:42.74 +54:58:05.5
23:17:53.18 +53:53:03.8
23:19:07.36 +55:41:18.2
23:31:38.06 +54:52:04.7
23:24:23.81 +56:17:15.3
23:17:35.25 +54:40:53.9
23:22:05.30 +52:39:33.0
23:26:37.11 +55:28:49.0
23:27:34.12 +54:33:50.7
23:15:17.13 +54:04:35.0
23:17:56.25 +55:25:42.4
23:24:51.30 +56:17:42.2
23:35:23.98 +56:20:57.3
23:43:35.21 +57:49:28.1
23:45:32.20 +57:23:44.0
23:44:20.54 +56:48:40.2
23:20:38.48 +52:15:03.9
23:36:00.61 +54:33:04.0
23:27:08.57 +57:56:28.7
23:19:16.70 +55:34:13.3
23:30:06.03 +54:28:15.6
23:15:12.87 +54:11:50.9
23:17:55.05 +54:18:14.4
23:13:56.50 +55:25:37.8
23:30:17.98 +54:25:55.5
23:12:34.34 +54:40:14.3
23:21:26.77 +51:25:56.2
23:19:56.24 +54:56:35.5
23:15:39.76 +54:30:28.8
23:15:58.54 +54:10:16.7
23:15:53.87 +57:02:25.2
23:29:11.22 +55:12:46.5
23:15:49.17 +54:42:21.6
23:17:45.41 +56:54:51.5
23:19:25.33 +55:38:48.2
23:15:35.46 +52:09:47.5
23:14:31.80 +53:50:27.8
23:27:37.01 +56:15:56.3
23:18:41.56 +54:46:21.0
23:22:21.61 +56:29:36.7
23:12:59.22 +55:34:38.1
23:12:18.99 +55:16:00.9
########### Completed Cas-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
23:43:47.21 +58:01:11.0
23:31:14.93 +54:16:11.9
23:23:47.40 +54:32:06.3
23:39:43.59 +57:07:19.3
00:26:43.55 +50:38:16.8
23:23:26.83 +55:05:04.9
23:48:15.65 +57:52:36.7
23:44:13.98 +57:45:24.9
23:28:42.59 +57:11:03.1
23:34:42.99 +57:22:12.9
23:39:42.20 +55:51:27.0
23:13:58.82 +53:19:37.0
23:16:39.91 +56:29:27.8
23:16:01.56 +55:36:22.2
23:15:47.76 +54:58:14.9
23:25:15.17 +56:00:10.4
23:32:31.21 +55:27:33.1
23:45:44.54 +57:58:28.6
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23:27:32.52 +54:43:03.7
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23:23:51.71 +56:20:24.8
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23:44:03.56 +57:40:10.8
23:32:13.05 +54:36:49.8
23:22:25.15 +55:31:37.9
23:32:03.93 +56:47:02.7
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23:21:26.83 +54:07:11.5
23:34:49.87 +54:52:42.5
23:37:22.76 +57:07:09.6
23:19:56.60 +56:53:58.7
23:24:50.08 +57:00:22.7
23:14:54.27 +55:00:57.8
23:36:45.10 +57:01:41.5
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23:33:48.63 +55:44:18.1
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23:27:51.82 +57:07:05.0
23:19:25.45 +56:55:07.4
23:18:08.89 +56:55:36.0
23:33:46.97 +56:23:25.9
23:25:09.08 +55:35:12.3
23:29:44.72 +55:16:19.1
23:14:18.36 +54:02:54.6
23:17:36.98 +52:53:25.7
23:16:33.42 +56:59:47.7
23:21:45.86 +54:25:14.4
23:34:25.78 +54:29:17.4
23:21:35.97 +52:15:13.3
23:17:54.28 +55:27:35.5
23:25:12.74 +54:23:17.1
23:18:20.22 +52:39:22.6
23:14:25.46 +53:35:42.3
23:37:34.22 +55:28:31.4
23:26:55.39 +57:19:49.3
23:13:47.45 +56:30:59.2
23:21:14.77 +54:14:41.7
23:32:57.84 +55:20:35.9
23:16:51.96 +54:13:37.3
23:35:58.96 +54:45:35.1
23:26:07.61 +57:14:57.4
23:31:32.30 +54:31:32.9
23:15:19.57 +56:28:53.9
23:13:58.59 +56:31:17.4
23:42:06.81 +57:58:08.8
23:16:30.27 +53:08:44.7
23:25:53.49 +55:45:47.2
23:32:21.04 +56:19:24.7
23:21:21.42 +56:54:37.7
23:45:57.96 +57:31:58.3
23:17:37.23 +51:54:22.0
23:27:57.66 +55:37:44.4
23:15:16.56 +53:02:09.3
23:44:44.22 +57:54:11.1
23:45:58.71 +56:57:42.7
23:29:41.45 +55:55:24.8
23:19:39.77 +55:04:10.7
23:19:48.73 +52:55:01.9
23:18:08.05 +53:41:11.3
23:32:36.20 +55:07:12.7
23:22:07.86 +54:45:26.6
23:18:06.95 +55:05:34.2
23:23:10.72 +56:57:08.7
23:16:20.46 +52:05:57.6
23:35:43.23 +54:55:15.1
23:26:02.49 +55:37:17.4
23:19:35.83 +54:10:39.1
23:16:25.10 +54:01:09.4
23:17:11.07 +53:36:00.8
23:30:41.40 +55:31:43.5
23:20:27.83 +51:25:08.0
23:17:08.15 +53:54:15.9
23:14:39.23 +54:17:58.8
23:18:33.81 +55:52:09.0
23:14:09.14 +56:26:10.1
23:40:01.78 +56:50:24.8
23:27:25.75 +53:28:43.0
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23:38:31.97 +56:57:45.4
23:32:02.00 +54:33:58.2
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23:14:34.19 +57:04:36.0
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23:26:18.51 +55:19:51.5
23:30:01.22 +55:54:14.2
23:30:15.05 +55:35:38.9
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23:37:47.13 +58:01:32.6
23:36:17.30 +58:00:14.4
23:43:53.25 +57:35:52.5
23:24:48.05 +56:02:35.3
23:26:39.23 +55:39:34.7
23:18:42.39 +54:57:41.2
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23:13:55.38 +55:27:50.3
00:26:17.02 +49:45:32.0
23:15:13.69 +52:09:41.4
23:46:40.40 +57:42:14.9
23:18:01.30 +54:07:27.0
23:16:09.31 +53:48:25.6
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23:32:32.93 +56:41:23.6
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23:28:13.78 +55:31:06.4
23:15:45.35 +54:47:50.6
23:11:24.30 +55:58:54.2
23:29:17.34 +54:35:12.9
23:44:16.96 +57:55:31.4
23:16:02.19 +52:58:01.9
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23:42:31.53 +56:49:09.8
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23:41:06.84 +56:50:15.3
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23:41:09.50 +56:50:24.5
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23:27:38.62 +57:03:07.5
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23:15:49.23 +52:50:40.9
23:30:06.24 +54:42:16.8
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23:43:25.89 +57:58:09.1
23:19:31.01 +53:07:24.0
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23:30:42.74 +54:58:05.5
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23:18:41.56 +54:46:21.0
23:22:21.61 +56:29:36.7
23:12:59.22 +55:34:38.1
23:12:18.99 +55:16:00.9
23:33:57.82 +55:18:00.7
###################################################################################
23:43:47.21 +58:01:11.0 -- not an asteroid (will add it to exclusion list)
23:31:14.93 +54:16:11.9 -- not an asteroid (will add it to exclusion list)
23:23:47.40 +54:32:06.3 -- not an asteroid (will add it to exclusion list)
23:39:43.59 +57:07:19.3 -- not an asteroid (will add it to exclusion list)
00:26:43.55 +50:38:16.8 -- not an asteroid (will add it to exclusion list)
23:23:26.83 +55:05:04.9 -- not an asteroid (will add it to exclusion list)
23:48:15.65 +57:52:36.7 -- not an asteroid (will add it to exclusion list)
23:44:13.98 +57:45:24.9 -- not an asteroid (will add it to exclusion list)
23:28:42.59 +57:11:03.1 -- not an asteroid (will add it to exclusion list)
23:34:42.99 +57:22:12.9 -- not an asteroid (will add it to exclusion list)
23:39:42.20 +55:51:27.0 -- not an asteroid (will add it to exclusion list)
23:13:58.82 +53:19:37.0 -- not an asteroid (will add it to exclusion list)
23:16:39.91 +56:29:27.8 -- not an asteroid (will add it to exclusion list)
23:16:01.56 +55:36:22.2 -- not an asteroid (will add it to exclusion list)
23:15:47.76 +54:58:14.9 -- not an asteroid (will add it to exclusion list)
23:25:15.17 +56:00:10.4 -- not an asteroid (will add it to exclusion list)
23:32:31.21 +55:27:33.1 -- not an asteroid (will add it to exclusion list)
23:45:44.54 +57:58:28.6 -- not an asteroid (will add it to exclusion list)
23:17:28.43 +53:27:01.5 -- not an asteroid (will add it to exclusion list)
23:27:32.52 +54:43:03.7 -- not an asteroid (will add it to exclusion list)
23:18:23.18 +52:39:51.7 -- not an asteroid (will add it to exclusion list)
23:15:38.74 +53:18:33.4 -- not an asteroid (will add it to exclusion list)
23:17:34.14 +53:34:44.7 -- not an asteroid (will add it to exclusion list)
23:23:51.71 +56:20:24.8 -- not an asteroid (will add it to exclusion list)
23:16:19.40 +54:47:52.9 -- not an asteroid (will add it to exclusion list)
23:29:25.81 +54:56:43.2 -- not an asteroid (will add it to exclusion list)
23:15:00.68 +55:27:37.5 -- not an asteroid (will add it to exclusion list)
23:44:03.56 +57:40:10.8 -- not an asteroid (will add it to exclusion list)
23:32:13.05 +54:36:49.8 -- not an asteroid (will add it to exclusion list)
23:22:25.15 +55:31:37.9 -- not an asteroid (will add it to exclusion list)
23:32:03.93 +56:47:02.7 -- not an asteroid (will add it to exclusion list)
23:23:32.97 +54:29:59.7 -- not an asteroid (will add it to exclusion list)
23:21:26.83 +54:07:11.5 -- not an asteroid (will add it to exclusion list)
23:34:49.87 +54:52:42.5 -- not an asteroid (will add it to exclusion list)
23:37:22.76 +57:07:09.6 -- not an asteroid (will add it to exclusion list)
23:19:56.60 +56:53:58.7 -- not an asteroid (will add it to exclusion list)
23:24:50.08 +57:00:22.7 -- not an asteroid (will add it to exclusion list)
23:14:54.27 +55:00:57.8 -- not an asteroid (will add it to exclusion list)
23:36:45.10 +57:01:41.5 -- not an asteroid (will add it to exclusion list)
23:14:30.31 +55:30:20.3 -- not an asteroid (will add it to exclusion list)
23:33:48.63 +55:44:18.1 -- not an asteroid (will add it to exclusion list)
23:23:09.89 +52:36:00.7 -- not an asteroid (will add it to exclusion list)
23:19:54.88 +54:33:51.7 -- not an asteroid (will add it to exclusion list)
23:27:51.82 +57:07:05.0 -- not an asteroid (will add it to exclusion list)
23:19:25.45 +56:55:07.4 -- not an asteroid (will add it to exclusion list)
23:18:08.89 +56:55:36.0 -- not an asteroid (will add it to exclusion list)
23:33:46.97 +56:23:25.9 -- not an asteroid (will add it to exclusion list)
23:25:09.08 +55:35:12.3 -- not an asteroid (will add it to exclusion list)
23:29:44.72 +55:16:19.1 -- not an asteroid (will add it to exclusion list)
23:14:18.36 +54:02:54.6 -- not an asteroid (will add it to exclusion list)
23:17:36.98 +52:53:25.7 -- not an asteroid (will add it to exclusion list)
23:16:33.42 +56:59:47.7 -- not an asteroid (will add it to exclusion list)
23:21:45.86 +54:25:14.4 -- not an asteroid (will add it to exclusion list)
23:34:25.78 +54:29:17.4 -- not an asteroid (will add it to exclusion list)
23:21:35.97 +52:15:13.3 -- not an asteroid (will add it to exclusion list)
23:17:54.28 +55:27:35.5 -- not an asteroid (will add it to exclusion list)
23:25:12.74 +54:23:17.1 -- not an asteroid (will add it to exclusion list)
23:18:20.22 +52:39:22.6 -- not an asteroid (will add it to exclusion list)
23:14:25.46 +53:35:42.3 -- not an asteroid (will add it to exclusion list)
23:37:34.22 +55:28:31.4 -- not an asteroid (will add it to exclusion list)
23:26:55.39 +57:19:49.3 -- not an asteroid (will add it to exclusion list)
23:13:47.45 +56:30:59.2 -- not an asteroid (will add it to exclusion list)
23:21:14.77 +54:14:41.7 -- not an asteroid (will add it to exclusion list)
23:32:57.84 +55:20:35.9 -- not an asteroid (will add it to exclusion list)
23:16:51.96 +54:13:37.3 -- not an asteroid (will add it to exclusion list)
23:35:58.96 +54:45:35.1 -- not an asteroid (will add it to exclusion list)
23:26:07.61 +57:14:57.4 -- not an asteroid (will add it to exclusion list)
23:31:32.30 +54:31:32.9 -- not an asteroid (will add it to exclusion list)
23:15:19.57 +56:28:53.9 -- not an asteroid (will add it to exclusion list)
23:13:58.59 +56:31:17.4 -- not an asteroid (will add it to exclusion list)
23:42:06.81 +57:58:08.8 -- not an asteroid (will add it to exclusion list)
23:16:30.27 +53:08:44.7 -- not an asteroid (will add it to exclusion list)
23:25:53.49 +55:45:47.2 -- not an asteroid (will add it to exclusion list)
23:32:21.04 +56:19:24.7 -- not an asteroid (will add it to exclusion list)
23:21:21.42 +56:54:37.7 -- not an asteroid (will add it to exclusion list)
23:45:57.96 +57:31:58.3 -- not an asteroid (will add it to exclusion list)
23:17:37.23 +51:54:22.0 -- not an asteroid (will add it to exclusion list)
23:27:57.66 +55:37:44.4 -- not an asteroid (will add it to exclusion list)
23:15:16.56 +53:02:09.3 -- not an asteroid (will add it to exclusion list)
23:44:44.22 +57:54:11.1 -- not an asteroid (will add it to exclusion list)
23:45:58.71 +56:57:42.7 -- not an asteroid (will add it to exclusion list)
23:29:41.45 +55:55:24.8 -- not an asteroid (will add it to exclusion list)
23:19:39.77 +55:04:10.7 -- not an asteroid (will add it to exclusion list)
23:19:48.73 +52:55:01.9 -- not an asteroid (will add it to exclusion list)
23:18:08.05 +53:41:11.3 -- not an asteroid (will add it to exclusion list)
23:32:36.20 +55:07:12.7 -- not an asteroid (will add it to exclusion list)
23:22:07.86 +54:45:26.6 -- not an asteroid (will add it to exclusion list)
23:18:06.95 +55:05:34.2 -- not an asteroid (will add it to exclusion list)
23:23:10.72 +56:57:08.7 -- not an asteroid (will add it to exclusion list)
23:16:20.46 +52:05:57.6 -- not an asteroid (will add it to exclusion list)
23:35:43.23 +54:55:15.1 -- not an asteroid (will add it to exclusion list)
23:26:02.49 +55:37:17.4 -- not an asteroid (will add it to exclusion list)
23:19:35.83 +54:10:39.1 -- not an asteroid (will add it to exclusion list)
23:16:25.10 +54:01:09.4 -- not an asteroid (will add it to exclusion list)
23:17:11.07 +53:36:00.8 -- not an asteroid (will add it to exclusion list)
23:30:41.40 +55:31:43.5 -- not an asteroid (will add it to exclusion list)
23:20:27.83 +51:25:08.0 -- not an asteroid (will add it to exclusion list)
23:17:08.15 +53:54:15.9 -- not an asteroid (will add it to exclusion list)
23:14:39.23 +54:17:58.8 -- not an asteroid (will add it to exclusion list)
23:18:33.81 +55:52:09.0 -- not an asteroid (will add it to exclusion list)
23:14:09.14 +56:26:10.1 -- not an asteroid (will add it to exclusion list)
23:40:01.78 +56:50:24.8 -- not an asteroid (will add it to exclusion list)
23:27:25.75 +53:28:43.0 -- not an asteroid (will add it to exclusion list)
23:16:22.30 +53:52:52.6 -- not an asteroid (will add it to exclusion list)
23:27:25.75 +56:43:28.8 -- not an asteroid (will add it to exclusion list)
23:13:32.11 +54:36:44.4 -- not an asteroid (will add it to exclusion list)
23:35:55.50 +54:52:45.0 -- not an asteroid (will add it to exclusion list)
23:14:34.44 +55:57:47.9 -- not an asteroid (will add it to exclusion list)
23:14:15.61 +53:53:54.8 -- not an asteroid (will add it to exclusion list)
23:28:14.02 +57:41:39.9 -- not an asteroid (will add it to exclusion list)
23:47:29.00 +57:54:32.3 -- not an asteroid (will add it to exclusion list)
23:38:31.97 +56:57:45.4 -- not an asteroid (will add it to exclusion list)
23:32:02.00 +54:33:58.2 -- not an asteroid (will add it to exclusion list)
23:17:11.07 +56:03:01.7 -- not an asteroid (will add it to exclusion list)
23:11:46.64 +55:24:34.7 -- not an asteroid (will add it to exclusion list)
23:23:03.31 +55:20:04.8 -- not an asteroid (will add it to exclusion list)
23:13:56.59 +54:17:45.0 -- not an asteroid (will add it to exclusion list)
23:14:34.19 +57:04:36.0 -- not an asteroid (will add it to exclusion list)
23:27:59.89 +56:00:06.1 -- not an asteroid (will add it to exclusion list)
23:16:35.08 +56:46:41.8 -- not an asteroid (will add it to exclusion list)
23:26:18.51 +55:19:51.5 -- not an asteroid (will add it to exclusion list)
23:30:01.22 +55:54:14.2 -- not an asteroid (will add it to exclusion list)
23:30:15.05 +55:35:38.9 -- not an asteroid (will add it to exclusion list)
23:14:30.40 +53:29:10.0 -- not an asteroid (will add it to exclusion list)
23:37:47.13 +58:01:32.6 -- not an asteroid (will add it to exclusion list)
23:36:17.30 +58:00:14.4 -- not an asteroid (will add it to exclusion list)
23:43:53.25 +57:35:52.5 -- not an asteroid (will add it to exclusion list)
23:24:48.05 +56:02:35.3 -- not an asteroid (will add it to exclusion list)
23:26:39.23 +55:39:34.7 -- not an asteroid (will add it to exclusion list)
23:18:42.39 +54:57:41.2 -- not an asteroid (will add it to exclusion list)
23:20:45.16 +55:50:06.0 -- not an asteroid (will add it to exclusion list)
23:13:55.38 +55:27:50.3 -- not an asteroid (will add it to exclusion list)
00:26:17.02 +49:45:32.0 -- not an asteroid (will add it to exclusion list)
23:15:13.69 +52:09:41.4 -- not an asteroid (will add it to exclusion list)
23:46:40.40 +57:42:14.9 -- not an asteroid (will add it to exclusion list)
23:18:01.30 +54:07:27.0 -- not an asteroid (will add it to exclusion list)
23:16:09.31 +53:48:25.6 -- not an asteroid (will add it to exclusion list)
23:21:55.39 +54:35:42.1 -- not an asteroid (will add it to exclusion list)
23:15:15.23 +53:51:11.9 -- not an asteroid (will add it to exclusion list)
23:32:32.93 +56:41:23.6 -- not an asteroid (will add it to exclusion list)
23:14:58.02 +56:01:19.0 -- not an asteroid (will add it to exclusion list)
23:28:13.78 +55:31:06.4 -- not an asteroid (will add it to exclusion list)
23:15:45.35 +54:47:50.6 -- not an asteroid (will add it to exclusion list)
23:11:24.30 +55:58:54.2 -- not an asteroid (will add it to exclusion list)
23:29:17.34 +54:35:12.9 -- not an asteroid (will add it to exclusion list)
23:44:16.96 +57:55:31.4 -- not an asteroid (will add it to exclusion list)
23:16:02.19 +52:58:01.9 -- not an asteroid (will add it to exclusion list)
23:14:32.70 +54:44:09.1 -- not an asteroid (will add it to exclusion list)
23:42:31.53 +56:49:09.8 -- not an asteroid (will add it to exclusion list)
23:21:31.31 +54:25:20.0 -- not an asteroid (will add it to exclusion list)
23:33:18.72 +56:16:57.8 -- not an asteroid (will add it to exclusion list)
23:13:29.33 +56:55:19.7 -- not an asteroid (will add it to exclusion list)
23:41:06.84 +56:50:15.3 -- not an asteroid (will add it to exclusion list)
23:19:18.64 +55:23:09.6 -- not an asteroid (will add it to exclusion list)
23:13:32.44 +55:15:28.7 -- not an asteroid (will add it to exclusion list)
23:13:03.08 +55:43:03.2 -- not an asteroid (will add it to exclusion list)
23:33:01.40 +54:38:42.6 -- not an asteroid (will add it to exclusion list)
23:53:22.36 +57:55:41.8 -- not an asteroid (will add it to exclusion list)
23:18:01.69 +54:03:48.9 -- not an asteroid (will add it to exclusion list)
23:12:34.49 +54:39:40.3 -- not an asteroid (will add it to exclusion list)
23:36:43.70 +57:59:50.0 -- not an asteroid (will add it to exclusion list)
23:15:12.47 +52:13:25.3 -- not an asteroid (will add it to exclusion list)
23:41:09.50 +56:50:24.5 -- not an asteroid (will add it to exclusion list)
23:14:50.04 +55:24:50.9 -- not an asteroid (will add it to exclusion list)
23:20:07.23 +55:43:22.5 -- not an asteroid (will add it to exclusion list)
23:14:23.65 +52:58:53.0 -- not an asteroid (will add it to exclusion list)
23:21:58.57 +54:52:10.1 -- not an asteroid (will add it to exclusion list)
23:19:10.89 +54:25:33.4 -- not an asteroid (will add it to exclusion list)
23:30:53.67 +55:01:29.5 -- not an asteroid (will add it to exclusion list)
23:19:38.69 +54:49:13.9 -- not an asteroid (will add it to exclusion list)
23:27:38.62 +57:03:07.5 -- not an asteroid (will add it to exclusion list)
23:34:15.18 +54:35:52.2 -- not an asteroid (will add it to exclusion list)
23:19:38.83 +54:22:29.4 -- not an asteroid (will add it to exclusion list)
23:17:54.85 +54:02:55.7 -- not an asteroid (will add it to exclusion list)
23:10:45.12 +56:08:16.7 -- not an asteroid (will add it to exclusion list)
23:15:05.48 +52:30:01.7 -- not an asteroid (will add it to exclusion list)
23:14:46.10 +57:01:34.0 -- not an asteroid (will add it to exclusion list)
23:14:46.63 +52:54:55.4 -- not an asteroid (will add it to exclusion list)
23:22:45.33 +52:22:47.1 -- not an asteroid (will add it to exclusion list)
23:20:26.01 +52:26:49.9 -- not an asteroid (will add it to exclusion list)
23:13:36.12 +55:38:46.1 -- not an asteroid (will add it to exclusion list)
23:26:51.40 +54:14:40.4 -- not an asteroid (will add it to exclusion list)
23:15:12.70 +53:15:41.0 -- not an asteroid (will add it to exclusion list)
23:15:37.17 +54:22:36.2 -- not an asteroid (will add it to exclusion list)
23:11:47.56 +55:27:46.1 -- not an asteroid (will add it to exclusion list)
23:26:53.36 +56:25:56.4 -- not an asteroid (will add it to exclusion list)
23:15:49.23 +52:50:40.9 -- not an asteroid (will add it to exclusion list)
23:30:06.24 +54:42:16.8 -- not an asteroid (will add it to exclusion list)
23:13:04.73 +56:43:23.7 -- not an asteroid (will add it to exclusion list)
23:15:17.99 +53:29:56.8 -- not an asteroid (will add it to exclusion list)
23:43:25.89 +57:58:09.1 -- not an asteroid (will add it to exclusion list)
23:19:31.01 +53:07:24.0 -- not an asteroid (will add it to exclusion list)
23:12:47.55 +54:41:56.4 -- not an asteroid (will add it to exclusion list)
23:21:29.40 +56:15:30.1 -- not an asteroid (will add it to exclusion list)
23:18:01.81 +53:42:03.7 -- not an asteroid (will add it to exclusion list)
23:36:08.16 +54:50:06.8 -- not an asteroid (will add it to exclusion list)
23:36:58.43 +54:29:57.6 -- not an asteroid (will add it to exclusion list)
23:25:04.57 +55:52:06.1 -- not an asteroid (will add it to exclusion list)
23:15:41.21 +53:21:41.6 -- not an asteroid (will add it to exclusion list)
23:14:43.64 +54:44:02.1 -- not an asteroid (will add it to exclusion list)
23:16:21.53 +53:04:54.1 -- not an asteroid (will add it to exclusion list)
23:31:52.24 +55:24:25.2 -- not an asteroid (will add it to exclusion list)
23:42:19.27 +56:52:00.2 -- not an asteroid (will add it to exclusion list)
23:27:13.16 +54:36:25.8 -- not an asteroid (will add it to exclusion list)
23:26:12.98 +55:30:59.2 -- not an asteroid (will add it to exclusion list)
23:31:02.76 +54:13:33.3 -- not an asteroid (will add it to exclusion list)
23:30:42.74 +54:58:05.5 -- not an asteroid (will add it to exclusion list)
23:17:53.18 +53:53:03.8 -- not an asteroid (will add it to exclusion list)
23:19:07.36 +55:41:18.2 -- not an asteroid (will add it to exclusion list)
23:31:38.06 +54:52:04.7 -- not an asteroid (will add it to exclusion list)
23:24:23.81 +56:17:15.3 -- not an asteroid (will add it to exclusion list)
23:17:35.25 +54:40:53.9 -- not an asteroid (will add it to exclusion list)
23:22:05.30 +52:39:33.0 -- not an asteroid (will add it to exclusion list)
23:26:37.11 +55:28:49.0 -- not an asteroid (will add it to exclusion list)
23:27:34.12 +54:33:50.7 -- not an asteroid (will add it to exclusion list)
23:15:17.13 +54:04:35.0 -- not an asteroid (will add it to exclusion list)
23:17:56.25 +55:25:42.4 -- not an asteroid (will add it to exclusion list)
23:24:51.30 +56:17:42.2 -- not an asteroid (will add it to exclusion list)
23:35:23.98 +56:20:57.3 -- not an asteroid (will add it to exclusion list)
23:43:35.21 +57:49:28.1 -- not an asteroid (will add it to exclusion list)
23:45:32.20 +57:23:44.0 -- not an asteroid (will add it to exclusion list)
23:44:20.54 +56:48:40.2 -- not an asteroid (will add it to exclusion list)
23:20:38.48 +52:15:03.9 -- not an asteroid (will add it to exclusion list)
23:36:00.61 +54:33:04.0 -- not an asteroid (will add it to exclusion list)
23:27:08.57 +57:56:28.7 -- not an asteroid (will add it to exclusion list)
23:19:16.70 +55:34:13.3 -- not an asteroid (will add it to exclusion list)
23:30:06.03 +54:28:15.6 -- not an asteroid (will add it to exclusion list)
23:15:12.87 +54:11:50.9 -- not an asteroid (will add it to exclusion list)
23:17:55.05 +54:18:14.4 -- not an asteroid (will add it to exclusion list)
23:13:56.50 +55:25:37.8 -- not an asteroid (will add it to exclusion list)
23:30:17.98 +54:25:55.5 -- not an asteroid (will add it to exclusion list)
23:12:34.34 +54:40:14.3 -- not an asteroid (will add it to exclusion list)
23:21:26.77 +51:25:56.2 -- not an asteroid (will add it to exclusion list)
23:19:56.24 +54:56:35.5 -- not an asteroid (will add it to exclusion list)
23:15:39.76 +54:30:28.8 -- not an asteroid (will add it to exclusion list)
23:15:58.54 +54:10:16.7 -- not an asteroid (will add it to exclusion list)
23:15:53.87 +57:02:25.2 -- not an asteroid (will add it to exclusion list)
23:29:11.22 +55:12:46.5 -- not an asteroid (will add it to exclusion list)
23:15:49.17 +54:42:21.6 -- not an asteroid (will add it to exclusion list)
23:17:45.41 +56:54:51.5 -- not an asteroid (will add it to exclusion list)
23:19:25.33 +55:38:48.2 -- not an asteroid (will add it to exclusion list)
23:15:35.46 +52:09:47.5 -- not an asteroid (will add it to exclusion list)
23:14:31.80 +53:50:27.8 -- not an asteroid (will add it to exclusion list)
23:27:37.01 +56:15:56.3 -- not an asteroid (will add it to exclusion list)
23:18:41.56 +54:46:21.0 -- not an asteroid (will add it to exclusion list)
23:22:21.61 +56:29:36.7 -- not an asteroid (will add it to exclusion list)
23:12:59.22 +55:34:38.1 -- not an asteroid (will add it to exclusion list)
23:12:18.99 +55:16:00.9 -- not an asteroid (will add it to exclusion list)
23:33:57.82 +55:18:00.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:26:17.02 +49:45:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:43.55 +50:38:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:10:45.12 +56:08:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:24.30 +55:58:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:46.64 +55:24:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:11:47.56 +55:27:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:18.99 +55:16:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:34.34 +54:40:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:34.49 +54:39:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:47.55 +54:41:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:12:59.22 +55:34:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:03.08 +55:43:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:04.73 +56:43:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:29.33 +56:55:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:32.11 +54:36:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:32.44 +55:15:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:36.12 +55:38:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:47.45 +56:30:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:55.38 +55:27:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:56.50 +55:25:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:56.59 +54:17:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:58.59 +56:31:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:13:58.82 +53:19:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:09.14 +56:26:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:15.61 +53:53:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:18.36 +54:02:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:23.65 +52:58:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:25.46 +53:35:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:30.31 +55:30:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:30.40 +53:29:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:31.80 +53:50:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:32.70 +54:44:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:34.19 +57:04:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:34.44 +55:57:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:39.23 +54:17:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:43.64 +54:44:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:46.10 +57:01:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:46.63 +52:54:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:50.04 +55:24:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:54.27 +55:00:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:14:58.02 +56:01:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:00.68 +55:27:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:05.48 +52:30:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:12.47 +52:13:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:12.70 +53:15:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:12.87 +54:11:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:13.69 +52:09:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:15.23 +53:51:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:16.56 +53:02:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:17.13 +54:04:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:17.99 +53:29:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:19.57 +56:28:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:35.46 +52:09:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:37.17 +54:22:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:38.74 +53:18:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:39.76 +54:30:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:41.21 +53:21:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:45.35 +54:47:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:47.76 +54:58:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:49.17 +54:42:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:49.23 +52:50:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:53.87 +57:02:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:15:58.54 +54:10:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:01.56 +55:36:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:02.19 +52:58:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:09.31 +53:48:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:19.40 +54:47:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:20.46 +52:05:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:21.53 +53:04:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:22.30 +53:52:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:25.10 +54:01:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:30.27 +53:08:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:33.42 +56:59:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:35.08 +56:46:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:39.91 +56:29:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:16:51.96 +54:13:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:08.15 +53:54:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:11.07 +53:36:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:11.07 +56:03:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:28.43 +53:27:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:34.14 +53:34:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:35.25 +54:40:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:36.98 +52:53:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:37.23 +51:54:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:45.41 +56:54:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:53.18 +53:53:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:54.28 +55:27:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:54.85 +54:02:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:55.05 +54:18:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:17:56.25 +55:25:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:01.30 +54:07:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:01.69 +54:03:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:01.81 +53:42:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:06.95 +55:05:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:08.05 +53:41:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:08.89 +56:55:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:20.22 +52:39:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:23.18 +52:39:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:33.81 +55:52:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:41.56 +54:46:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:18:42.39 +54:57:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:07.36 +55:41:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:10.89 +54:25:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:16.70 +55:34:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:18.64 +55:23:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:25.33 +55:38:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:25.45 +56:55:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:31.01 +53:07:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:35.83 +54:10:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:38.69 +54:49:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:38.83 +54:22:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:39.77 +55:04:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:48.73 +52:55:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:54.88 +54:33:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:56.24 +54:56:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:19:56.60 +56:53:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:07.23 +55:43:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:26.01 +52:26:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:27.83 +51:25:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:38.48 +52:15:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:20:45.16 +55:50:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:14.77 +54:14:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:21.42 +56:54:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:26.77 +51:25:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:26.83 +54:07:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:29.40 +56:15:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:31.31 +54:25:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:35.97 +52:15:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:45.86 +54:25:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:55.39 +54:35:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:21:58.57 +54:52:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:05.30 +52:39:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:07.86 +54:45:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:21.61 +56:29:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:25.15 +55:31:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:22:45.33 +52:22:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:03.31 +55:20:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:09.89 +52:36:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:10.72 +56:57:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:26.83 +55:05:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:32.97 +54:29:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:47.40 +54:32:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:23:51.71 +56:20:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:23.81 +56:17:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:48.05 +56:02:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:50.08 +57:00:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:51.30 +56:17:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:04.57 +55:52:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:09.08 +55:35:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:12.74 +54:23:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:15.17 +56:00:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:53.49 +55:45:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:02.49 +55:37:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:07.61 +57:14:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:12.98 +55:30:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:18.51 +55:19:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:37.11 +55:28:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:39.23 +55:39:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:51.40 +54:14:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:53.36 +56:25:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:26:55.39 +57:19:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:08.57 +57:56:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:13.16 +54:36:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:25.75 +53:28:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:25.75 +56:43:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:32.52 +54:43:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:34.12 +54:33:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:37.01 +56:15:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:38.62 +57:03:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:51.82 +57:07:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:57.66 +55:37:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:27:59.89 +56:00:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:13.78 +55:31:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:14.02 +57:41:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:28:42.59 +57:11:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:11.22 +55:12:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:17.34 +54:35:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:25.81 +54:56:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:41.45 +55:55:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:29:44.72 +55:16:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:01.22 +55:54:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:06.03 +54:28:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:06.24 +54:42:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:15.05 +55:35:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:17.98 +54:25:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:41.40 +55:31:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:42.74 +54:58:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:30:53.67 +55:01:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:02.76 +54:13:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:14.93 +54:16:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:32.30 +54:31:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:38.06 +54:52:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:31:52.24 +55:24:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:02.00 +54:33:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:03.93 +56:47:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:13.05 +54:36:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:21.04 +56:19:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:31.21 +55:27:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:32.93 +56:41:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:36.20 +55:07:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:32:57.84 +55:20:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:01.40 +54:38:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:18.72 +56:16:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:46.97 +56:23:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:48.63 +55:44:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:33:57.82 +55:18:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:15.18 +54:35:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:25.78 +54:29:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:42.99 +57:22:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:49.87 +54:52:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:23.98 +56:20:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:43.23 +54:55:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:55.50 +54:52:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:58.96 +54:45:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:00.61 +54:33:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:08.16 +54:50:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:17.30 +58:00:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:43.70 +57:59:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:45.10 +57:01:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:58.43 +54:29:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:22.76 +57:07:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:34.22 +55:28:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:47.13 +58:01:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:31.97 +56:57:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:42.20 +55:51:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:43.59 +57:07:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:01.78 +56:50:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:06.84 +56:50:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:09.50 +56:50:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:06.81 +57:58:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:19.27 +56:52:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:31.53 +56:49:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:25.89 +57:58:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:35.21 +57:49:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:47.21 +58:01:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:53.25 +57:35:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:03.56 +57:40:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:13.98 +57:45:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:16.96 +57:55:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:20.54 +56:48:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:44.22 +57:54:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:32.20 +57:23:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:44.54 +57:58:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:57.96 +57:31:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:58.71 +56:57:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:40.40 +57:42:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:29.00 +57:54:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:15.65 +57:52:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:22.36 +57:55:41.8 -- 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)
00:26:17.02 +49:45:32.0 -- not a known variable star
00:26:43.55 +50:38:16.8 -- not a known variable star
23:10:45.12 +56:08:16.7 -- not a known variable star
23:11:24.30 +55:58:54.2 -- not a known variable star
23:11:46.64 +55:24:34.7 -- not a known variable star
23:11:47.56 +55:27:46.1 -- not a known variable star
23:12:18.99 +55:16:00.9 -- a known variable star
23:12:34.34 +54:40:14.3 -- not a known variable star
23:12:34.49 +54:39:40.3 -- not a known variable star
23:12:47.55 +54:41:56.4 -- not a known variable star
23:12:59.22 +55:34:38.1 -- not a known variable star
23:13:03.08 +55:43:03.2 -- not a known variable star
23:13:04.73 +56:43:23.7 -- not a known variable star
23:13:29.33 +56:55:19.7 -- not a known variable star
23:13:32.11 +54:36:44.4 -- not a known variable star
23:13:32.44 +55:15:28.7 -- not a known variable star
23:13:36.12 +55:38:46.1 -- not a known variable star
23:13:47.45 +56:30:59.2 -- not a known variable star
23:13:55.38 +55:27:50.3 -- not a known variable star
23:13:56.50 +55:25:37.8 -- a known variable star
23:13:56.59 +54:17:45.0 -- not a known variable star
23:13:58.59 +56:31:17.4 -- a known variable star
23:13:58.82 +53:19:37.0 -- not a known variable star
23:14:09.14 +56:26:10.1 -- not a known variable star
23:14:15.61 +53:53:54.8 -- not a known variable star
23:14:18.36 +54:02:54.6 -- not a known variable star
23:14:23.65 +52:58:53.0 -- a known variable star
23:14:25.46 +53:35:42.3 -- a known variable star
23:14:30.31 +55:30:20.3 -- not a known variable star
23:14:30.40 +53:29:10.0 -- not a known variable star
23:14:31.80 +53:50:27.8 -- not a known variable star
23:14:32.70 +54:44:09.1 -- not a known variable star
23:14:34.19 +57:04:36.0 -- not a known variable star
23:14:34.44 +55:57:47.9 -- not a known variable star
23:14:39.23 +54:17:58.8 -- not a known variable star
23:14:43.64 +54:44:02.1 -- not a known variable star
23:14:46.10 +57:01:34.0 -- not a known variable star
23:14:46.63 +52:54:55.4 -- not a known variable star
23:14:50.04 +55:24:50.9 -- not a known variable star
23:14:54.27 +55:00:57.8 -- not a known variable star
23:14:58.02 +56:01:19.0 -- not a known variable star
23:15:00.68 +55:27:37.5 -- not a known variable star
23:15:05.48 +52:30:01.7 -- not a known variable star
23:15:12.47 +52:13:25.3 -- not a known variable star
23:15:12.70 +53:15:41.0 -- not a known variable star
23:15:12.87 +54:11:50.9 -- a known variable star
23:15:13.69 +52:09:41.4 -- not a known variable star
23:15:15.23 +53:51:11.9 -- a known variable star
23:15:16.56 +53:02:09.3 -- a known variable star
23:15:17.13 +54:04:35.0 -- not a known variable star
23:15:17.99 +53:29:56.8 -- not a known variable star
23:15:19.57 +56:28:53.9 -- not a known variable star
23:15:35.46 +52:09:47.5 -- not a known variable star
23:15:37.17 +54:22:36.2 -- not a known variable star
23:15:38.74 +53:18:33.4 -- a known variable star
23:15:39.76 +54:30:28.8 -- not a known variable star
23:15:41.21 +53:21:41.6 -- not a known variable star
23:15:45.35 +54:47:50.6 -- not a known variable star
23:15:47.76 +54:58:14.9 -- not a known variable star
23:15:49.17 +54:42:21.6 -- a known variable star
23:15:49.23 +52:50:40.9 -- not a known variable star
23:15:53.87 +57:02:25.2 -- not a known variable star
23:15:58.54 +54:10:16.7 -- not a known variable star
23:16:01.56 +55:36:22.2 -- not a known variable star
23:16:02.19 +52:58:01.9 -- not a known variable star
23:16:09.31 +53:48:25.6 -- not a known variable star
23:16:19.40 +54:47:52.9 -- not a known variable star
23:16:20.46 +52:05:57.6 -- not a known variable star
23:16:21.53 +53:04:54.1 -- not a known variable star
23:16:22.30 +53:52:52.6 -- not a known variable star
23:16:25.10 +54:01:09.4 -- not a known variable star
23:16:30.27 +53:08:44.7 -- not a known variable star
23:16:33.42 +56:59:47.7 -- not a known variable star
23:16:35.08 +56:46:41.8 -- not a known variable star
23:16:39.91 +56:29:27.8 -- not a known variable star
23:16:51.96 +54:13:37.3 -- not a known variable star
23:17:08.15 +53:54:15.9 -- not a known variable star
23:17:11.07 +53:36:00.8 -- not a known variable star
23:17:11.07 +56:03:01.7 -- not a known variable star
23:17:28.43 +53:27:01.5 -- not a known variable star
23:17:34.14 +53:34:44.7 -- not a known variable star
23:17:35.25 +54:40:53.9 -- not a known variable star
23:17:36.98 +52:53:25.7 -- not a known variable star
23:17:37.23 +51:54:22.0 -- not a known variable star
23:17:45.41 +56:54:51.5 -- not a known variable star
23:17:53.18 +53:53:03.8 -- not a known variable star
23:17:54.28 +55:27:35.5 -- not a known variable star
23:17:54.85 +54:02:55.7 -- not a known variable star
23:17:55.05 +54:18:14.4 -- not a known variable star
23:17:56.25 +55:25:42.4 -- not a known variable star
23:18:01.30 +54:07:27.0 -- not a known variable star
23:18:01.69 +54:03:48.9 -- a known variable star
23:18:01.81 +53:42:03.7 -- not a known variable star
23:18:06.95 +55:05:34.2 -- not a known variable star
23:18:08.05 +53:41:11.3 -- not a known variable star
23:18:08.89 +56:55:36.0 -- not a known variable star
23:18:20.22 +52:39:22.6 -- not a known variable star
23:18:23.18 +52:39:51.7 -- not a known variable star
23:18:33.81 +55:52:09.0 -- not a known variable star
23:18:41.56 +54:46:21.0 -- not a known variable star
23:18:42.39 +54:57:41.2 -- a known variable star
23:19:07.36 +55:41:18.2 -- not a known variable star
23:19:10.89 +54:25:33.4 -- not a known variable star
23:19:16.70 +55:34:13.3 -- not a known variable star
23:19:18.64 +55:23:09.6 -- a known variable star
23:19:25.33 +55:38:48.2 -- a known variable star
23:19:25.45 +56:55:07.4 -- not a known variable star
23:19:31.01 +53:07:24.0 -- not a known variable star
23:19:35.83 +54:10:39.1 -- not a known variable star
23:19:38.69 +54:49:13.9 -- not a known variable star
23:19:38.83 +54:22:29.4 -- not a known variable star
23:19:39.77 +55:04:10.7 -- not a known variable star
23:19:48.73 +52:55:01.9 -- not a known variable star
23:19:54.88 +54:33:51.7 -- not a known variable star
23:19:56.24 +54:56:35.5 -- not a known variable star
23:19:56.60 +56:53:58.7 -- not a known variable star
23:20:07.23 +55:43:22.5 -- not a known variable star
23:20:26.01 +52:26:49.9 -- not a known variable star
23:20:27.83 +51:25:08.0 -- not a known variable star
23:20:38.48 +52:15:03.9 -- not a known variable star
23:20:45.16 +55:50:06.0 -- not a known variable star
23:21:14.77 +54:14:41.7 -- not a known variable star
23:21:21.42 +56:54:37.7 -- not a known variable star
23:21:26.77 +51:25:56.2 -- not a known variable star
23:21:26.83 +54:07:11.5 -- not a known variable star
23:21:29.40 +56:15:30.1 -- not a known variable star
23:21:31.31 +54:25:20.0 -- not a known variable star
23:21:35.97 +52:15:13.3 -- not a known variable star
23:21:45.86 +54:25:14.4 -- not a known variable star
23:21:55.39 +54:35:42.1 -- not a known variable star
23:21:58.57 +54:52:10.1 -- not a known variable star
23:22:05.30 +52:39:33.0 -- not a known variable star
23:22:07.86 +54:45:26.6 -- not a known variable star
23:22:21.61 +56:29:36.7 -- not a known variable star
23:22:25.15 +55:31:37.9 -- not a known variable star
23:22:45.33 +52:22:47.1 -- not a known variable star
23:23:03.31 +55:20:04.8 -- not a known variable star
23:23:09.89 +52:36:00.7 -- not a known variable star
23:23:10.72 +56:57:08.7 -- not a known variable star
23:23:26.83 +55:05:04.9 -- not a known variable star
23:23:32.97 +54:29:59.7 -- not a known variable star
23:23:47.40 +54:32:06.3 -- not a known variable star
23:23:51.71 +56:20:24.8 -- not a known variable star
23:24:23.81 +56:17:15.3 -- not a known variable star
23:24:48.05 +56:02:35.3 -- not a known variable star
23:24:50.08 +57:00:22.7 -- not a known variable star
23:24:51.30 +56:17:42.2 -- not a known variable star
23:25:04.57 +55:52:06.1 -- not a known variable star
23:25:09.08 +55:35:12.3 -- not a known variable star
23:25:12.74 +54:23:17.1 -- not a known variable star
23:25:15.17 +56:00:10.4 -- not a known variable star
23:25:53.49 +55:45:47.2 -- not a known variable star
23:26:02.49 +55:37:17.4 -- not a known variable star
23:26:07.61 +57:14:57.4 -- not a known variable star
23:26:12.98 +55:30:59.2 -- not a known variable star
23:26:18.51 +55:19:51.5 -- not a known variable star
23:26:37.11 +55:28:49.0 -- not a known variable star
23:26:39.23 +55:39:34.7 -- not a known variable star
23:26:51.40 +54:14:40.4 -- a known variable star
23:26:53.36 +56:25:56.4 -- not a known variable star
23:26:55.39 +57:19:49.3 -- not a known variable star
23:27:08.57 +57:56:28.7 -- not a known variable star
23:27:13.16 +54:36:25.8 -- not a known variable star
23:27:25.75 +53:28:43.0 -- not a known variable star
23:27:25.75 +56:43:28.8 -- not a known variable star
23:27:32.52 +54:43:03.7 -- not a known variable star
23:27:34.12 +54:33:50.7 -- not a known variable star
23:27:37.01 +56:15:56.3 -- not a known variable star
23:27:38.62 +57:03:07.5 -- not a known variable star
23:27:51.82 +57:07:05.0 -- not a known variable star
23:27:57.66 +55:37:44.4 -- not a known variable star
23:27:59.89 +56:00:06.1 -- not a known variable star
23:28:13.78 +55:31:06.4 -- not a known variable star
23:28:14.02 +57:41:39.9 -- not a known variable star
23:28:42.59 +57:11:03.1 -- not a known variable star
23:29:11.22 +55:12:46.5 -- not a known variable star
23:29:17.34 +54:35:12.9 -- not a known variable star
23:29:25.81 +54:56:43.2 -- not a known variable star
23:29:41.45 +55:55:24.8 -- not a known variable star
23:29:44.72 +55:16:19.1 -- not a known variable star
23:30:01.22 +55:54:14.2 -- not a known variable star
23:30:06.03 +54:28:15.6 -- not a known variable star
23:30:06.24 +54:42:16.8 -- not a known variable star
23:30:15.05 +55:35:38.9 -- not a known variable star
23:30:17.98 +54:25:55.5 -- not a known variable star
23:30:41.40 +55:31:43.5 -- not a known variable star
23:30:42.74 +54:58:05.5 -- a known variable star
23:30:53.67 +55:01:29.5 -- not a known variable star
23:31:02.76 +54:13:33.3 -- not a known variable star
23:31:14.93 +54:16:11.9 -- not a known variable star
23:31:32.30 +54:31:32.9 -- not a known variable star
23:31:38.06 +54:52:04.7 -- not a known variable star
23:31:52.24 +55:24:25.2 -- not a known variable star
23:32:02.00 +54:33:58.2 -- not a known variable star
23:32:03.93 +56:47:02.7 -- not a known variable star
23:32:13.05 +54:36:49.8 -- not a known variable star
23:32:21.04 +56:19:24.7 -- not a known variable star
23:32:31.21 +55:27:33.1 -- not a known variable star
23:32:32.93 +56:41:23.6 -- not a known variable star
23:32:36.20 +55:07:12.7 -- not a known variable star
23:32:57.84 +55:20:35.9 -- not a known variable star
23:33:01.40 +54:38:42.6 -- not a known variable star
23:33:18.72 +56:16:57.8 -- not a known variable star
23:33:46.97 +56:23:25.9 -- not a known variable star
23:33:48.63 +55:44:18.1 -- not a known variable star
23:33:57.82 +55:18:00.7 -- not a known variable star
23:34:15.18 +54:35:52.2 -- a known variable star
23:34:25.78 +54:29:17.4 -- not a known variable star
23:34:42.99 +57:22:12.9 -- not a known variable star
23:34:49.87 +54:52:42.5 -- not a known variable star
23:35:23.98 +56:20:57.3 -- not a known variable star
23:35:43.23 +54:55:15.1 -- not a known variable star
23:35:55.50 +54:52:45.0 -- not a known variable star
23:35:58.96 +54:45:35.1 -- not a known variable star
23:36:00.61 +54:33:04.0 -- not a known variable star
23:36:08.16 +54:50:06.8 -- not a known variable star
23:36:17.30 +58:00:14.4 -- not a known variable star
23:36:43.70 +57:59:50.0 -- not a known variable star
23:36:45.10 +57:01:41.5 -- not a known variable star
23:36:58.43 +54:29:57.6 -- not a known variable star
23:37:22.76 +57:07:09.6 -- not a known variable star
23:37:34.22 +55:28:31.4 -- not a known variable star
23:37:47.13 +58:01:32.6 -- a known variable star
23:38:31.97 +56:57:45.4 -- a known variable star
23:39:42.20 +55:51:27.0 -- not a known variable star
23:39:43.59 +57:07:19.3 -- not a known variable star
23:40:01.78 +56:50:24.8 -- not a known variable star
23:41:06.84 +56:50:15.3 -- not a known variable star
23:41:09.50 +56:50:24.5 -- not a known variable star
23:42:06.81 +57:58:08.8 -- not a known variable star
23:42:19.27 +56:52:00.2 -- not a known variable star
23:42:31.53 +56:49:09.8 -- not a known variable star
23:43:25.89 +57:58:09.1 -- not a known variable star
23:43:35.21 +57:49:28.1 -- not a known variable star
23:43:47.21 +58:01:11.0 -- not a known variable star
23:43:53.25 +57:35:52.5 -- not a known variable star
23:44:03.56 +57:40:10.8 -- not a known variable star
23:44:13.98 +57:45:24.9 -- not a known variable star
23:44:16.96 +57:55:31.4 -- not a known variable star
23:44:20.54 +56:48:40.2 -- not a known variable star
23:44:44.22 +57:54:11.1 -- not a known variable star
23:45:32.20 +57:23:44.0 -- not a known variable star
23:45:44.54 +57:58:28.6 -- not a known variable star
23:45:57.96 +57:31:58.3 -- a known variable star
23:45:58.71 +56:57:42.7 -- not a known variable star
23:46:40.40 +57:42:14.9 -- not a known variable star
23:47:29.00 +57:54:32.3 -- not a known variable star
23:48:15.65 +57:52:36.7 -- not a known variable star
23:53:22.36 +57:55:41.8 -- not a known variable star
Found 229 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
249 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 249 (excluding asteroids and hot pixels, 229 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)2461292.75967416 -observatory V36
11:51:08.02 +01:55:33.0 Mercury (-0.8mag)
13:40:54.39 -15:14:59.6 Venus (-4.7mag)
07:19:16.59 +22:51:06.4 Mars (1.2mag)
09:10:39.64 +16:50:43.2 Jupiter (-1.8mag)
00:51:16.45 +02:35:23.1 Saturn (0.4mag)
04:13:42.36 +21:02:02.3 Uranus (5.7mag)
00:13:33.61 -00:04:29.2 Neptune (7.7mag)
20:25:27.63 -23:40:03.4 Pluto (14.5mag)
09:38:20.14 +14:11:48.2 Moon (-8.7mag)
-rw-r--r-- 1 apache apache 362 Sep 9 01:34 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461292.75967416:
09:10:38.97 +16:50:46.9 Io (6.2mag)
09:10:48.34 +16:50:00.5 Europa (6.3mag)
09:10:26.22 +16:51:50.7 Ganymede (5.7mag)
09:10:28.56 +16:51:39.8 Callisto (6.9mag)
09:08:29.98 +17:08:06.5 Himalia (15.7mag)
09:10:43.48 +16:50:25.5 Thebe (16.6mag)
09:08:05.96 +17:02:01.0 Elara (17.7mag)
09:14:30.42 +16:17:43.2 Pasiphae (17.9mag)
09:11:36.16 +17:09:02.2 Carme (19.0mag)
00:51:04.39 +02:35:39.2 Titan (8.3mag)
00:51:20.99 +02:35:09.8 Rhea (9.6mag)
00:51:26.31 +02:37:42.7 Iapetus (11.0mag)
00:51:32.36 +02:35:06.1 Hyperion (14.3mag)
00:50:01.18 +02:24:56.5 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 9 01:34 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461292.75967416:
22:20:21.55 +03:01:21.7 JWST
16:17:30.21 +47:30:18.8 Chandra
10:30:35.38 -57:45:11.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 9 01:34 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461292.75967416 -observatory V36
03:41:33.22 +19:25:45.4 17.4mag P/1996 R2 (Lagerkvist)
18:03:37.86 -34:10:29.5 14.4mag P/2010 H2 (Vales)
07:20:56.70 -70:24:38.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:54.47 +33:45:04.8 17.7mag C/2017 K2 (PANSTARRS)
22:11:55.76 +28:25:44.9 17.5mag C/2022 E2 (ATLAS)
07:11:39.59 +25:56:34.2 16.9mag C/2022 N2 (PANSTARRS)
10:51:18.33 +27:09:22.2 17.1mag C/2022 QE78 (ATLAS)
09:49:54.81 +05:13:20.1 18.0mag C/2022 R6 (PANSTARRS)
15:29:01.62 -15:49:17.2 14.9mag C/2023 R1 (PANSTARRS)
08:40:05.90 +33:00:52.1 15.8mag C/2024 E1 (Wierzchos)
15:06:51.22 +15:18:01.3 17.9mag C/2024 G6 (ATLAS)
18:32:24.76 +43:05:54.5 13.7mag C/2024 J3 (ATLAS)
20:23:30.38 +49:11:34.5 17.4mag C/2024 R4 (PANSTARRS)
05:36:38.19 -13:03:13.5 15.1mag C/2024 T5 (ATLAS)
07:12:17.31 +18:08:57.4 17.8mag C/2025 J1 (Borisov)
11:21:09.07 +18:36:56.3 16.8mag C/2025 V2 (Rankin)
13:21:14.93 -00:02:32.5 16.8mag C/2025 Y1 (ATLAS)
16:46:36.87 +73:42:24.7 16.1mag C/2026 A2 (Bok)
03:04:47.44 +46:04:12.6 17.5mag C/2026 B2 (Sun-Gao)
12:15:05.55 +11:26:36.8 17.5mag A/2026 E1
22:27:38.35 -35:09:17.1 7.8mag 10P/Tempel
11:49:29.18 -05:36:57.5 16.3mag 29P/Schwassmann-Wachmann
12:12:31.33 -05:42:53.4 17.6mag 63P/Wild
06:43:06.67 +19:06:01.6 13.7mag 78P/Gehrels
20:16:10.80 -26:11:20.4 17.2mag 84P/Giclas
03:17:20.65 +15:01:12.6 17.2mag 88P/Howell
05:44:46.22 +29:22:44.2 16.9mag 112P/Urata-Niijima
07:37:36.35 +24:18:31.1 15.9mag 114P/Wiseman-Skiff
10:32:16.17 +20:27:01.0 14.8mag 123P/West-Hartley
12:50:55.81 -22:01:13.9 17.5mag 124P/Mrkos
06:19:46.70 +20:34:39.4 15.9mag 128P/Shoemaker-Holt
02:24:15.07 -17:21:41.0 11.3mag 161P/Hartley-IRAS
08:58:19.29 +37:32:12.4 16.4mag 162P/Siding Spring
09:34:36.91 +12:32:40.1 13.2mag 169P/NEAT
03:26:01.99 +08:18:35.9 17.7mag 220P/McNaught
04:53:20.73 +36:55:50.3 15.2mag 260P/McNaught
08:37:07.45 +35:29:25.8 17.3mag 295P/LINEAR
15:26:31.16 -00:28:09.5 17.9mag 391P/Kowalski
09:29:28.59 +16:45:00.2 17.8mag 450P/LONEOS
-rw-r--r-- 1 apache apache 1.9K Sep 9 01:34 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
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
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
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
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
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
-rw-r--r-- 1 apache apache 5.7K Sep 9 01:34 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
-rw-r--r-- 1 apache apache 190K Sep 9 01:34 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
23:11:22.440 +03:34:45.08 AT 2026yur 2026-08-06.81 22.15
23:52:10.400 +03:53:48.67 AT 2026yuq 2026-08-06.76 22.26
01:28:25.390 -00:33:31.00 AT 2026yup 2026-07-22.87 22.24
06:19:46.733 +50:57:31.05 AT 2026yuo 2026-08-13.50 19.744
23:24:50.114 +15:25:58.38 AT 2026yun 2026-08-10.05 19.96
00:25:27.120 +20:14:05.91 SN 2026yum 2026-08-13.09 18.04
22:02:49.666 -13:05:30.39 AT 2026yul 2026-08-12.92 18.89
21:45:50.911 -04:08:31.57 AT 2026yuk 2026-08-12.78 19.08
01:02:47.624 -06:59:05.24 AT 2026yuj 2026-08-13.05 19.25
23:50:13.455 +20:53:14.83 AT 2026yui 2026-08-12.94 19.46
22:53:22.575 -18:00:52.62 AT 2026yuh 2026-08-12.37 19.1729
01:03:55.125 -10:40:35.60 AT 2026yug 2026-08-10.42 20.3834
22:18:45.584 -09:23:49.69 AT 2026yuf 2026-08-08.36 20.7186
20:49:39.970 +17:00:06.86 AT 2026yue 2026-08-10.93 20.1
20:59:25.458 +10:53:21.92 AT 2026yud 2026-08-11.36 21.56
21:58:23.744 -28:57:27.15 AT 2026yuc 2026-08-11.43 21.11
00:12:25.184 -01:24:55.24 AT 2026yub 2026-08-07.68 20.14
23:47:47.304 +17:27:46.66 AT 2026yua 2026-08-09.11 19.97
02:47:39.785 +19:08:06.82 AT 2026ytz 2026-08-11.18 20.24
16:58:27.059 +18:21:36.28 AT 2026yty 2026-08-11.32 20.59
-rw-r--r-- 1 apache apache 88K Sep 9 01:34 tns_transients_list.txt
