This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.58 01:56:38.12 +59:15:33.7
131.18823 -2.56326 galactic Cas Second-epoch detections are separated by 0.7" and 5.7 pix
The object was found in VSX 0" X Cas
Type: M
# Max. Min./Amp. JD0 Period
9.450 V 13.200 V 2457020.00000 415.000000000000 C5,4e(N1e)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.12 +59:15:33.7: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.12 +59:15:33.7: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 56 38.12 +59 15 33.7 8.6 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
X Cas,2461228.7512,8.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
X Cas 20260707.2512 8.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.29 01:43:36.46 +58:48:08.4
129.65675 -3.38658 galactic Cas Second-epoch detections are separated by 0.3" and 5.6 pix
The object was found in VSX 1" V0917 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
10.500 V 11.200 V M7
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:36.46 +58:48:08.4: 14.72 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:36.46 +58:48:08.4: 10.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.22 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 43 36.46 +58 48 08.4 9.3 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
V0917 Cas,2461228.7512,9.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0917 Cas 20260707.2512 9.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.80 02:24:29.85 +59:24:31.5
134.53125 -1.35093 galactic Cas Second-epoch detections are separated by 0.3" and 5.9 pix
The object was found in VSX 1" V0672 Cas
Type: SR
# Max. Min./Amp. JD0 Period
15.000 B 17.400 B 302.000000000000
ATTENTION: measured mag 10.80 is 4.2 mag brighter than the VSX record maximum brightness 15.00 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:29.85 +59:24:31.5: 15.65 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:29.85 +59:24:31.5: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 24 29.85 +59 24 31.5 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0672 Cas,2461228.7512,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0672 Cas 20260707.2512 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.54 02:21:40.73 +60:54:41.6
133.68152 -0.06276 galactic Cas Second-epoch detections are separated by 0.3" and 5.8 pix
The object was found in VSX 1" DE Cas
Type: SRB
# Max. Min./Amp. JD0 Period
13.900 pg 15.100 pg 2428925.00000 151.000000000000 M6
ATTENTION: measured mag 9.54 is 4.4 mag brighter than the VSX record maximum brightness 13.90 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:40.73 +60:54:41.6: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:40.73 +60:54:41.6: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 21 40.73 +60 54 41.6 9.5 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
DE Cas,2461228.7512,9.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DE Cas 20260707.2512 9.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 11.44 01:02:45.67 +63:46:46.0
124.18241 0.93519 galactic Cas Second-epoch detections are separated by 1.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:02:45.67 +63:46:46.0 (user input) | T | P | (position from user input) J-Ks=0.928+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:45.67 +63:46:46.0: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:45.67 +63:46:46.0: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 02 45.67 +63 46 46.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 11.31 01:55:33.43 +62:51:23.2
130.17014 0.88927 galactic Cas Second-epoch detections are separated by 4.5" and 6.2 pix
The object was found in VSX18" ZTF J015530.84+625127.0
Type: BY
# Max. Min./Amp. JD0 Period
18.289 r Y 0.140 r 2458351.87810 1.514835700000
ATTENTION: measured mag 11.31 is 6.8 mag brighter than the VSX record maximum brightness 18.15 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:33.43 +62:51:23.2: 12.17 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:33.43 +62:51:23.2: 14.49 +/- 0.08 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 07 07.2512* 01 55 33.43 +62 51 23.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J015530.84+625127.0,2461228.7512,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015530.84+625127.0 20260707.2512 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.96 01:32:27.31 +64:14:12.8
127.37165 1.71929 galactic Cas Second-epoch detections are separated by 2.9" and 5.6 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 | 01:32:27.31 +64:14:12.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:27.31 +64:14:12.8: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:27.31 +64:14:12.8: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 07 07.2512* 01 32 27.31 +64 14 12.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.74 02:04:53.86 +64:12:10.7
130.82006 2.46208 galactic Cas Second-epoch detections are separated by 4.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:04:53.86 +64:12:10.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:04:53.86 +64:12:10.7: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:04:53.86 +64:12:10.7: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 04 53.86 +64 12 10.7 10.7 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,2461228.7512,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.69 01:26:06.09 +59:01:11.0
127.38868 -3.55175 galactic Cas Second-epoch detections are separated by 5.6" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J021.5231+59.0209 | 01:26:06.09 +59:01:11.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:06.09 +59:01:11.0: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:06.09 +59:01:11.0: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 26 06.09 +59 01 11.0 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.5231+59.0209,2461228.7512,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021.5231+59.0209 20260707.2512 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.66 01:51:44.29 +60:38:43.1
130.25900 -1.36575 galactic Cas Second-epoch detections are separated by 2.2" and 5.4 pix
The object was found in VSX21" Gaia DR3 508173284866588544
Type: ROT
# Max. Min./Amp. JD0 Period
14.540 G 14.560 G 13.389700000000 K
ATTENTION: measured mag 10.66 is 3.9 mag brighter than the VSX record maximum brightness 14.54 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:44.29 +60:38:43.1: 13.48 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:44.29 +60:38:43.1: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 51 44.29 +60 38 43.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508173284866588544,2461228.7512,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 508173284866588544 20260707.2512 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 11.01 01:09:25.27 +64:35:19.7
124.86044 1.78442 galactic Cas Second-epoch detections are separated by 1.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:09:25.27 +64:35:19.7 (user input) | T | P | (position from user input) J-Ks=0.557+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:25.27 +64:35:19.7: 12.46 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:25.27 +64:35:19.7: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 07 07.2512* 01 09 25.27 +64 35 19.7 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.80 01:13:07.51 +58:55:53.3
125.73308 -3.82227 galactic Cas Second-epoch detections are separated by 4.6" and 5.0 pix
The object was found in VSX 2" Gaia DR3 414108381479338368
Type: VAR
# Max. Min./Amp. JD0 Period
13.530 G 13.560 G 0.456759000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:07.51 +58:55:53.3: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:07.51 +58:55:53.3: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 13 07.51 +58 55 53.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414108381479338368,2461228.7512,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 414108381479338368 20260707.2512 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.47 01:40:55.21 +57:55:17.8
129.48358 -4.31932 galactic Cas Second-epoch detections are separated by 4.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.2276+57.9295 | 01:40:55.21 +57:55:17.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:55.21 +57:55:17.8: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:55.21 +57:55:17.8: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 40 55.21 +57 55 17.8 10.5 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 J025.2276+57.9295,2461228.7512,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J025.2276+57.9295 20260707.2512 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.17 02:18:13.88 +57:38:00.5
134.36667 -3.29855 galactic Per 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 | ATO J034.5644+57.6268 | 02:18:13.88 +57:38:00.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K1 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:13.88 +57:38:00.5: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:13.88 +57:38:00.5: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 18 13.88 +57 38 00.5 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J034.5644+57.6268,2461228.7512,10.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J034.5644+57.6268 20260707.2512 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.67 01:11:45.03 +61:13:57.5
125.37422 -1.54275 galactic Cas Second-epoch detections are separated by 1.7" and 5.1 pix
The object was found in VSX 2" ZTF J011144.73+611356.9
Type: RS
# Max. Min./Amp. JD0 Period
13.552 r Y 0.107 r 2458423.79830 1.359407700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:45.03 +61:13:57.5: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:45.03 +61:13:57.5: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 11 45.03 +61 13 57.5 10.7 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 J011144.73+611356.9,2461228.7512,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011144.73+611356.9 20260707.2512 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.60 00:56:47.64 +60:38:48.7
123.58874 -2.21806 galactic Cas Second-epoch detections are separated by 2.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426546125736902528 | 00:56:44.52 +60:38:23.6 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.712+/-0.026 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:56:47.64 +60:38:48.7: 10.68 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:56:47.64 +60:38:48.7: 13.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 56 47.64 +60 38 48.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426546125736902528,2461228.7512,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 426546125736902528 20260707.2512 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.30 01:13:51.48 +58:12:20.1
125.89093 -4.53730 galactic Cas Second-epoch detections are separated by 8.0" and 4.3 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 J018.4686+58.2100 | 01:13:51.48 +58:12:20.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:51.48 +58:12:20.1: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:51.48 +58:12:20.1: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 13 51.48 +58 12 20.1 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J018.4686+58.2100,2461228.7512,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J018.4686+58.2100 20260707.2512 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.60 00:54:31.45 +59:24:01.9
123.32538 -3.46886 galactic Cas Second-epoch detections are separated by 4.8" and 5.9 pix
The object was found in VSX 3" V0415 Cas
Type: EA/DS
# Max. Min./Amp. JD0 Period
14.000 pg 16.800 pg 2429106.58700 12.536157000000
ATTENTION: measured mag 10.60 is 3.4 mag brighter than the VSX record maximum brightness 14.00 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:54:31.45 +59:24:01.9: 11.93 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:54:31.45 +59:24:01.9: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.34 +/- 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 07 07.2512* 00 54 31.45 +59 24 01.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0415 Cas,2461228.7512,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0415 Cas 20260707.2512 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.38 01:17:48.27 +57:17:35.1
126.50394 -5.39569 galactic Cas Second-epoch detections are separated by 1.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:17:48.27 +57:17:35.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:48.27 +57:17:35.1: 12.84 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:48.27 +57:17:35.1: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 17 48.27 +57 17 35.1 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.99 02:25:56.68 +56:38:22.1
135.69341 -3.87243 galactic Per Second-epoch detections are separated by 2.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457634404691160448 | 02:25:53.98 +56:38:46.3 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:56.68 +56:38:22.1: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:56.68 +56:38:22.1: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 25 56.68 +56 38 22.1 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457634404691160448,2461228.7512,9.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457634404691160448 20260707.2512 9.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.87 02:01:40.01 +58:27:27.8
132.02549 -3.16862 galactic Cas Second-epoch detections are separated by 3.0" and 5.9 pix
The object was found in VSX 7" Gaia DR3 505504181723708416
Type: ROT
# Max. Min./Amp. JD0 Period
12.810 G 12.860 G 2.222820000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:40.01 +58:27:27.8: 12.81 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:40.01 +58:27:27.8: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 01 40.01 +58 27 27.8 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505504181723708416,2461228.7512,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 505504181723708416 20260707.2512 9.87CV 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 07 07.2512 2461228.7512 10.23 00:52:55.14 +58:28:53.1
123.12605 -4.38977 galactic Cas Second-epoch detections are separated by 1.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J013.2201+58.4812 | 00:52:55.14 +58:28:53.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:55.14 +58:28:53.1: 11.21 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:55.14 +58:28:53.1: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 52 55.14 +58 28 53.1 10.2 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 J013.2201+58.4812,2461228.7512,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J013.2201+58.4812 20260707.2512 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.27 00:59:04.64 +61:08:53.8
123.85379 -1.70980 galactic Cas Second-epoch detections are separated by 0.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:59:04.64 +61:08:53.8 (user input) | T | P | (position from user input) J-Ks=0.220+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:59:04.64 +61:08:53.8: 10.40 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:59:04.64 +61:08:53.8: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 59 04.64 +61 08 53.8 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.93 01:01:40.14 +58:50:23.6
124.25831 -4.00551 galactic Cas Second-epoch detections are separated by 0.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J015.4178+58.8525 | 01:01:40.14 +58:50:23.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.770+/-0.026 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:40.14 +58:50:23.6: 12.99 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:01:40.14 +58:50:23.6: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 01 40.14 +58 50 23.6 9.9 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 J015.4178+58.8525,2461228.7512,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015.4178+58.8525 20260707.2512 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.54 02:23:04.39 +56:30:08.5
135.37084 -4.14012 galactic Per Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458285624814498048 | 02:23:02.07 +56:30:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1965LS....C05....0H LS V +56 40 J-Ks=0.885+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:04.39 +56:30:08.5: 11.35 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:04.39 +56:30:08.5: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 23 04.39 +56 30 08.5 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 458285624814498048,2461228.7512,9.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 458285624814498048 20260707.2512 9.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.81 02:33:52.47 +57:01:39.2
136.55783 -3.10934 galactic Per Second-epoch detections are separated by 0.6" and 6.2 pix
The object was found in VSX 1" DW Per
Type: DCEP
# Max. Min./Amp. JD0 Period
11.200 V 11.860 V 2436906.70300 3.649785000000 F6Ib
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:52.47 +57:01:39.2: 12.77 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:52.47 +57:01:39.2: 11.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 52.47 +57 01 39.2 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DW Per,2461228.7512,8.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DW Per 20260707.2512 8.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.78 02:36:31.33 +57:11:40.8
136.82403 -2.81533 galactic Per Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457813144048325248 | 02:36:28.37 +57:11:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1928AnHar.100...49C HD 236972 J-Ks=0.092+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:31.33 +57:11:40.8: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:31.33 +57:11:40.8: 10.31 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.31 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 36 31.33 +57 11 40.8 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457813144048325248,2461228.7512,7.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457813144048325248 20260707.2512 7.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 6.83 02:31:25.68 +55:59:07.1
136.64324 -4.20154 galactic Per Second-epoch detections are separated by 0.7" and 6.2 pix
The object was found in VSX19" Gaia DR3 457343205908261760
Type: ROT
# Max. Min./Amp. JD0 Period
16.250 G 16.350 G 0.771500000000 M
ATTENTION: measured mag 6.83 is 9.4 mag brighter than the VSX record maximum brightness 16.25 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:25.68 +55:59:07.1: 12.35 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:25.68 +55:59:07.1: 9.55 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.55 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 25.68 +55 59 07.1 6.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457343205908261760,2461228.7512,6.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457343205908261760 20260707.2512 6.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.01 02:34:34.26 +56:21:55.4
136.90259 -3.68306 galactic Per Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457749475453771648 | 02:34:34.64 +56:21:57.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:34.26 +56:21:55.4: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:34.26 +56:21:55.4: 9.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.60 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 34.26 +56 21 55.4 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457749475453771648,2461228.7512,7.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457749475453771648 20260707.2512 7.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.08 02:34:43.98 +56:06:06.6
137.02593 -3.91720 galactic Per Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6785+56.0961 | 02:34:44.47 +56:06:09.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:43.98 +56:06:06.6: 12.37 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:43.98 +56:06:06.6: 9.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.76 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 43.98 +56 06 06.6 7.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.6785+56.0961,2461228.7512,7.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.6785+56.0961 20260707.2512 7.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.12 02:30:53.66 +56:14:27.7
136.47771 -3.99257 galactic Per Second-epoch detections are separated by 0.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457384093997742208 | 02:30:54.14 +56:14:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:53.66 +56:14:27.7: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:53.66 +56:14:27.7: 10.01 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.01 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 53.66 +56 14 27.7 7.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457384093997742208,2461228.7512,7.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457384093997742208 20260707.2512 7.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.12 02:33:34.37 +55:54:24.4
136.95159 -4.15979 galactic Per Second-epoch detections are separated by 2.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3939+55.9184 | 02:33:35.02 +55:54:27.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.37 +55:54:24.4: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.37 +55:54:24.4: 9.85 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.85 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 34.37 +55 54 24.4 7.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.3939+55.9184,2461228.7512,7.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.3939+55.9184 20260707.2512 7.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.39 02:34:05.29 +56:25:32.0
136.81753 -3.65344 galactic Per Second-epoch detections are separated by 0.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457750815483540992 | 02:34:05.68 +56:25:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:05.29 +56:25:32.0: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:05.29 +56:25:32.0: 10.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.18 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 05.29 +56 25 32.0 7.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457750815483540992,2461228.7512,7.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457750815483540992 20260707.2512 7.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.45 02:31:25.68 +56:07:04.6
136.59309 -4.07869 galactic Per Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457379661591549312 | 02:31:25.96 +56:07:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:25.68 +56:07:04.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:25.68 +56:07:04.6: 10.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 25.68 +56 07 04.6 7.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457379661591549312,2461228.7512,7.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457379661591549312 20260707.2512 7.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.43 02:32:15.41 +56:38:50.3
136.49877 -3.54529 galactic Per Second-epoch detections are separated by 0.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457772187240678912 | 02:32:15.71 +56:38:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.015+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:15.41 +56:38:50.3: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:15.41 +56:38:50.3: 10.27 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.27 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 15.41 +56 38 50.3 7.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457772187240678912,2461228.7512,7.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457772187240678912 20260707.2512 7.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.49 02:29:11.88 +56:17:58.5
136.23676 -4.02586 galactic Per Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.2903+56.3099 | 02:29:12.29 +56:17:57.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:11.88 +56:17:58.5: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:11.88 +56:17:58.5: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.26 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 11.88 +56 17 58.5 7.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.2903+56.3099,2461228.7512,7.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.2903+56.3099 20260707.2512 7.49CV 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 07 07.2512 2461228.7512 7.66 02:31:06.52 +56:30:41.9
136.40344 -3.73062 galactic Per Second-epoch detections are separated by 0.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457581971731866368 | 02:31:06.88 +56:30:40.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:06.52 +56:30:41.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:06.52 +56:30:41.9: 10.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.43 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 06.52 +56 30 41.9 7.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457581971731866368,2461228.7512,7.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457581971731866368 20260707.2512 7.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.63 02:32:55.20 +56:39:40.3
136.57789 -3.49773 galactic Per Second-epoch detections are separated by 0.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2188+56.6593 | 02:32:55.49 +56:39:40.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.759+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:55.20 +56:39:40.3: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:55.20 +56:39:40.3: 10.33 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.33 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 55.20 +56 39 40.3 7.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.2188+56.6593,2461228.7512,7.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.2188+56.6593 20260707.2512 7.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.72 02:34:03.63 +56:30:43.3
136.78054 -3.57515 galactic Per Second-epoch detections are separated by 0.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457755763285796480 | 02:34:03.88 +56:30:45.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:03.63 +56:30:43.3: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:03.63 +56:30:43.3: 10.32 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.32 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 03.63 +56 30 43.3 7.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457755763285796480,2461228.7512,7.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457755763285796480 20260707.2512 7.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.75 02:30:12.38 +56:11:25.1
136.40779 -4.07538 galactic Per Second-epoch detections are separated by 0.5" and 6.1 pix
The object was found in VSX22" ZTF J023014.84+561117.4
Type: EW
# Max. Min./Amp. JD0 Period
18.223 r Y 0.543 r 2458387.94220 0.264294400000
ATTENTION: measured mag 7.75 is 9.9 mag brighter than the VSX record maximum brightness 17.68 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:12.38 +56:11:25.1: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:12.38 +56:11:25.1: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 12.38 +56 11 25.1 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J023014.84+561117.4,2461228.7512,7.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023014.84+561117.4 20260707.2512 7.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.78 02:28:50.73 +56:20:49.0
136.17372 -3.99983 galactic Per Second-epoch detections are separated by 0.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457554415218933120 | 02:28:50.80 +56:20:47.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.101+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:50.73 +56:20:49.0: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:50.73 +56:20:49.0: 10.63 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.63 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 28 50.73 +56 20 49.0 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457554415218933120,2461228.7512,7.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457554415218933120 20260707.2512 7.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.99 02:31:37.61 +56:33:36.4
136.45145 -3.65881 galactic Per Second-epoch detections are separated by 0.7" and 6.1 pix
The object was found in VSX16" Gaia DR3 457583792795921664
Type: ROT
# Max. Min./Amp. JD0 Period
15.730 G 15.790 G K
ATTENTION: measured mag 7.99 is 7.7 mag brighter than the VSX record maximum brightness 15.73 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:37.61 +56:33:36.4: 12.47 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:37.61 +56:33:36.4: 10.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.77 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 37.61 +56 33 36.4 8.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457583792795921664,2461228.7512,7.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457583792795921664 20260707.2512 7.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.12 02:32:18.25 +56:21:26.4
136.61520 -3.81104 galactic Per Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457388938720751616 | 02:32:18.57 +56:21:26.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:18.25 +56:21:26.4: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:18.25 +56:21:26.4: 10.88 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.88 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 18.25 +56 21 26.4 8.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457388938720751616,2461228.7512,8.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457388938720751616 20260707.2512 8.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.18 02:31:45.44 +55:57:57.8
136.69330 -4.20197 galactic Per Second-epoch detections are separated by 1.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9520+55.9630 | 02:31:46.12 +55:57:58.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:45.44 +55:57:57.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:45.44 +55:57:57.8: 11.13 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 45.44 +55 57 57.8 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.9520+55.9630,2461228.7512,8.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.9520+55.9630 20260707.2512 8.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.25 02:30:49.34 +56:11:02.2
136.48986 -4.04925 galactic Per Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457383716040658304 | 02:30:49.82 +56:11:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:49.34 +56:11:02.2: 12.93 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:49.34 +56:11:02.2: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 49.34 +56 11 02.2 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457383716040658304,2461228.7512,8.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457383716040658304 20260707.2512 8.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.31 02:30:37.31 +56:22:57.8
136.38938 -3.87535 galactic Per Second-epoch detections are separated by 0.6" and 6.1 pix
The object was found in VSX19" Gaia DR3 457575031062827776
Type: ROT
# Max. Min./Amp. JD0 Period
15.200 G 15.240 G K
ATTENTION: measured mag 8.31 is 6.9 mag brighter than the VSX record maximum brightness 15.20 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:37.31 +56:22:57.8: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:37.31 +56:22:57.8: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 37.31 +56 22 57.8 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457575031062827776,2461228.7512,8.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457575031062827776 20260707.2512 8.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.25 02:34:28.50 +56:22:24.5
136.88717 -3.68077 galactic Per Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6214+56.3728 | 02:34:29.15 +56:22:22.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:28.50 +56:22:24.5: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:28.50 +56:22:24.5: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 28.50 +56 22 24.5 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.6214+56.3728,2461228.7512,8.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.6214+56.3728 20260707.2512 8.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.33 02:33:34.12 +56:11:47.9
136.83931 -3.89244 galactic Per Second-epoch detections are separated by 0.9" and 6.1 pix
The object was found in VSX 7" Gaia DR3 457371518333663744
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.980 G 11.010 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.12 +56:11:47.9: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.12 +56:11:47.9: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 34.12 +56 11 47.9 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457371518333663744,2461228.7512,8.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457371518333663744 20260707.2512 8.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.36 02:35:42.61 +56:44:19.7
136.90157 -3.27800 galactic Per Second-epoch detections are separated by 0.7" and 6.1 pix
The object was found in VSX 2" Gaia DR3 457785175221622144
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.720 G 10.770 G 5.916700000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:42.61 +56:44:19.7: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:42.61 +56:44:19.7: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 42.61 +56 44 19.7 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457785175221622144,2461228.7512,8.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457785175221622144 20260707.2512 8.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.32 02:29:40.94 +56:20:04.5
136.28632 -3.96849 galactic Per Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457550704367181056 | 02:29:41.31 +56:20:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:40.94 +56:20:04.5: 10.56 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:40.94 +56:20:04.5: 11.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 40.94 +56 20 04.5 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457550704367181056,2461228.7512,8.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457550704367181056 20260707.2512 8.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.42 02:34:04.59 +56:42:29.8
136.70666 -3.39327 galactic Per Second-epoch detections are separated by 0.6" and 6.1 pix
The object was found in VSX21" Gaia DR3 457775687633336704
Type: RS
# Max. Min./Amp. JD0 Period
17.400 G 17.580 G K
ATTENTION: measured mag 8.42 is 9.0 mag brighter than the VSX record maximum brightness 17.40 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:04.59 +56:42:29.8: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:04.59 +56:42:29.8: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 04.59 +56 42 29.8 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457775687633336704,2461228.7512,8.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457775687633336704 20260707.2512 8.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.38 02:34:26.00 +56:29:14.3
136.83765 -3.57806 galactic Per Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457752877067783040 | 02:34:26.47 +56:29:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:26.00 +56:29:14.3: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:26.00 +56:29:14.3: 11.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 26.00 +56 29 14.3 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457752877067783040,2461228.7512,8.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457752877067783040 20260707.2512 8.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.39 02:33:05.10 +56:13:02.1
136.76913 -3.89921 galactic Per Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457372446046599424 | 02:33:05.74 +56:12:59.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:05.10 +56:13:02.1: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:05.10 +56:13:02.1: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 05.10 +56 13 02.1 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457372446046599424,2461228.7512,8.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457372446046599424 20260707.2512 8.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.43 02:28:49.03 +56:07:35.6
136.25134 -4.20622 galactic Per Second-epoch detections are separated by 1.1" and 6.3 pix
The object was found in VSX 4" Gaia DR3 457541805195095296
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.960 G 11.030 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:49.03 +56:07:35.6: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:49.03 +56:07:35.6: 11.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 28 49.03 +56 07 35.6 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457541805195095296,2461228.7512,8.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457541805195095296 20260707.2512 8.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.38 02:32:13.91 +55:56:22.5
136.76498 -4.20129 galactic Per Second-epoch detections are separated by 2.3" and 6.0 pix
The object was found in VSX 6" V1071 Per
Type: EW
# Max. Min./Amp. JD0 Period
10.940 V 11.240 V 2457070.72700 0.359847600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:13.91 +55:56:22.5: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:13.91 +55:56:22.5: 11.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 13.91 +55 56 22.5 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1071 Per,2461228.7512,8.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1071 Per 20260707.2512 8.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.50 02:34:13.00 +56:12:36.6
136.91741 -3.84521 galactic Per Second-epoch detections are separated by 1.0" and 6.1 pix
The object was found in VSX 4" Gaia DR3 457326232196815232
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.910 G 10.930 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.00 +56:12:36.6: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.00 +56:12:36.6: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 13.00 +56 12 36.6 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457326232196815232,2461228.7512,8.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457326232196815232 20260707.2512 8.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.48 02:35:28.90 +56:28:21.8
136.97691 -3.53516 galactic Per Second-epoch detections are separated by 0.4" and 6.2 pix
The object was found in VSX 3" Gaia DR3 457711026906434048
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.890 G 10.920 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:28.90 +56:28:21.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:28.90 +56:28:21.8: 11.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 28.90 +56 28 21.8 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457711026906434048,2461228.7512,8.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457711026906434048 20260707.2512 8.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.53 02:30:03.66 +56:22:33.4
136.31973 -3.91061 galactic Per Second-epoch detections are separated by 0.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457574305207452288 | 02:30:04.15 +56:22:32.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:03.66 +56:22:33.4: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:03.66 +56:22:33.4: 11.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 03.66 +56 22 33.4 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457574305207452288,2461228.7512,8.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457574305207452288 20260707.2512 8.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.54 02:34:43.49 +56:34:06.4
136.84324 -3.48768 galactic Per Second-epoch detections are separated by 0.9" and 6.1 pix
The object was found in VSX 2" Gaia DR3 457759061822261632
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.990 G 11.080 G 0.079441300000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:43.49 +56:34:06.4: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:43.49 +56:34:06.4: 11.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 43.49 +56 34 06.4 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457759061822261632,2461228.7512,8.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457759061822261632 20260707.2512 8.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.57 02:29:58.04 +56:08:50.1
136.39291 -4.12773 galactic Per Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457359423705242368 | 02:29:58.63 +56:08:48.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:58.04 +56:08:50.1: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:58.04 +56:08:50.1: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 58.04 +56 08 50.1 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457359423705242368,2461228.7512,8.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457359423705242368 20260707.2512 8.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.63 02:31:00.12 +56:00:29.2
136.57930 -4.20283 galactic Per Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457355163097206784 | 02:31:00.46 +56:00:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:00.12 +56:00:29.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:00.12 +56:00:29.2: 11.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 00.12 +56 00 29.2 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457355163097206784,2461228.7512,8.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457355163097206784 20260707.2512 8.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.71 02:34:13.62 +56:18:40.6
136.87955 -3.75141 galactic Per Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457749097496685824 | 02:34:14.13 +56:18:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.62 +56:18:40.6: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.62 +56:18:40.6: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 13.62 +56 18 40.6 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457749097496685824,2461228.7512,8.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457749097496685824 20260707.2512 8.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.70 02:30:59.13 +56:08:43.7
136.52544 -4.07639 galactic Per Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457380619359718400 | 02:30:59.49 +56:08:45.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:59.13 +56:08:43.7: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:59.13 +56:08:43.7: 11.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 59.13 +56 08 43.7 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457380619359718400,2461228.7512,8.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457380619359718400 20260707.2512 8.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.76 02:28:34.90 +56:13:02.9
136.18728 -4.13370 galactic Per Second-epoch detections are separated by 3.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457551872598387456 | 02:28:35.19 +56:13:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:34.90 +56:13:02.9: 12.75 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:34.90 +56:13:02.9: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 28 34.90 +56 13 02.9 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457551872598387456,2461228.7512,8.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457551872598387456 20260707.2512 8.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.81 02:32:19.08 +56:15:24.4
136.65528 -3.90332 galactic Per Second-epoch detections are separated by 1.2" and 6.1 pix
The object was found in VSX 5" Gaia DR3 457388045367612800
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.410 G 11.440 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:19.08 +56:15:24.4: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:19.08 +56:15:24.4: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 19.08 +56 15 24.4 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457388045367612800,2461228.7512,8.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457388045367612800 20260707.2512 8.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.78 02:29:39.02 +56:11:32.8
136.33501 -4.10215 galactic Per Second-epoch detections are separated by 0.3" and 6.1 pix
The object was found in VSX 7" NSV 15519
Type: SR
# Max. Min./Amp. JD0 Period
12.400 V 13.100 V 2458443.36190 299.178129200000 C
ATTENTION: measured mag 8.78 is 3.6 mag brighter than the VSX record maximum brightness 12.40 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:39.02 +56:11:32.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:39.02 +56:11:32.8: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 39.02 +56 11 32.8 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 15519,2461228.7512,8.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 15519 20260707.2512 8.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.86 02:27:59.59 +56:09:19.5
136.13365 -4.22142 galactic Per Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457545614823486720 | 02:27:59.64 +56:09:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.917+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:59.59 +56:09:19.5: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:59.59 +56:09:19.5: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 27 59.59 +56 09 19.5 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457545614823486720,2461228.7512,8.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457545614823486720 20260707.2512 8.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.89 02:34:12.75 +56:11:54.4
136.92142 -3.85625 galactic Per Second-epoch detections are separated by 1.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457326232196815232 | 02:34:13.32 +56:12:39.2 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:12.75 +56:11:54.4: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:12.75 +56:11:54.4: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 12.75 +56 11 54.4 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457326232196815232,2461228.7512,8.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457326232196815232 20260707.2512 8.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.82 02:29:26.60 +56:00:56.3
136.37381 -4.27707 galactic Per Second-epoch detections are separated by 1.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457352620476607744 | 02:29:27.28 +56:00:57.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:26.60 +56:00:56.3: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:26.60 +56:00:56.3: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 26.60 +56 00 56.3 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457352620476607744,2461228.7512,8.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457352620476607744 20260707.2512 8.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.86 02:29:59.42 +56:13:01.1
136.36989 -4.06182 galactic Per Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457548814581644416 | 02:30:00.12 +56:12:59.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:59.42 +56:13:01.1: 11.59 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:59.42 +56:13:01.1: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 59.42 +56 13 01.1 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457548814581644416,2461228.7512,8.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457548814581644416 20260707.2512 8.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.94 02:31:29.57 +56:26:21.8
136.47994 -3.77759 galactic Per Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457393749084094976 | 02:31:29.77 +56:26:22.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.329+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:29.57 +56:26:21.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:29.57 +56:26:21.8: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 29.57 +56 26 21.8 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457393749084094976,2461228.7512,8.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457393749084094976 20260707.2512 8.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.88 02:33:51.65 +56:11:00.3
136.88201 -3.88900 galactic Per Second-epoch detections are separated by 1.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4611+56.1832 | 02:33:52.13 +56:11:00.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:51.65 +56:11:00.3: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:51.65 +56:11:00.3: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 51.65 +56 11 00.3 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.4611+56.1832,2461228.7512,8.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.4611+56.1832 20260707.2512 8.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.92 02:35:00.16 +56:43:10.0
136.81967 -3.33371 galactic Per Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457764520717250560 | 02:35:00.38 +56:43:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.105+/-0.026 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:00.16 +56:43:10.0: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:00.16 +56:43:10.0: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 00.16 +56 43 10.0 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457764520717250560,2461228.7512,8.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457764520717250560 20260707.2512 8.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.87 02:30:43.88 +55:58:11.5
136.55851 -4.25248 galactic Per Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.6774+55.9705 | 02:30:44.39 +55:58:12.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:43.88 +55:58:11.5: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:43.88 +55:58:11.5: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 43.88 +55 58 11.5 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.6774+55.9705,2461228.7512,8.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.6774+55.9705 20260707.2512 8.87CV 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 07 07.2512 2461228.7512 8.99 02:33:48.69 +55:57:06.6
136.96513 -4.10534 galactic Per Second-epoch detections are separated by 2.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4666+55.9563 | 02:33:49.36 +55:57:06.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:48.69 +55:57:06.6: 12.91 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:48.69 +55:57:06.6: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 48.69 +55 57 06.6 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.4666+55.9563,2461228.7512,8.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.4666+55.9563 20260707.2512 8.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.99 02:30:00.30 +56:17:42.9
136.34260 -3.98840 galactic Per Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457549639215308800 | 02:30:00.77 +56:17:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:00.30 +56:17:42.9: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:00.30 +56:17:42.9: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 00.30 +56 17 42.9 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457549639215308800,2461228.7512,8.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457549639215308800 20260707.2512 8.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.93 02:33:50.75 +55:59:56.4
136.95134 -4.05996 galactic Per Second-epoch detections are separated by 2.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457322349546464896 | 02:33:51.13 +55:59:55.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:50.75 +55:59:56.4: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:50.75 +55:59:56.4: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 50.75 +55 59 56.4 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457322349546464896,2461228.7512,8.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457322349546464896 20260707.2512 8.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.02 02:28:41.03 +56:12:03.3
136.20662 -4.14389 galactic Per Second-epoch detections are separated by 0.9" and 6.1 pix
The object was found in VSX 6" ASASSN-V J022841.63+561200.9
Type: L
# Max. Min./Amp. JD0 Period
12.590 V 12.860 V
ATTENTION: measured mag 9.02 is 3.6 mag brighter than the VSX record maximum brightness 12.59 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:41.03 +56:12:03.3: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:41.03 +56:12:03.3: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 28 41.03 +56 12 03.3 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J022841.63+561200.9,2461228.7512,9.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022841.63+561200.9 20260707.2512 9.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.96 02:34:03.12 +56:00:34.9
136.97386 -4.03898 galactic Per Second-epoch detections are separated by 1.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457322280826978560 | 02:34:03.58 +56:00:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:03.12 +56:00:34.9: 12.99 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:03.12 +56:00:34.9: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 03.12 +56 00 34.9 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457322280826978560,2461228.7512,8.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457322280826978560 20260707.2512 8.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.01 02:28:56.63 +56:11:03.7
136.24644 -4.14598 galactic Per Second-epoch detections are separated by 1.1" and 6.3 pix
The object was found in VSX14" ZTF J022856.73+561050.0
Type: RS
# Max. Min./Amp. JD0 Period
16.955 r Y 0.059 r 2458475.80570 0.641758300000
ATTENTION: measured mag 9.01 is 7.9 mag brighter than the VSX record maximum brightness 16.90 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:56.63 +56:11:03.7: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:56.63 +56:11:03.7: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 28 56.63 +56 11 03.7 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J022856.73+561050.0,2461228.7512,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022856.73+561050.0 20260707.2512 9.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.05 02:36:27.29 +56:56:50.8
136.91322 -3.04613 galactic Per Second-epoch detections are separated by 0.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.1156+56.9471 | 02:36:27.75 +56:56:49.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:27.29 +56:56:50.8: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:27.29 +56:56:50.8: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 36 27.29 +56 56 50.8 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J039.1156+56.9471,2461228.7512,9.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.1156+56.9471 20260707.2512 9.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.15 02:34:09.50 +56:41:03.1
136.72636 -3.41115 galactic Per Second-epoch detections are separated by 2.2" and 5.9 pix
The object was found in VSX 7" Gaia DR3 457775240955622912
Type: ROT
# Max. Min./Amp. JD0 Period
11.750 G 11.790 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:09.50 +56:41:03.1: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:09.50 +56:41:03.1: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 09.50 +56 41 03.1 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457775240955622912,2461228.7512,9.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457775240955622912 20260707.2512 9.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.07 02:35:40.34 +56:37:58.5
136.93833 -3.37746 galactic Per Second-epoch detections are separated by 0.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457760539289289856 | 02:35:40.84 +56:38:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:40.34 +56:37:58.5: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:40.34 +56:37:58.5: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 40.34 +56 37 58.5 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457760539289289856,2461228.7512,9.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457760539289289856 20260707.2512 9.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.06 02:34:34.53 +56:36:41.0
136.80756 -3.45608 galactic Per Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457762325995735040 | 02:34:34.87 +56:36:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2 2004AJ....128..463R G 174- 4
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:34.53 +56:36:41.0: 12.84 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:34.53 +56:36:41.0: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 34.53 +56 36 41.0 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457762325995735040,2461228.7512,9.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457762325995735040 20260707.2512 9.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.12 02:35:12.53 +56:50:10.0
136.80019 -3.21526 galactic Per Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8034+56.8391 | 02:35:12.85 +56:50:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:12.53 +56:50:10.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:12.53 +56:50:10.0: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 12.53 +56 50 10.0 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.8034+56.8391,2461228.7512,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.8034+56.8391 20260707.2512 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.14 02:33:28.33 +56:18:30.9
136.78379 -3.79425 galactic Per Second-epoch detections are separated by 2.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3673+56.3061 | 02:33:28.77 +56:18:31.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:28.33 +56:18:30.9: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:28.33 +56:18:30.9: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 28.33 +56 18 30.9 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.3673+56.3061,2461228.7512,9.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.3673+56.3061 20260707.2512 9.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.09 02:30:38.35 +56:11:55.5
136.46062 -4.04506 galactic Per Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457360523216287616 | 02:30:38.75 +56:11:55.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:38.35 +56:11:55.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:38.35 +56:11:55.5: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 38.35 +56 11 55.5 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457360523216287616,2461228.7512,9.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457360523216287616 20260707.2512 9.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.20 02:34:37.65 +56:32:36.9
136.84052 -3.51580 galactic Per Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6528+56.5460 | 02:34:37.95 +56:32:37.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:37.65 +56:32:36.9: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:37.65 +56:32:36.9: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 37.65 +56 32 36.9 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.6528+56.5460,2461228.7512,9.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.6528+56.5460 20260707.2512 9.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.25 02:33:57.85 +56:36:42.0
136.72975 -3.48835 galactic Per Second-epoch detections are separated by 1.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457757412554149760 | 02:33:58.20 +56:36:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:57.85 +56:36:42.0: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:57.85 +56:36:42.0: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 57.85 +56 36 42.0 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457757412554149760,2461228.7512,9.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457757412554149760 20260707.2512 9.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.22 02:34:43.75 +56:51:49.3
136.72893 -3.21537 galactic Per Second-epoch detections are separated by 1.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457801736615450240 | 02:34:44.20 +56:51:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:43.75 +56:51:49.3: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:43.75 +56:51:49.3: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 43.75 +56 51 49.3 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457801736615450240,2461228.7512,9.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457801736615450240 20260707.2512 9.22CV 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 07 07.2512 2461228.7512 9.21 02:34:13.66 +56:19:36.9
136.87357 -3.73696 galactic Per Second-epoch detections are separated by 1.0" and 6.4 pix
The object was found in VSX24" Gaia DR3 457749161916090496
Type: ROT
# Max. Min./Amp. JD0 Period
17.690 G 17.800 G
ATTENTION: measured mag 9.21 is 8.5 mag brighter than the VSX record maximum brightness 17.69 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.66 +56:19:36.9: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.66 +56:19:36.9: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 13.66 +56 19 36.9 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457749161916090496,2461228.7512,9.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457749161916090496 20260707.2512 9.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.19 02:34:22.42 +56:20:28.4
136.88672 -3.71593 galactic Per Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5944+56.3413 | 02:34:22.68 +56:20:28.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.252+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:22.42 +56:20:28.4: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:22.42 +56:20:28.4: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 22.42 +56 20 28.4 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.5944+56.3413,2461228.7512,9.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.5944+56.3413 20260707.2512 9.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.21 02:35:16.02 +56:26:20.3
136.96277 -3.57781 galactic Per Second-epoch detections are separated by 0.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457710477150655104 | 02:35:16.32 +56:26:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:16.02 +56:26:20.3: 11.03 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:16.02 +56:26:20.3: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 16.02 +56 26 20.3 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457710477150655104,2461228.7512,9.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457710477150655104 20260707.2512 9.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.26 02:28:10.75 +56:06:42.8
136.17378 -4.25247 galactic Per Second-epoch detections are separated by 3.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457543798059942784 | 02:28:10.98 +56:06:41.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.793+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:10.75 +56:06:42.8: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:10.75 +56:06:42.8: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 28 10.75 +56 06 42.8 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457543798059942784,2461228.7512,9.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457543798059942784 20260707.2512 9.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.30 02:32:37.23 +56:00:39.2
136.78818 -4.11465 galactic Per Second-epoch detections are separated by 2.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457363443795236736 | 02:32:37.60 +56:00:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:37.23 +56:00:39.2: 12.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:37.23 +56:00:39.2: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 37.23 +56 00 39.2 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457363443795236736,2461228.7512,9.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457363443795236736 20260707.2512 9.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.26 02:29:46.43 +56:03:52.1
136.39864 -4.21460 galactic Per Second-epoch detections are separated by 3.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457358564711288576 | 02:29:46.93 +56:03:52.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:46.43 +56:03:52.1: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:46.43 +56:03:52.1: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 46.43 +56 03 52.1 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457358564711288576,2461228.7512,9.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457358564711288576 20260707.2512 9.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.29 02:29:43.15 +56:05:11.6
136.38332 -4.19693 galactic Per Second-epoch detections are separated by 0.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457358770869699584 | 02:29:43.62 +56:05:12.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:43.15 +56:05:11.6: 12.39 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:43.15 +56:05:11.6: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 43.15 +56 05 11.6 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457358770869699584,2461228.7512,9.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457358770869699584 20260707.2512 9.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.30 02:29:39.10 +56:20:59.6
136.27667 -3.95585 galactic Per Second-epoch detections are separated by 1.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.4149+56.3474 | 02:29:39.41 +56:21:00.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:39.10 +56:20:59.6: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:39.10 +56:20:59.6: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 39.10 +56 20 59.6 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.4149+56.3474,2461228.7512,9.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.4149+56.3474 20260707.2512 9.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.26 02:33:06.27 +56:00:33.3
136.85148 -4.09032 galactic Per Second-epoch detections are separated by 1.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457363993551045760 | 02:33:06.84 +56:00:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:06.27 +56:00:33.3: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:06.27 +56:00:33.3: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 06.27 +56 00 33.3 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457363993551045760,2461228.7512,9.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457363993551045760 20260707.2512 9.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.32 02:35:22.31 +56:48:50.7
136.82936 -3.22684 galactic Per Second-epoch detections are separated by 0.6" and 6.2 pix
The object was found in VSX21" Gaia DR3 457788782994109440
Type: RS
# Max. Min./Amp. JD0 Period
15.830 G 15.960 G K
ATTENTION: measured mag 9.32 is 6.5 mag brighter than the VSX record maximum brightness 15.83 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:22.31 +56:48:50.7: 12.20 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:22.31 +56:48:50.7: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 22.31 +56 48 50.7 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457788782994109440,2461228.7512,9.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457788782994109440 20260707.2512 9.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.35 02:36:27.90 +56:50:29.8
136.95629 -3.14284 galactic Per Second-epoch detections are separated by 1.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.1180+56.8422 | 02:36:28.32 +56:50:31.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:27.90 +56:50:29.8: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:27.90 +56:50:29.8: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 36 27.90 +56 50 29.8 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J039.1180+56.8422,2461228.7512,9.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.1180+56.8422 20260707.2512 9.35CV 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 07 07.2512 2461228.7512 9.35 02:31:43.40 +56:14:44.1
136.58293 -3.94499 galactic Per Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457382685248448384 | 02:31:43.75 +56:14:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:43.40 +56:14:44.1: 12.26 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:43.40 +56:14:44.1: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 43.40 +56 14 44.1 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457382685248448384,2461228.7512,9.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457382685248448384 20260707.2512 9.35CV 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 07 07.2512 2461228.7512 9.38 02:33:30.82 +56:43:01.2
136.63190 -3.41496 galactic Per Second-epoch detections are separated by 1.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3826+56.7191 | 02:33:31.00 +56:43:01.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.239+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:30.82 +56:43:01.2: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:30.82 +56:43:01.2: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 30.82 +56 43 01.2 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.3826+56.7191,2461228.7512,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.3826+56.7191 20260707.2512 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.45 02:36:18.23 +56:52:16.6
136.92431 -3.12426 galactic Per Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457788027079795584 | 02:36:18.77 +56:52:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:18.23 +56:52:16.6: 11.48 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:18.23 +56:52:16.6: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 36 18.23 +56 52 16.6 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457788027079795584,2461228.7512,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457788027079795584 20260707.2512 9.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.37 02:32:49.98 +56:14:33.6
136.72696 -3.88911 galactic Per Second-epoch detections are separated by 0.3" and 6.2 pix
The object was found in VSX 9" Gaia DR3 457375366624349696
Type: ROT
# Max. Min./Amp. JD0 Period
16.490 G 16.530 G K
ATTENTION: measured mag 9.37 is 7.1 mag brighter than the VSX record maximum brightness 16.49 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:49.98 +56:14:33.6: 13.12 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:49.98 +56:14:33.6: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 49.98 +56 14 33.6 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457375366624349696,2461228.7512,9.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457375366624349696 20260707.2512 9.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.47 02:33:02.07 +56:26:23.7
136.67726 -3.69617 galactic Per Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2606+56.4396 | 02:33:02.56 +56:26:22.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:02.07 +56:26:23.7: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:02.07 +56:26:23.7: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 02.07 +56 26 23.7 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.2606+56.4396,2461228.7512,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.2606+56.4396 20260707.2512 9.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.44 02:29:40.37 +56:13:41.1
136.32468 -4.06789 galactic Per Second-epoch detections are separated by 1.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457549703634773504 | 02:29:40.64 +56:13:41.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.047+/-0.036 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:40.37 +56:13:41.1: 13.05 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:40.37 +56:13:41.1: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 40.37 +56 13 41.1 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457549703634773504,2461228.7512,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457549703634773504 20260707.2512 9.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.43 02:33:07.80 +56:14:49.7
136.76345 -3.86920 galactic Per Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457375538423034496 | 02:33:08.17 +56:14:48.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:07.80 +56:14:49.7: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:07.80 +56:14:49.7: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 07.80 +56 14 49.7 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457375538423034496,2461228.7512,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457375538423034496 20260707.2512 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.55 02:34:06.45 +56:06:18.8
136.94403 -3.94787 galactic Per Second-epoch detections are separated by 2.0" and 6.1 pix
The object was not found in VSX
The object was found in ASASSN-V 4" ASASSN-V J023406.97+560618.0
Type: EA
MeanMag 12.45 m Amp. 1.03 m Period 0.2057389 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:06.45 +56:06:18.8: 10.95 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:06.45 +56:06:18.8: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 06.45 +56 06 18.8 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461228.7512,9.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260707.2512 9.55CV 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 07 07.2512 2461228.7512 9.45 02:29:33.63 +56:09:09.1
136.33820 -4.14386 galactic Per Second-epoch detections are separated by 1.8" 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 | Gaia DR3 457547199673991168 | 02:29:34.17 +56:09:08.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:33.63 +56:09:09.1: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:33.63 +56:09:09.1: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 33.63 +56 09 09.1 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457547199673991168,2461228.7512,9.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457547199673991168 20260707.2512 9.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.48 02:31:12.76 +56:27:39.4
136.43587 -3.77220 galactic Per Second-epoch detections are separated by 1.6" and 5.9 pix
The object was found in VSX19" Gaia DR3 457393920882782336
Type: ROT
# Max. Min./Amp. JD0 Period
15.310 G 15.340 G F
ATTENTION: measured mag 9.48 is 5.8 mag brighter than the VSX record maximum brightness 15.31 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:12.76 +56:27:39.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:12.76 +56:27:39.4: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 12.76 +56 27 39.4 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457393920882782336,2461228.7512,9.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457393920882782336 20260707.2512 9.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.52 02:30:38.96 +56:15:15.0
136.44114 -3.99314 galactic Per Second-epoch detections are separated by 1.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457384952991198080 | 02:30:39.44 +56:15:12.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:38.96 +56:15:15.0: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:38.96 +56:15:15.0: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 38.96 +56 15 15.0 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457384952991198080,2461228.7512,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457384952991198080 20260707.2512 9.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.43 02:33:40.00 +56:00:07.2
136.92701 -4.06684 galactic Per Second-epoch detections are separated by 2.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457316508390945792 | 02:33:40.52 +56:00:07.2 (Gaia DR3) | ROT (local) | 0.393643000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:40.00 +56:00:07.2: 12.20 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:40.00 +56:00:07.2: 12.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 40.00 +56 00 07.2 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457316508390945792,2461228.7512,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457316508390945792 20260707.2512 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.59 02:31:04.55 +56:05:04.2
136.56010 -4.12816 galactic Per Second-epoch detections are separated by 2.6" and 6.1 pix
The object was found in VSX21" ZTF J023102.07+560506.0
Type: RS
# Max. Min./Amp. JD0 Period
16.508 r Y 0.070 r 2458425.80690 0.946063100000
ATTENTION: measured mag 9.59 is 6.8 mag brighter than the VSX record maximum brightness 16.44 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:04.55 +56:05:04.2: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:04.55 +56:05:04.2: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 04.55 +56 05 04.2 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J023102.07+560506.0,2461228.7512,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023102.07+560506.0 20260707.2512 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.55 02:31:32.20 +56:41:26.6
136.39056 -3.54254 galactic Per 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 | Gaia DR3 457585613854845952 | 02:31:32.49 +56:41:24.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:32.20 +56:41:26.6: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:32.20 +56:41:26.6: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 32.20 +56 41 26.6 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457585613854845952,2461228.7512,9.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457585613854845952 20260707.2512 9.55CV 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 07 07.2512 2461228.7512 9.53 02:34:20.44 +56:29:01.4
136.82722 -3.58631 galactic Per Second-epoch detections are separated by 1.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5849+56.4836 | 02:34:20.39 +56:29:01.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.231+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:20.44 +56:29:01.4: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:20.44 +56:29:01.4: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 20.44 +56 29 01.4 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.5849+56.4836,2461228.7512,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.5849+56.4836 20260707.2512 9.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.57 02:35:35.89 +56:45:06.5
136.88232 -3.27205 galactic Per Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457785450099520768 | 02:35:36.21 +56:45:09.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:35.89 +56:45:06.5: 13.09 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:35.89 +56:45:06.5: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 35.89 +56 45 06.5 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457785450099520768,2461228.7512,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457785450099520768 20260707.2512 9.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.95 01:18:14.29 +61:44:37.2
126.09868 -0.96319 galactic Cas Second-epoch detections are separated by 0.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:14.29 +61:44:37.2 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:14.29 +61:44:37.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:14.29 +61:44:37.2: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 18 14.29 +61 44 37.2 9.9 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,2461228.7512,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.56 02:34:31.65 +56:11:10.4
136.96666 -3.85054 galactic Per Second-epoch detections are separated by 3.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6110+56.1853 | 02:34:32.06 +56:11:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:31.65 +56:11:10.4: 11.84 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:31.65 +56:11:10.4: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 31.65 +56 11 10.4 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.6110+56.1853,2461228.7512,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.6110+56.1853 20260707.2512 9.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.54 02:30:49.94 +56:26:29.6
136.39436 -3.80990 galactic Per Second-epoch detections are separated by 0.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457575821336762496 | 02:30:50.16 +56:26:30.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.217+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:49.94 +56:26:29.6: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:49.94 +56:26:29.6: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 49.94 +56 26 29.6 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457575821336762496,2461228.7512,9.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457575821336762496 20260707.2512 9.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.55 02:34:41.02 +56:11:01.2
136.98772 -3.84447 galactic Per Second-epoch detections are separated by 3.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6605+56.1803 | 02:34:41.56 +56:11:01.9 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:41.02 +56:11:01.2: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:41.02 +56:11:01.2: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 41.02 +56 11 01.2 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.6605+56.1803,2461228.7512,9.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.6605+56.1803 20260707.2512 9.55CV 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 07 07.2512 2461228.7512 9.85 01:58:16.33 +59:38:58.0
131.29081 -2.13325 galactic Cas Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:58:16.33 +59:38:58.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:16.33 +59:38:58.0: 12.65 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:16.33 +59:38:58.0: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 58 16.33 +59 38 58.0 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 9.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.94 00:58:55.96 +58:04:06.0
123.92627 -4.78894 galactic Cas Second-epoch detections are separated by 0.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:58:55.96 +58:04:06.0 (user input) | T | P | (position from user input) J-Ks=0.236+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:58:55.96 +58:04:06.0: 12.14 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:58:55.96 +58:04:06.0: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 58 55.96 +58 04 06.0 9.9 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,2461228.7512,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.58 02:36:20.12 +56:57:28.9
136.89405 -3.04282 galactic Per Second-epoch detections are separated by 0.4" and 6.1 pix
The object was found in VSX 4" ASASSN-V J023620.50+565726.0
Type: SRS
# Max. Min./Amp. JD0 Period
13.140 V 13.240 V 2457613.04700 25.122000000000
ATTENTION: measured mag 9.58 is 3.6 mag brighter than the VSX record maximum brightness 13.14 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:20.12 +56:57:28.9: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:20.12 +56:57:28.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 36 20.12 +56 57 28.9 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J023620.50+565726.0,2461228.7512,9.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023620.50+565726.0 20260707.2512 9.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.66 02:34:07.76 +56:29:06.5
136.79972 -3.59629 galactic Per Second-epoch detections are separated by 2.6" and 5.8 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 | 02:34:07.76 +56:29:06.5 (user input) | T | P | (position from user input) J-Ks=0.256+/-0.040 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:07.76 +56:29:06.5: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:07.76 +56:29:06.5: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 07.76 +56 29 06.5 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 9.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.06 01:20:56.93 +62:03:29.7
126.38166 -0.61567 galactic Cas Second-epoch detections are separated by 1.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 510938036905942144 | 01:20:56.96 +62:03:30.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.519+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:56.93 +62:03:29.7: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:56.93 +62:03:29.7: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 20 56.93 +62 03 29.7 10.1 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 510938036905942144,2461228.7512,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 510938036905942144 20260707.2512 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.65 02:30:26.95 +56:10:13.2
136.44669 -4.08130 galactic Per Second-epoch detections are separated by 1.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457361107331848064 | 02:30:27.25 +56:10:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:26.95 +56:10:13.2: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:26.95 +56:10:13.2: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 26.95 +56 10 13.2 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457361107331848064,2461228.7512,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457361107331848064 20260707.2512 9.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.77 02:32:54.24 +56:43:29.3
136.55151 -3.43978 galactic Per 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 | Gaia DR3 457773385529748864 | 02:32:54.55 +56:43:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.771+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:54.24 +56:43:29.3: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:54.24 +56:43:29.3: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 54.24 +56 43 29.3 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457773385529748864,2461228.7512,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457773385529748864 20260707.2512 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.78 02:37:19.18 +57:14:52.0
136.90223 -2.72384 galactic Per Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457894881562487168 | 02:37:19.41 +57:14:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.357+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:19.18 +57:14:52.0: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:19.18 +57:14:52.0: 12.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 37 19.18 +57 14 52.0 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457894881562487168,2461228.7512,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457894881562487168 20260707.2512 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.69 02:34:09.77 +56:06:36.9
136.94921 -3.94025 galactic Per Second-epoch detections are separated by 3.9" and 6.7 pix
The object was found in VSX 5" Gaia DR3 457324617289144576
Type: RS
# Max. Min./Amp. JD0 Period
12.140 G 12.220 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:09.77 +56:06:36.9: 12.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:09.77 +56:06:36.9: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 09.77 +56 06 36.9 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457324617289144576,2461228.7512,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457324617289144576 20260707.2512 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.63 02:34:27.75 +56:43:25.0
136.74965 -3.35865 galactic Per Second-epoch detections are separated by 2.0" 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 | ATO J038.6167+56.7240 | 02:34:27.75 +56:43:25.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:27.75 +56:43:25.0: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:27.75 +56:43:25.0: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 27.75 +56 43 25.0 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.6167+56.7240,2461228.7512,9.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.6167+56.7240 20260707.2512 9.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.69 02:29:16.26 +56:06:17.5
136.31831 -4.20306 galactic Per Second-epoch detections are separated by 2.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457546718637685760 | 02:29:16.73 +56:06:18.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:16.26 +56:06:17.5: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:16.26 +56:06:17.5: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 16.26 +56 06 17.5 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457546718637685760,2461228.7512,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457546718637685760 20260707.2512 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.32 00:36:55.88 +62:32:57.4
121.26095 -0.27540 galactic Cas Second-epoch detections are separated by 3.0" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 430697366244614272 | 00:37:00.66 +62:32:35.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1956PMcCO..13a....B AG+62 73
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:36:55.88 +62:32:57.4: 12.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:36:55.88 +62:32:57.4: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 07 07.2512* 00 36 55.88 +62 32 57.4 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430697366244614272,2461228.7512,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 430697366244614272 20260707.2512 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.72 02:32:36.04 +56:17:21.3
136.67926 -3.85836 galactic Per Second-epoch detections are separated by 2.1" 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 | ATO J038.1553+56.2815 | 02:32:36.50 +56:17:21.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:36.04 +56:17:21.3: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:36.04 +56:17:21.3: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 36.04 +56 17 21.3 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.1553+56.2815,2461228.7512,9.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.1553+56.2815 20260707.2512 9.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.74 02:33:10.79 +56:00:07.1
136.86403 -4.09301 galactic Per Second-epoch detections are separated by 2.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457363993551045760 | 02:33:06.84 +56:00:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:10.79 +56:00:07.1: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:10.79 +56:00:07.1: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 10.79 +56 00 07.1 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457363993551045760,2461228.7512,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457363993551045760 20260707.2512 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.75 02:34:25.23 +56:10:43.9
136.95576 -3.86310 galactic Per Second-epoch detections are separated by 2.6" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457325957318911616 | 02:34:25.79 +56:10:43.5 (Gaia DR3) | E (local) | 3.840110000000 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:25.23 +56:10:43.9: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:25.23 +56:10:43.9: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 25.23 +56 10 43.9 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457325957318911616,2461228.7512,9.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457325957318911616 20260707.2512 9.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.79 02:34:50.44 +56:14:15.1
136.98690 -3.78636 galactic Per Second-epoch detections are separated by 1.0" and 6.3 pix
The object was found in VSX 4" GPX-TF8A-1104
Type: ROT
# Max. Min./Amp. JD0 Period
12.380 V 12.640 V 2457600.79000 1.894100000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:50.44 +56:14:15.1: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:50.44 +56:14:15.1: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 50.44 +56 14 15.1 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GPX-TF8A-1104,2461228.7512,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GPX-TF8A-1104 20260707.2512 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.72 02:35:36.46 +56:50:34.4
136.84782 -3.18772 galactic Per Second-epoch detections are separated by 3.0" and 5.7 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 457789225369131136 | 02:35:36.20 +56:50:29.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:36.46 +56:50:34.4: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:36.46 +56:50:34.4: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 36.46 +56 50 34.4 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457789225369131136,2461228.7512,9.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457789225369131136 20260707.2512 9.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.66 02:34:18.67 +56:07:36.4
136.96191 -3.91702 galactic Per Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5805+56.1272 | 02:34:19.32 +56:07:38.2 (Gaia DR3) | SINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:18.67 +56:07:36.4: 12.21 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:18.67 +56:07:36.4: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 18.67 +56 07 36.4 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.5805+56.1272,2461228.7512,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.5805+56.1272 20260707.2512 9.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.11 01:29:33.01 +61:46:26.5
127.42247 -0.76497 galactic Cas Second-epoch detections are separated by 1.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:29:33.01 +61:46:26.5 (user input) | T | P | (position from user input) J-Ks=0.908+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:33.01 +61:46:26.5: 12.95 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:33.01 +61:46:26.5: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 29 33.01 +61 46 26.5 10.1 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,2461228.7512,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.74 02:32:56.64 +56:40:53.9
136.57312 -3.47758 galactic Per Second-epoch detections are separated by 2.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.2275+56.6930 | 02:32:56.88 +56:40:52.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.724+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:56.64 +56:40:53.9: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:56.64 +56:40:53.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 56.64 +56 40 53.9 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.2275+56.6930,2461228.7512,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.2275+56.6930 20260707.2512 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.79 02:29:17.29 +56:14:27.8
136.27009 -4.07562 galactic Per Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.3264+56.2443 | 02:29:17.29 +56:14:27.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:17.29 +56:14:27.8: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:17.29 +56:14:27.8: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 17.29 +56 14 27.8 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.3264+56.2443,2461228.7512,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.3264+56.2443 20260707.2512 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.76 02:34:14.18 +56:14:09.6
136.90993 -3.82033 galactic Per Second-epoch detections are separated by 1.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457326399692569216 | 02:34:14.66 +56:14:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:14.18 +56:14:09.6: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:14.18 +56:14:09.6: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 14.18 +56 14 09.6 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457326399692569216,2461228.7512,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457326399692569216 20260707.2512 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.73 02:33:48.88 +56:37:03.6
136.70842 -3.49075 galactic Per Second-epoch detections are separated by 1.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.4542+56.6177 | 02:33:49.01 +56:37:03.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.940+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:48.88 +56:37:03.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:48.88 +56:37:03.6: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 48.88 +56 37 03.6 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.4542+56.6177,2461228.7512,9.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.4542+56.6177 20260707.2512 9.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.82 02:33:06.38 +56:40:26.3
136.59669 -3.47614 galactic Per Second-epoch detections are separated by 1.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457773011874358656 | 02:33:06.63 +56:40:27.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.512+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:06.38 +56:40:26.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:06.38 +56:40:26.3: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 06.38 +56 40 26.3 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457773011874358656,2461228.7512,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457773011874358656 20260707.2512 9.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.84 02:30:25.27 +56:22:03.9
136.36917 -3.89962 galactic Per Second-epoch detections are separated by 1.9" and 6.0 pix
The object was found in VSX 2" GPX-TF8A-1480
Type: DSCT
# Max. Min./Amp. JD0 Period
12.420 V 12.450 V 2457007.82350 0.087013000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:25.27 +56:22:03.9: 12.03 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:25.27 +56:22:03.9: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 25.27 +56 22 03.9 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GPX-TF8A-1480,2461228.7512,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GPX-TF8A-1480 20260707.2512 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.79 02:33:21.47 +56:24:37.7
136.72994 -3.70624 galactic Per Second-epoch detections are separated by 4.2" 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 | Gaia DR3 457378935732571392 | 02:33:21.33 +56:24:34.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:21.47 +56:24:37.7: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:21.47 +56:24:37.7: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 21.47 +56 24 37.7 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457378935732571392,2461228.7512,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457378935732571392 20260707.2512 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.70 02:30:31.77 +56:03:29.5
136.49913 -4.18113 galactic Per Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.6353+56.0504 | 02:30:32.40 +56:03:28.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:31.77 +56:03:29.5: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:31.77 +56:03:29.5: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 31.77 +56 03 29.5 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.6353+56.0504,2461228.7512,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.6353+56.0504 20260707.2512 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.82 02:36:24.29 +56:49:27.5
136.95555 -3.16199 galactic Per Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.1040+56.8238 | 02:36:24.98 +56:49:25.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:24.29 +56:49:27.5: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:24.29 +56:49:27.5: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 36 24.29 +56 49 27.5 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J039.1040+56.8238,2461228.7512,9.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.1040+56.8238 20260707.2512 9.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.21 01:22:23.94 +61:13:51.6
126.64957 -1.41706 galactic Cas Second-epoch detections are separated by 1.0" and 5.5 pix
The object was found in VSX 1" NSVS J0122238+611352
Type: M
# Max. Min./Amp. JD0 Period
14.871 r Y 3.740 r 2458328.87710 325.120339600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:23.94 +61:13:51.6: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:23.94 +61:13:51.6: 15.76 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.76 +/- 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 07 07.2512* 01 22 23.94 +61 13 51.6 10.2 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
NSVS J0122238+611352,2461228.7512,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0122238+611352 20260707.2512 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.81 02:31:05.38 +56:00:31.6
136.59043 -4.19761 galactic Per Second-epoch detections are separated by 2.1" 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 | Gaia DR3 457355163097206784 | 02:31:00.46 +56:00:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:05.38 +56:00:31.6: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:05.38 +56:00:31.6: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 05.38 +56 00 31.6 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457355163097206784,2461228.7512,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457355163097206784 20260707.2512 9.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.88 02:32:31.70 +56:04:31.5
136.75160 -4.05990 galactic Per Second-epoch detections are separated by 1.7" and 6.6 pix
The object was found in VSX18" Gaia DR3 457365299221088896
Type: ROT
# Max. Min./Amp. JD0 Period
14.750 G 14.800 G G
ATTENTION: measured mag 9.88 is 4.9 mag brighter than the VSX record maximum brightness 14.75 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:31.70 +56:04:31.5: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:31.70 +56:04:31.5: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 31.70 +56 04 31.5 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457365299221088896,2461228.7512,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457365299221088896 20260707.2512 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.94 02:32:32.91 +56:21:52.5
136.64380 -3.79146 galactic Per Second-epoch detections are separated by 3.4" and 6.7 pix
The object was found in VSX 6" Gaia DR3 457388831340431104
Type: E
# Max. Min./Amp. JD0 Period
18.340 G 18.680 G 0.272690000000
ATTENTION: measured mag 9.94 is 8.4 mag brighter than the VSX record maximum brightness 18.34 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:32.91 +56:21:52.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:32.91 +56:21:52.5: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 32.91 +56 21 52.5 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457388831340431104,2461228.7512,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457388831340431104 20260707.2512 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.88 02:32:29.84 +55:59:08.6
136.78184 -4.14448 galactic Per Second-epoch detections are separated by 4.3" and 5.6 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 J038.1327+55.9847 | 02:32:30.22 +55:59:10.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:29.84 +55:59:08.6: 12.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:29.84 +55:59:08.6: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 29.84 +55 59 08.6 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.1327+55.9847,2461228.7512,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.1327+55.9847 20260707.2512 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.99 02:31:57.79 +56:05:41.6
136.67108 -4.07184 galactic Per 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 | ATO J037.9859+56.1042 | 02:31:58.14 +56:05:42.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:57.79 +56:05:41.6: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:57.79 +56:05:41.6: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 57.79 +56 05 41.6 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.9859+56.1042,2461228.7512,9.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.9859+56.1042 20260707.2512 9.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.52 00:52:12.50 +64:57:21.6
123.01350 2.08437 galactic Cas Second-epoch detections are separated by 1.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 524435405436784000 | 00:52:06.66 +64:57:18.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1966UppAn...5d...1O [O66] 9: 83 J-Ks=0.408+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:12.50 +64:57:21.6: 12.62 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:12.50 +64:57:21.6: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 52 12.50 +64 57 21.6 10.5 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 524435405436784000,2461228.7512,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 524435405436784000 20260707.2512 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.97 02:34:01.32 +56:28:57.2
136.78702 -3.60439 galactic Per Second-epoch detections are separated by 2.8" 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 J038.5076+56.4818 | 02:34:01.83 +56:28:54.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:01.32 +56:28:57.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:01.32 +56:28:57.2: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 01.32 +56 28 57.2 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.5076+56.4818,2461228.7512,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.5076+56.4818 20260707.2512 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.92 02:24:56.80 +56:48:21.5
135.50583 -3.76551 galactic Per Second-epoch detections are separated by 0.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:24:56.80 +56:48:21.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:56.80 +56:48:21.5: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:56.80 +56:48:21.5: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 24 56.80 +56 48 21.5 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,9.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 9.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.88 02:34:29.42 +56:26:00.5
136.86583 -3.62463 galactic Per Second-epoch detections are separated by 0.6" 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 J038.6238+56.4333 | 02:34:29.71 +56:26:00.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.771+/-0.029 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:29.42 +56:26:00.5: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:29.42 +56:26:00.5: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 29.42 +56 26 00.5 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.6238+56.4333,2461228.7512,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.6238+56.4333 20260707.2512 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.03 02:34:22.66 +56:27:54.2
136.83919 -3.60155 galactic Per Second-epoch detections are separated by 2.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457752396031468416 | 02:34:23.09 +56:27:53.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:22.66 +56:27:54.2: 12.27 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:22.66 +56:27:54.2: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 22.66 +56 27 54.2 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457752396031468416,2461228.7512,10.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457752396031468416 20260707.2512 10.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.88 02:27:24.27 +56:18:01.8
136.00432 -4.11605 galactic Per Second-epoch detections are separated by 1.8" 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 | ATO J036.8584+56.2997 | 02:27:24.37 +56:17:58.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:24.27 +56:18:01.8: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:24.27 +56:18:01.8: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 27 24.27 +56 18 01.8 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J036.8584+56.2997,2461228.7512,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J036.8584+56.2997 20260707.2512 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.93 02:33:00.93 +56:09:31.2
136.78265 -3.95703 galactic Per Second-epoch detections are separated by 1.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:33:00.93 +56:09:31.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:00.93 +56:09:31.2: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:00.93 +56:09:31.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 00.93 +56 09 31.2 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.00 02:31:09.24 +56:03:13.3
136.58185 -4.15261 galactic Per Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457355884651667456 | 02:31:09.69 +56:03:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:09.24 +56:03:13.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:09.24 +56:03:13.3: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 09.24 +56 03 13.3 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457355884651667456,2461228.7512,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457355884651667456 20260707.2512 10.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.12 02:30:43.64 +56:25:16.2
136.38853 -3.83424 galactic Per Second-epoch detections are separated by 2.7" 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 | 02:30:43.64 +56:25:16.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:43.64 +56:25:16.2: 12.14 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:43.64 +56:25:16.2: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 43.64 +56 25 16.2 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.06 02:31:06.56 +56:11:58.4
136.52108 -4.01979 galactic Per Second-epoch detections are separated by 1.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457380864182360448 | 02:31:06.89 +56:11:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:06.56 +56:11:58.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:06.56 +56:11:58.4: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 06.56 +56 11 58.4 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457380864182360448,2461228.7512,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457380864182360448 20260707.2512 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.88 02:29:37.98 +56:28:56.4
136.22506 -3.83380 galactic Per Second-epoch detections are separated by 2.6" and 6.1 pix
The object was found in VSX12" Gaia DR3 457578913713211520
Type: ROT
# Max. Min./Amp. JD0 Period
15.070 G 15.110 G F
ATTENTION: measured mag 9.88 is 5.2 mag brighter than the VSX record maximum brightness 15.07 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:37.98 +56:28:56.4: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:37.98 +56:28:56.4: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 37.98 +56 28 56.4 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457578913713211520,2461228.7512,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457578913713211520 20260707.2512 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.98 02:31:42.63 +56:28:20.1
136.49542 -3.73581 galactic Per Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457394127041197312 | 02:31:42.96 +56:28:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:42.63 +56:28:20.1: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:42.63 +56:28:20.1: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 42.63 +56 28 20.1 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457394127041197312,2461228.7512,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457394127041197312 20260707.2512 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.02 02:35:20.59 +56:30:28.5
136.94550 -3.51023 galactic Per Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8377+56.5074 | 02:35:21.06 +56:30:26.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:20.59 +56:30:28.5: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:20.59 +56:30:28.5: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 20.59 +56 30 28.5 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.8377+56.5074,2461228.7512,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.8377+56.5074 20260707.2512 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.89 02:30:09.49 +56:13:06.4
136.39105 -4.05176 galactic Per Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457549123819532032 | 02:30:10.01 +56:13:05.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:09.49 +56:13:06.4: 12.76 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:09.49 +56:13:06.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 09.49 +56 13 06.4 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457549123819532032,2461228.7512,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457549123819532032 20260707.2512 9.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.11 02:34:14.15 +56:41:49.8
136.73117 -3.39507 galactic Per Second-epoch detections are separated by 1.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 457775623214421632 | 02:34:14.15 +56:41:49.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.437+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:14.15 +56:41:49.8: 11.84 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:14.15 +56:41:49.8: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 14.15 +56 41 49.8 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457775623214421632,2461228.7512,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457775623214421632 20260707.2512 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.87 02:32:08.77 +55:55:37.5
136.75862 -4.21740 galactic Per Second-epoch detections are separated by 3.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.0417+55.9259 | 02:32:08.77 +55:55:37.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.414+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:08.77 +55:55:37.5: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:08.77 +55:55:37.5: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 08.77 +55 55 37.5 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.0417+55.9259,2461228.7512,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.0417+55.9259 20260707.2512 9.87CV 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 07 07.2512 2461228.7512 9.90 02:30:43.84 +56:23:45.5
136.39841 -3.85743 galactic Per Second-epoch detections are separated by 3.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457575168501767424 | 02:30:44.21 +56:23:43.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:43.84 +56:23:45.5: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:43.84 +56:23:45.5: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 43.84 +56 23 45.5 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457575168501767424,2461228.7512,9.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457575168501767424 20260707.2512 9.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.12 02:36:19.80 +56:48:29.7
136.95246 -3.18078 galactic Per Second-epoch detections are separated by 1.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:36:19.80 +56:48:29.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:19.80 +56:48:29.7: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:19.80 +56:48:29.7: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 36 19.80 +56 48 29.7 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.13 02:26:52.95 +56:05:48.3
136.01040 -4.33226 galactic Per Second-epoch detections are separated by 4.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:26:52.95 +56:05:48.3 (user input) | T | P | (position from user input) J-Ks=0.279+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:52.95 +56:05:48.3: 10.04 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:52.95 +56:05:48.3: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 26 52.95 +56 05 48.3 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.07 02:30:10.17 +56:16:14.7
136.37298 -4.00264 galactic Per Second-epoch detections are separated by 1.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:30:10.17 +56:16:14.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:10.17 +56:16:14.7: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:10.17 +56:16:14.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 10.17 +56 16 14.7 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.44 00:51:32.84 +59:59:12.6
122.94562 -2.88491 galactic Cas Second-epoch detections are separated by 2.0" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426864434349441664 | 00:51:36.39 +59:59:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.041 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:32.84 +59:59:12.6: 11.12 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:32.84 +59:59:12.6: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 51 32.84 +59 59 12.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426864434349441664,2461228.7512,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 426864434349441664 20260707.2512 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.48 00:47:11.57 +58:29:06.7
122.37557 -4.38197 galactic Cas Second-epoch detections are separated by 3.9" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J011.7996+58.4919 | 00:47:11.57 +58:29:06.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A6IV (LAMOST DR5)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:47:11.57 +58:29:06.7: 11.35 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:47:11.57 +58:29:06.7: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 47 11.57 +58 29 06.7 10.5 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 J011.7996+58.4919,2461228.7512,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011.7996+58.4919 20260707.2512 10.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.04 02:31:28.87 +56:18:16.5
136.52940 -3.90305 galactic Per Second-epoch detections are separated by 0.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.8513+56.3054 | 02:31:28.87 +56:18:16.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:28.87 +56:18:16.5: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:28.87 +56:18:16.5: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 28.87 +56 18 16.5 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.8513+56.3054,2461228.7512,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.8513+56.3054 20260707.2512 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.07 02:30:53.06 +56:31:32.6
136.36940 -3.72918 galactic Per Second-epoch detections are separated by 0.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457582688983611904 | 02:30:53.28 +56:31:32.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.348+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:53.06 +56:31:32.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:53.06 +56:31:32.6: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 53.06 +56 31 32.6 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457582688983611904,2461228.7512,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457582688983611904 20260707.2512 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.05 02:27:18.79 +56:05:55.8
136.06579 -4.30859 galactic Per Second-epoch detections are separated by 2.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457461673982952192 | 02:27:18.75 +56:05:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.477+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:18.79 +56:05:55.8: 11.69 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:18.79 +56:05:55.8: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 27 18.79 +56 05 55.8 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457461673982952192,2461228.7512,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457461673982952192 20260707.2512 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.11 02:33:06.79 +56:01:45.3
136.84493 -4.07138 galactic Per Second-epoch detections are separated by 3.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457364092325569536 | 02:33:07.21 +56:01:46.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:06.79 +56:01:45.3: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:06.79 +56:01:45.3: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 06.79 +56 01 45.3 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457364092325569536,2461228.7512,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457364092325569536 20260707.2512 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.19 02:31:41.25 +56:32:00.9
136.46925 -3.68022 galactic Per Second-epoch detections are separated by 2.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:31:41.25 +56:32:00.9 (user input) | T | P | (position from user input) J-Ks=0.765+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:41.25 +56:32:00.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:41.25 +56:32:00.9: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 41.25 +56 32 00.9 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.12 02:30:31.12 +56:33:56.5
136.30758 -3.71098 galactic Per Second-epoch detections are separated by 1.3" 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 | ATO J037.6520+56.5687 | 02:30:31.30 +56:33:55.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.945+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:31.12 +56:33:56.5: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:31.12 +56:33:56.5: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 31.12 +56 33 56.5 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.6520+56.5687,2461228.7512,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.6520+56.5687 20260707.2512 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.67 01:19:41.75 +62:51:05.3
126.14897 0.15636 galactic Cas Second-epoch detections are separated by 2.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:19:41.75 +62:51:05.3 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:41.75 +62:51:05.3: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:41.75 +62:51:05.3: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 19 41.75 +62 51 05.3 10.7 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,2461228.7512,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.15 02:31:35.16 +56:11:21.0
136.58658 -4.00444 galactic Per Second-epoch detections are separated by 2.6" and 6.6 pix
The object was found in VSX 4" Gaia DR3 457380314426542848
Type: ROT
# Max. Min./Amp. JD0 Period
12.620 G 12.650 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:35.16 +56:11:21.0: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:35.16 +56:11:21.0: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 35.16 +56 11 21.0 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457380314426542848,2461228.7512,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457380314426542848 20260707.2512 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.39 01:13:12.83 +60:19:03.4
125.62711 -2.44013 galactic Cas Second-epoch detections are separated by 7.6" and 5.3 pix
The object was found in VSX 5" Gaia DR3 510403261937788160
Type: L
# Max. Min./Amp. JD0 Period
12.340 G 12.490 G M
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:12.83 +60:19:03.4: 12.34 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:12.83 +60:19:03.4: 13.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 13 12.83 +60 19 03.4 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510403261937788160,2461228.7512,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 510403261937788160 20260707.2512 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.13 02:32:40.03 +56:36:59.2
136.56281 -3.55236 galactic Per Second-epoch detections are separated by 2.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:40.03 +56:36:59.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:40.03 +56:36:59.2: 11.13 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:40.03 +56:36:59.2: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 40.03 +56 36 59.2 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.13 02:32:47.85 +56:09:08.3
136.75697 -3.97451 galactic Per Second-epoch detections are separated by 1.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:47.85 +56:09:08.3 (user input) | T | P | (position from user input) J-Ks=0.762+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:47.85 +56:09:08.3: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:47.85 +56:09:08.3: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 47.85 +56 09 08.3 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.46 00:45:38.04 +56:46:39.0
122.13249 -6.08524 galactic Cas Second-epoch detections are separated by 7.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 00:45:38.04 +56:46:39.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:45:38.04 +56:46:39.0: 11.18 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:45:38.04 +56:46:39.0: 13.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 45 38.04 +56 46 39.0 10.5 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,2461228.7512,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.27 02:36:38.41 +57:22:31.7
136.76727 -2.64291 galactic Per Second-epoch detections are separated by 1.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:36:38.41 +57:22:31.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:38.41 +57:22:31.7: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:38.41 +57:22:31.7: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 36 38.41 +57 22 31.7 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.55 01:41:54.61 +62:34:04.7
128.70797 0.26361 galactic Cas Second-epoch detections are separated by 1.1" and 5.2 pix
The object was found in VSX 1" NSVS J0141549+623406
Type: M
# Max. Min./Amp. JD0 Period
14.358 r Y 4.570 r 2458452.99090 303.989771700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:54.61 +62:34:04.7: 13.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:54.61 +62:34:04.7: 15.44 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.44 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 41 54.61 +62 34 04.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0141549+623406,2461228.7512,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0141549+623406 20260707.2512 10.55CV 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 07 07.2512 2461228.7512 10.29 02:34:49.29 +56:45:55.6
136.77882 -3.30100 galactic Per Second-epoch detections are separated by 2.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.7078+56.7658 | 02:34:49.29 +56:45:55.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:49.29 +56:45:55.6: 10.72 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:49.29 +56:45:55.6: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 49.29 +56 45 55.6 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.7078+56.7658,2461228.7512,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.7078+56.7658 20260707.2512 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.62 00:54:25.48 +60:12:30.6
123.30330 -2.66110 galactic Cas Second-epoch detections are separated by 1.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 426149030239670016 | 00:54:21.76 +60:12:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1935BSD...C01....0S BSD 8- 343 J-Ks=0.402+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:54:25.48 +60:12:30.6: 11.31 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:54:25.48 +60:12:30.6: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 54 25.48 +60 12 30.6 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426149030239670016,2461228.7512,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 426149030239670016 20260707.2512 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.19 02:29:02.28 +56:16:34.5
136.22470 -4.05573 galactic Per Second-epoch detections are separated by 3.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:29:02.28 +56:16:34.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:02.28 +56:16:34.5: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:02.28 +56:16:34.5: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 02.28 +56 16 34.5 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.87 00:41:56.47 +63:42:31.2
121.88043 0.85631 galactic Cas Second-epoch detections are separated by 1.7" and 4.5 pix
The object was found in VSX 3" ASASSN-V J004155.99+634230.1
Type: SR
# Max. Min./Amp. JD0 Period
15.300 V < 16.900 V 2457638.00000 372.000000000000
ATTENTION: measured mag 10.87 is 4.4 mag brighter than the VSX record maximum brightness 15.30 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:41:56.47 +63:42:31.2: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:41:56.47 +63:42:31.2: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 41 56.47 +63 42 31.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J004155.99+634230.1,2461228.7512,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J004155.99+634230.1 20260707.2512 10.87CV 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 07 07.2512 2461228.7512 10.23 02:31:41.77 +56:00:50.9
136.66713 -4.16069 galactic Per Second-epoch detections are separated by 2.2" and 6.6 pix
The object was found in VSX 7" Gaia DR3 457343686944562560
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.950 G 12.980 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:41.77 +56:00:50.9: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:41.77 +56:00:50.9: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 41.77 +56 00 50.9 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457343686944562560,2461228.7512,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457343686944562560 20260707.2512 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.20 02:36:51.36 +57:09:36.5
136.87929 -2.82918 galactic Per Second-epoch detections are separated by 3.5" and 5.7 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 J039.2227+57.1583 | 02:36:51.36 +57:09:36.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.719+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:51.36 +57:09:36.5: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:51.36 +57:09:36.5: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 36 51.36 +57 09 36.5 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J039.2227+57.1583,2461228.7512,10.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.2227+57.1583 20260707.2512 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.33 02:30:46.17 +56:43:56.8
136.27711 -3.54344 galactic Per Second-epoch detections are separated by 2.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.6884+56.7331 | 02:30:46.17 +56:43:56.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:46.17 +56:43:56.8: 11.51 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:46.17 +56:43:56.8: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 46.17 +56 43 56.8 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.6884+56.7331,2461228.7512,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.6884+56.7331 20260707.2512 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.22 02:35:58.60 +56:46:23.5
136.92171 -3.23204 galactic Per Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:35:58.60 +56:46:23.5 (user input) | T | P | (position from user input) J-Ks=0.267+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:58.60 +56:46:23.5: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:58.60 +56:46:23.5: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 58.60 +56 46 23.5 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.22CV 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 07 07.2512 2461228.7512 10.13 02:32:16.64 +56:27:15.9
136.57479 -3.72265 galactic Per Second-epoch detections are separated by 2.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:32:16.64 +56:27:15.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:16.64 +56:27:15.9: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:16.64 +56:27:15.9: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 16.64 +56 27 15.9 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.24 02:27:39.64 +56:13:54.9
136.06252 -4.16703 galactic Per Second-epoch detections are separated by 6.3" 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 | 02:27:39.64 +56:13:54.9 (user input) | T | P | (position from user input) J-Ks=0.660+/-0.026 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:39.64 +56:13:54.9: 12.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:39.64 +56:13:54.9: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 27 39.64 +56 13 54.9 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.29 02:35:00.66 +56:49:39.3
136.77855 -3.23366 galactic Per Second-epoch detections are separated by 1.2" and 6.3 pix
The object was found in VSX11" Gaia DR3 457789676348544640
Type: ROT
# Max. Min./Amp. JD0 Period
16.380 G 16.410 G K
ATTENTION: measured mag 10.29 is 6.1 mag brighter than the VSX record maximum brightness 16.38 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:00.66 +56:49:39.3: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:00.66 +56:49:39.3: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 00.66 +56 49 39.3 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457789676348544640,2461228.7512,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457789676348544640 20260707.2512 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.49 02:10:24.12 +60:01:13.6
132.65156 -1.35274 galactic Cas Second-epoch detections are separated by 1.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:10:24.12 +60:01:13.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.329+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:24.12 +60:01:13.6: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:24.12 +60:01:13.6: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 07 07.2512* 02 10 24.12 +60 01 13.6 10.5 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,2461228.7512,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.38 02:35:30.82 +56:47:10.6
136.85814 -3.24485 galactic Per Second-epoch detections are separated by 1.5" and 6.1 pix
The object was found in VSX 8" ASASSN-V J023531.65+564707.2
Type: SR
# Max. Min./Amp. JD0 Period
15.900 g Y 0.630 g 2459413.08000 82.930000000000
ATTENTION: measured mag 10.38 is 4.9 mag brighter than the VSX record maximum brightness 15.27 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:30.82 +56:47:10.6: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:30.82 +56:47:10.6: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 35 30.82 +56 47 10.6 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J023531.65+564707.2,2461228.7512,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023531.65+564707.2 20260707.2512 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.64 01:18:36.81 +58:41:39.1
126.46460 -3.99103 galactic Cas Second-epoch detections are separated by 2.2" and 5.7 pix
The object was found in VSX22" Gaia DR3 413902596701682816
Type: ROT
# Max. Min./Amp. JD0 Period
15.180 G 15.220 G K
ATTENTION: measured mag 10.64 is 4.5 mag brighter than the VSX record maximum brightness 15.18 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:36.81 +58:41:39.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:36.81 +58:41:39.1: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 07 07.2512* 01 18 36.81 +58 41 39.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413902596701682816,2461228.7512,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 413902596701682816 20260707.2512 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.61 01:38:33.84 +60:47:25.3
128.65255 -1.55688 galactic Cas Second-epoch detections are separated by 0.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:38:33.84 +60:47:25.3 (user input) | T | P | (position from user input) J-Ks=0.216+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:33.84 +60:47:25.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:33.84 +60:47:25.3: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 38 33.84 +60 47 25.3 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.93 00:39:40.06 +61:06:36.3
121.51011 -1.72917 galactic Cas Second-epoch detections are separated by 1.0" and 5.0 pix
The object was found in VSX 1" Gaia DR3 427216930905906176
Type: VAR
# Max. Min./Amp. JD0 Period
13.680 G 13.770 G 0.014693700000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:39:40.06 +61:06:36.3: 12.39 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:39:40.06 +61:06:36.3: 13.80 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 00 39 40.06 +61 06 36.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 427216930905906176,2461228.7512,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 427216930905906176 20260707.2512 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.38 02:32:40.73 +56:57:45.9
136.43207 -3.23158 galactic Per Second-epoch detections are separated by 2.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.1703+56.9612 | 02:32:40.73 +56:57:45.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:40.73 +56:57:45.9: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:40.73 +56:57:45.9: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 40.73 +56 57 45.9 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.1703+56.9612,2461228.7512,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.1703+56.9612 20260707.2512 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.51 01:59:33.54 +60:01:44.6
131.34889 -1.72476 galactic Cas Second-epoch detections are separated by 1.9" and 5.9 pix
The object was found in VSX17" ZTF J015934.53+600159.8
Type: SR
# Max. Min./Amp. JD0 Period
15.783 r Y 0.432 r 2458492.34860 197.227334200000
ATTENTION: measured mag 10.51 is 4.8 mag brighter than the VSX record maximum brightness 15.35 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:33.54 +60:01:44.6: 13.52 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:33.54 +60:01:44.6: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 07 07.2512* 01 59 33.54 +60 01 44.6 10.5 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 J015934.53+600159.8,2461228.7512,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015934.53+600159.8 20260707.2512 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.49 02:31:36.56 +56:43:54.7
136.38426 -3.50068 galactic Per Second-epoch detections are separated by 1.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9034+56.7337 | 02:31:36.56 +56:43:54.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:36.56 +56:43:54.7: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:36.56 +56:43:54.7: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 36.56 +56 43 54.7 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.9034+56.7337,2461228.7512,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.9034+56.7337 20260707.2512 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.86 01:31:48.39 +64:21:55.8
127.28193 1.83524 galactic Cas Second-epoch detections are separated by 1.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:31:48.39 +64:21:55.8 (user input) | T | P | (position from user input) J-Ks=0.974+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.39 +64:21:55.8: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.39 +64:21:55.8: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 31 48.39 +64 21 55.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.38 02:36:01.82 +56:57:52.5
136.85319 -3.05315 galactic Per Second-epoch detections are separated by 3.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:36:01.82 +56:57:52.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:01.82 +56:57:52.5: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:01.82 +56:57:52.5: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 36 01.82 +56 57 52.5 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.35 02:31:05.41 +56:13:06.4
136.51149 -4.00329 galactic Per Second-epoch detections are separated by 1.8" and 5.9 pix
The object was found in VSX 7" ASASSN-V J023106.14+561303.8
Type: SR
# Max. Min./Amp. JD0 Period
15.100 g Y 0.300 g 2459399.10000 36.910000000000
ATTENTION: measured mag 10.35 is 4.4 mag brighter than the VSX record maximum brightness 14.80 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:05.41 +56:13:06.4: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:05.41 +56:13:06.4: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 05.41 +56 13 06.4 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J023106.14+561303.8,2461228.7512,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J023106.14+561303.8 20260707.2512 10.35CV 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 07 07.2512 2461228.7512 10.19 02:32:56.45 +56:04:07.6
136.80748 -4.04407 galactic Per Second-epoch detections are separated by 2.8" 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 | Gaia DR3 457365501074840320 | 02:32:56.93 +56:04:05.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:56.45 +56:04:07.6: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:56.45 +56:04:07.6: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 56.45 +56 04 07.6 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457365501074840320,2461228.7512,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457365501074840320 20260707.2512 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.84 01:29:32.94 +63:19:37.2
127.19354 0.77103 galactic Cas Second-epoch detections are separated by 1.6" and 5.5 pix
The object was found in VSX21" Gaia DR3 512422828587465216
Type: S
# Max. Min./Amp. JD0 Period
14.920 G 15.600 G A
ATTENTION: measured mag 10.84 is 4.1 mag brighter than the VSX record maximum brightness 14.92 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:32.94 +63:19:37.2: 12.84 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:32.94 +63:19:37.2: 13.51 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 29 32.94 +63 19 37.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512422828587465216,2461228.7512,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 512422828587465216 20260707.2512 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.88 01:18:48.37 +64:12:21.1
125.90444 1.49218 galactic Cas Second-epoch detections are separated by 0.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:18:48.37 +64:12:21.1 (user input) | T | P | (position from user input) J-Ks=0.908+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:48.37 +64:12:21.1: 11.63 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:48.37 +64:12:21.1: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 07 07.2512* 01 18 48.37 +64 12 21.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.65 01:56:32.59 +59:56:29.5
131.00640 -1.90563 galactic Cas Second-epoch detections are separated by 1.7" and 5.6 pix
The object was found in VSX 0" NSV 15406
Type: M
# Max. Min./Amp. JD0 Period
12.800 V 15.000 V 409.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:32.59 +59:56:29.5: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:32.59 +59:56:29.5: 16.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 56 32.59 +59 56 29.5 10.7 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
NSV 15406,2461228.7512,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 15406 20260707.2512 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.65 02:01:39.11 +61:45:17.0
131.13773 0.00673 galactic Cas Second-epoch detections are separated by 1.1" and 5.7 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 | 02:01:39.11 +61:45:17.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:39.11 +61:45:17.0: 12.32 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:39.11 +61:45:17.0: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 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 07 07.2512* 02 01 39.11 +61 45 17.0 10.7 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,2461228.7512,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.87 02:01:03.64 +64:43:31.2
130.27883 2.85135 galactic Cas Second-epoch detections are separated by 3.2" and 5.6 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 | 02:01:03.64 +64:43:31.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:03.64 +64:43:31.2: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:03.64 +64:43:31.2: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 01 03.64 +64 43 31.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.87CV 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 07 07.2512 2461228.7512 10.68 02:02:54.02 +60:15:41.6
131.68769 -1.38970 galactic Cas Second-epoch detections are separated by 0.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 507950977353541248 | 02:02:48.33 +60:15:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.870+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:54.02 +60:15:41.6: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:54.02 +60:15:41.6: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 02 54.02 +60 15 41.6 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507950977353541248,2461228.7512,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 507950977353541248 20260707.2512 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.43 02:32:36.48 +56:53:27.0
136.45056 -3.30176 galactic Per Second-epoch detections are separated by 4.3" and 6.7 pix
The object was found in VSX11" Gaia DR3 457968961159054848
Type: ROT
# Max. Min./Amp. JD0 Period
17.610 G 17.690 G K
ATTENTION: measured mag 10.43 is 7.2 mag brighter than the VSX record maximum brightness 17.61 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:36.48 +56:53:27.0: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:36.48 +56:53:27.0: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 36.48 +56 53 27.0 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457968961159054848,2461228.7512,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457968961159054848 20260707.2512 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.84 01:55:53.21 +64:15:24.7
129.86042 2.25553 galactic Cas Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:55:53.21 +64:15:24.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:55:53.21 +64:15:24.7: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:55:53.21 +64:15:24.7: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 55 53.21 +64 15 24.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.87 02:21:38.41 +65:44:30.3
132.02520 4.47518 galactic Cas Second-epoch detections are separated by 2.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 517069845756285184 | 02:21:38.42 +65:45:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:38.41 +65:44:30.3: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:38.41 +65:44:30.3: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 21 38.41 +65 44 30.3 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 517069845756285184,2461228.7512,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 517069845756285184 20260707.2512 10.87CV 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 07 07.2512 2461228.7512 10.76 01:38:06.02 +58:10:36.7
129.06846 -4.13784 galactic Cas Second-epoch detections are separated by 4.0" and 4.9 pix
The object was found in VSX10" Gaia DR3 508962699851411840
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
16.190 G 16.240 G A
ATTENTION: measured mag 10.76 is 5.4 mag brighter than the VSX record maximum brightness 16.19 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:06.02 +58:10:36.7: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:06.02 +58:10:36.7: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 38 06.02 +58 10 36.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508962699851411840,2461228.7512,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 508962699851411840 20260707.2512 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.77 01:59:06.11 +59:55:34.4
131.32039 -1.83892 galactic Cas Second-epoch detections are separated by 1.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 507895516435392512 | 01:59:07.43 +59:54:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B2 1953IzKry..10..120K [K53] 683 J-Ks=0.818+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:06.11 +59:55:34.4: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:06.11 +59:55:34.4: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 07 07.2512* 01 59 06.11 +59 55 34.4 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 507895516435392512,2461228.7512,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 507895516435392512 20260707.2512 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.99 01:31:48.54 +64:22:27.8
127.28081 1.84406 galactic Cas Second-epoch detections are separated by 1.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:31:48.54 +64:22:27.8 (user input) | T | P | (position from user input) J-Ks=0.844+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.54 +64:22:27.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.54 +64:22:27.8: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 31 48.54 +64 22 27.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.62 02:35:15.89 +56:49:40.2
136.81048 -3.21990 galactic Per Second-epoch detections are separated by 1.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8034+56.8391 | 02:35:12.85 +56:50:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:15.89 +56:49:40.2: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:15.89 +56:49:40.2: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 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 07 07.2512* 02 35 15.89 +56 49 40.2 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.8034+56.8391,2461228.7512,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.8034+56.8391 20260707.2512 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.59 02:34:25.60 +56:19:16.4
136.90127 -3.73153 galactic Per Second-epoch detections are separated by 2.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.6075+56.3202 | 02:34:25.60 +56:19:16.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:25.60 +56:19:16.4: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:25.60 +56:19:16.4: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 25.60 +56 19 16.4 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.6075+56.3202,2461228.7512,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.6075+56.3202 20260707.2512 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 11.09 01:06:55.51 +59:18:57.7
124.91028 -3.49622 galactic Cas Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:06:55.51 +59:18:57.7 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:55.51 +59:18:57.7: 13.17 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:55.51 +59:18:57.7: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 06 55.51 +59 18 57.7 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.54 02:33:21.63 +56:36:57.4
136.65130 -3.51635 galactic Per Second-epoch detections are separated by 2.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3416+56.6152 | 02:33:21.63 +56:36:57.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:21.63 +56:36:57.4: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:21.63 +56:36:57.4: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 21.63 +56 36 57.4 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.3416+56.6152,2461228.7512,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.3416+56.6152 20260707.2512 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.60 02:33:15.69 +56:38:32.9
136.62851 -3.49707 galactic Per Second-epoch detections are separated by 3.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.3158+56.6419 | 02:33:15.69 +56:38:32.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.433+/-0.052 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:15.69 +56:38:32.9: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:15.69 +56:38:32.9: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 15.69 +56 38 32.9 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.3158+56.6419,2461228.7512,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.3158+56.6419 20260707.2512 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 11.22 01:23:08.00 +63:07:27.6
126.50497 0.47268 galactic Cas Second-epoch detections are separated by 2.8" and 5.6 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 | 01:23:08.00 +63:07:27.6 (user input) | T | P | (position from user input) J-Ks=0.538+/-0.029 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:08.00 +63:07:27.6: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:08.00 +63:07:27.6: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 23 08.00 +63 07 27.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 11.22CV 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 07 07.2512 2461228.7512 10.55 02:26:25.60 +56:08:18.7
135.93587 -4.31617 galactic Per Second-epoch detections are separated by 4.3" and 5.5 pix
The object was found in VSX 3" Gaia DR3 457465492216219008
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.870 G 12.900 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:25.60 +56:08:18.7: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:25.60 +56:08:18.7: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 26 25.60 +56 08 18.7 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457465492216219008,2461228.7512,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457465492216219008 20260707.2512 10.55CV 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 07 07.2512 2461228.7512 10.24 02:27:39.96 +56:48:08.2
135.85532 -3.63544 galactic Per Second-epoch detections are separated by 0.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:27:39.96 +56:48:08.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:39.96 +56:48:08.2: 11.53 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:39.96 +56:48:08.2: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 27 39.96 +56 48 08.2 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.72 01:58:35.42 +58:39:55.9
131.58313 -3.07372 galactic Cas Second-epoch detections are separated by 1.4" and 5.5 pix
The object was found in VSX 1" ASASSN-V J015835.37+583955.1
Type: L:
# Max. Min./Amp. JD0 Period
15.300 V 16.000 V
ATTENTION: measured mag 10.72 is 4.6 mag brighter than the VSX record maximum brightness 15.30 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:35.42 +58:39:55.9: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:35.42 +58:39:55.9: 14.83 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 58 35.42 +58 39 55.9 10.7 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
ASASSN-V J015835.37+583955.1,2461228.7512,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015835.37+583955.1 20260707.2512 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.25 02:33:58.86 +57:33:07.0
136.36879 -2.61990 galactic Per Second-epoch detections are separated by 1.2" 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 | Gaia DR3 458023730583462144 | 02:33:58.96 +57:33:04.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:58.86 +57:33:07.0: 12.08 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:58.86 +57:33:07.0: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 58.86 +57 33 07.0 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 458023730583462144,2461228.7512,10.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 458023730583462144 20260707.2512 10.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.78 02:19:03.95 +62:47:34.1
132.75766 1.60477 galactic Cas Second-epoch detections are separated by 1.2" and 5.5 pix
The object was found in VSX 1" ASASSN-V J021904.01+624734.4
Type: SR
# Max. Min./Amp. JD0 Period
13.890 V 14.180 V 2457429.00000 487.000000000000
ATTENTION: measured mag 9.78 is 4.1 mag brighter than the VSX record maximum brightness 13.89 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:03.95 +62:47:34.1: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:03.95 +62:47:34.1: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 07 07.2512* 02 19 03.95 +62 47 34.1 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J021904.01+624734.4,2461228.7512,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021904.01+624734.4 20260707.2512 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.36 02:14:38.60 +57:52:11.6
133.83648 -3.22946 galactic Per Second-epoch detections are separated by 0.4" and 5.8 pix
The object was found in VSX 2" ZTF J021438.50+575209.6
Type: SR
# Max. Min./Amp. JD0 Period
15.358 g Y 0.302 g 2458291.28930 110.696719600000
ATTENTION: measured mag 10.36 is 4.7 mag brighter than the VSX record maximum brightness 15.06 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:38.60 +57:52:11.6: 13.15 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:38.60 +57:52:11.6: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 14 38.60 +57 52 11.6 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J021438.50+575209.6,2461228.7512,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021438.50+575209.6 20260707.2512 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.10 01:14:11.39 +61:16:04.2
125.66368 -1.48318 galactic Cas Second-epoch detections are separated by 3.7" and 5.1 pix
The object was found in VSX 2" ASASSN-V J011411.20+611605.2
Type: SR
# Max. Min./Amp. JD0 Period
13.253 r Y 0.436 r 2458475.78320 80.440504000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:11.39 +61:16:04.2: 12.95 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:11.39 +61:16:04.2: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 14 11.39 +61 16 04.2 10.1 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
ASASSN-V J011411.20+611605.2,2461228.7512,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011411.20+611605.2 20260707.2512 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.00 02:33:59.56 +55:56:25.8
136.99297 -4.10601 galactic Per Second-epoch detections are separated by 1.7" and 6.0 pix
The object was found in VSX 3" Gaia DR3 457313205553053184
Type: ROT
# Max. Min./Amp. JD0 Period
12.440 G 12.480 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:59.56 +55:56:25.8: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:59.56 +55:56:25.8: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 33 59.56 +55 56 25.8 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457313205553053184,2461228.7512,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457313205553053184 20260707.2512 10.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.02 02:29:11.49 +56:22:46.6
136.20631 -3.95181 galactic Per Second-epoch detections are separated by 2.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.2825+56.3782 | 02:29:11.71 +56:22:43.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:11.49 +56:22:46.6: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:11.49 +56:22:46.6: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 29 11.49 +56 22 46.6 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.2825+56.3782,2461228.7512,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.2825+56.3782 20260707.2512 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.79 02:38:01.93 +58:50:39.9
136.35260 -1.22170 galactic Cas Second-epoch detections are separated by 1.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.5186+58.8445 | 02:38:02.39 +58:50:41.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:01.93 +58:50:39.9: 10.04 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:01.93 +58:50:39.9: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 38 01.93 +58 50 39.9 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.5186+58.8445,2461228.7512,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.5186+58.8445 20260707.2512 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.82 02:10:17.96 +60:59:00.3
132.35013 -0.43806 galactic Cas Second-epoch detections are separated by 1.5" and 5.9 pix
The object was found in VSX 3" NSVS J0210179+605902
Type: SR
# Max. Min./Amp. JD0 Period
14.153 r Y 0.631 r 2458450.25450 296.241215300000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:17.96 +60:59:00.3: 13.54 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:17.96 +60:59:00.3: 14.75 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 10 17.96 +60 59 00.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0210179+605902,2461228.7512,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0210179+605902 20260707.2512 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.14 02:14:27.88 +64:44:14.1
131.64552 3.27946 galactic Cas Second-epoch detections are separated by 2.4" and 5.1 pix
The object was found in VSX 1" NSVS J0214284+644418
Type: SR
# Max. Min./Amp. JD0 Period
12.916 r Y 0.345 r 2458352.87040 121.127267000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:27.88 +64:44:14.1: 11.33 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:27.88 +64:44:14.1: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 07 07.2512* 02 14 27.88 +64 44 14.1 10.1 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
NSVS J0214284+644418,2461228.7512,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0214284+644418 20260707.2512 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.28 02:05:05.79 +58:16:24.3
132.50931 -3.22203 galactic Per Second-epoch detections are separated by 0.7" and 5.7 pix
The object was found in VSX 1" V0661 Per
Type: SR:
# Max. Min./Amp. JD0 Period
13.500 V 14.200 V
ATTENTION: measured mag 9.28 is 4.2 mag brighter than the VSX record maximum brightness 13.50 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:05:05.79 +58:16:24.3: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:05:05.79 +58:16:24.3: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 05 05.79 +58 16 24.3 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0661 Per,2461228.7512,9.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0661 Per 20260707.2512 9.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.12 01:21:54.90 +61:20:55.9
126.57782 -1.30696 galactic Cas Second-epoch detections are separated by 1.4" and 5.5 pix
The object was found in ASASSN-V 2" ASASSN-V J012154.67+612055.1
Type: SR
MeanMag 14.81 m Amp. 2.24 m Period 397.1456143 d
ATTENTION: measured mag 9.12 is 3.5 mag brighter than the ASASSN-V record maximum brightness 12.57 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:54.90 +61:20:55.9: 13.30 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:54.90 +61:20:55.9: 14.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 21 54.90 +61 20 55.9 9.1 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
VARIABLE_NAME,2461228.7512,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260707.2512 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.05 02:27:56.18 +56:10:22.0
136.11991 -4.20814 galactic Per Second-epoch detections are separated by 3.2" and 5.7 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 | 02:27:56.18 +56:10:22.0 (user input) | T | P | (position from user input) J-Ks=0.734+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:56.18 +56:10:22.0: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:56.18 +56:10:22.0: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 27 56.18 +56 10 22.0 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.71 02:28:12.03 +64:31:53.4
133.10107 3.58739 galactic Cas Second-epoch detections are separated by 0.2" and 5.7 pix
The object was found in VSX 0" NSVS J0228122+643156
Type: SR
# Max. Min./Amp. JD0 Period
13.081 r Y 0.937 r 2458466.24640 234.996798300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:12.03 +64:31:53.4: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:12.03 +64:31:53.4: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 28 12.03 +64 31 53.4 9.7 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
NSVS J0228122+643156,2461228.7512,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0228122+643156 20260707.2512 9.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.20 02:31:45.74 +56:26:46.2
136.51194 -3.75725 galactic Per Second-epoch detections are separated by 0.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457393336767227264 | 02:31:45.96 +56:26:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.346+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:45.74 +56:26:46.2: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:45.74 +56:26:46.2: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.81 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 45.74 +56 26 46.2 8.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457393336767227264,2461228.7512,8.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457393336767227264 20260707.2512 8.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.31 02:37:21.05 +57:19:39.0
136.87440 -2.64900 galactic Per Second-epoch detections are separated by 3.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.3273+57.3275 | 02:37:21.05 +57:19:39.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.845+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:21.05 +57:19:39.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:21.05 +57:19:39.0: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 37 21.05 +57 19 39.0 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J039.3273+57.3275,2461228.7512,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.3273+57.3275 20260707.2512 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.32 01:46:47.71 +60:09:41.2
129.77129 -1.97315 galactic Cas Second-epoch detections are separated by 2.4" and 5.1 pix
The object was found in ASASSN-V 2" ASASSN-V J014647.54+600940.1
Type: SR
MeanMag 14.6 m Amp. 0.53 m Period 88.0 d
ATTENTION: measured mag 10.32 is 3.8 mag brighter than the ASASSN-V record maximum brightness 14.07 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:47.71 +60:09:41.2: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:47.71 +60:09:41.2: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 46 47.71 +60 09 41.2 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461228.7512,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260707.2512 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.81 02:19:16.58 +59:42:22.1
133.80787 -1.29789 galactic Cas Second-epoch detections are separated by 0.7" and 5.7 pix
The object was found in VSX 1" ZTF J021916.76+594221.6
Type: SR
# Max. Min./Amp. JD0 Period
14.063 g Y 0.424 g 2458349.86040 72.477681200000 MS
ATTENTION: measured mag 8.81 is 4.8 mag brighter than the VSX record maximum brightness 13.64 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:16.58 +59:42:22.1: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:16.58 +59:42:22.1: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 19 16.58 +59 42 22.1 8.8 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
ZTF J021916.76+594221.6,2461228.7512,8.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021916.76+594221.6 20260707.2512 8.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.23 02:24:41.36 +58:22:34.6
134.91813 -2.30858 galactic Per Second-epoch detections are separated by 0.2" and 5.9 pix
The object was found in VSX 2" ASASSN-V J022441.46+582233.3
Type: SR
# Max. Min./Amp. JD0 Period
14.827 g Y 0.387 g 2458366.56600 67.480010700000
ATTENTION: measured mag 9.23 is 5.2 mag brighter than the VSX record maximum brightness 14.44 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:41.36 +58:22:34.6: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:41.36 +58:22:34.6: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 24 41.36 +58 22 34.6 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J022441.46+582233.3,2461228.7512,9.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J022441.46+582233.3 20260707.2512 9.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.94 01:25:43.56 +60:50:05.6
127.09937 -1.75911 galactic Cas Second-epoch detections are separated by 0.3" and 5.3 pix
The object was found in VSX 2" ZTF J012543.34+605006.2
Type: SR
# Max. Min./Amp. JD0 Period
14.923 g Y 0.462 g 2458271.66140 289.704203100000
ATTENTION: measured mag 9.94 is 4.5 mag brighter than the VSX record maximum brightness 14.46 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:43.56 +60:50:05.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:43.56 +60:50:05.6: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 07 07.2512* 01 25 43.56 +60 50 05.6 9.9 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 J012543.34+605006.2,2461228.7512,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012543.34+605006.2 20260707.2512 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.84 02:11:29.16 +59:35:35.7
132.91086 -1.71863 galactic Cas Second-epoch detections are separated by 0.6" and 5.7 pix
The object was found in VSX 3" ZTF J021128.91+593533.9
Type: SR
# Max. Min./Amp. JD0 Period
14.643 r Y 0.766 r 2458306.02430 268.274401400000
ATTENTION: measured mag 10.84 is 3.0 mag brighter than the VSX record maximum brightness 13.88 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:29.16 +59:35:35.7: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:29.16 +59:35:35.7: 14.92 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 11 29.16 +59 35 35.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J021128.91+593533.9,2461228.7512,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021128.91+593533.9 20260707.2512 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.42 02:19:47.96 +56:25:10.1
134.97304 -4.37246 galactic Per Second-epoch detections are separated by 2.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458272499382317568 | 02:19:48.03 +56:25:07.5 (Gaia DR3) | S (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.171+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:47.96 +56:25:10.1: 12.33 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:47.96 +56:25:10.1: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 19 47.96 +56 25 10.1 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 458272499382317568,2461228.7512,9.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 458272499382317568 20260707.2512 9.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.38 02:24:52.10 +58:00:24.5
135.07072 -2.64597 galactic Per Second-epoch detections are separated by 1.3" and 6.1 pix
The object was found in VSX 1" V0760 Per
Type: LB
# Max. Min./Amp. JD0 Period
12.100 R1 12.700 R1 2451437.21000 231.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:52.10 +58:00:24.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:52.10 +58:00:24.5: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 24 52.10 +58 00 24.5 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0760 Per,2461228.7512,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0760 Per 20260707.2512 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.23 02:34:12.75 +56:03:48.5
136.97375 -3.98071 galactic Per Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.5561+56.0631 | 02:34:13.47 +56:03:47.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:12.75 +56:03:48.5: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:12.75 +56:03:48.5: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 12.75 +56 03 48.5 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J038.5561+56.0631,2461228.7512,9.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J038.5561+56.0631 20260707.2512 9.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.23 02:32:02.00 +57:03:30.7
136.31422 -3.17637 galactic Per Second-epoch detections are separated by 0.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9985+57.0505 | 02:32:02.00 +57:03:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.309+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:02.00 +57:03:30.7: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:02.00 +57:03:30.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 32 02.00 +57 03 30.7 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.9985+57.0505,2461228.7512,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.9985+57.0505 20260707.2512 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.12 02:22:56.66 +57:11:45.2
135.11311 -3.49579 galactic Per Second-epoch detections are separated by 0.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J035.7523+57.1948 | 02:22:56.77 +57:11:44.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.065+/-0.038 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:56.66 +57:11:45.2: 9.54 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:56.66 +57:11:45.2: 10.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 22 56.66 +57 11 45.2 8.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J035.7523+57.1948,2461228.7512,8.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J035.7523+57.1948 20260707.2512 8.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.82 02:14:40.15 +62:26:25.5
132.39356 1.10753 galactic Cas Second-epoch detections are separated by 2.0" and 5.5 pix
The object was found in VSX 1" NSVS 1831601
Type: SR
# Max. Min./Amp. JD0 Period
13.824 r Y 0.886 r 2451335.36000 379.834003600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:14:40.15 +62:26:25.5: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:14:40.15 +62:26:25.5: 14.40 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 14 40.15 +62 26 25.5 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1831601,2461228.7512,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1831601 20260707.2512 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.16 01:26:54.02 +58:45:08.8
127.52753 -3.80252 galactic Cas Second-epoch detections are separated by 0.2" and 5.6 pix
The object was found in VSX 1" ZTF J012653.83+584508.8
Type: SR
# Max. Min./Amp. JD0 Period
15.801 g Y 0.268 g 2458378.87400 104.320008700000
ATTENTION: measured mag 10.16 is 5.4 mag brighter than the VSX record maximum brightness 15.53 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:54.02 +58:45:08.8: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:54.02 +58:45:08.8: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 26 54.02 +58 45 08.8 10.2 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 J012653.83+584508.8,2461228.7512,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012653.83+584508.8 20260707.2512 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.67 02:23:49.46 +56:41:26.7
135.40214 -3.92751 galactic Per Second-epoch detections are separated by 0.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458382381836763136 | 02:23:49.38 +56:41:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:23:49.46 +56:41:26.7: 11.56 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:23:49.46 +56:41:26.7: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 23 49.46 +56 41 26.7 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 458382381836763136,2461228.7512,9.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 458382381836763136 20260707.2512 9.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.63 01:28:07.88 +58:27:03.1
127.72895 -4.07871 galactic Cas Second-epoch detections are separated by 0.6" and 5.5 pix
The object was found in VSX 0" ASASSN-V J012807.84+582702.8
Type: SR
# Max. Min./Amp. JD0 Period
14.320 V 14.780 V 2458335.90770 122.552347700000
ATTENTION: measured mag 10.63 is 3.7 mag brighter than the VSX record maximum brightness 14.32 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:07.88 +58:27:03.1: 11.96 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:07.88 +58:27:03.1: 14.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 28 07.88 +58 27 03.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J012807.84+582702.8,2461228.7512,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012807.84+582702.8 20260707.2512 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.43 01:24:30.55 +59:38:48.3
127.10464 -2.95679 galactic Cas Second-epoch detections are separated by 0.9" and 5.5 pix
The object was found in VSX 0" ASASSN-V J012430.51+593847.9
Type: SR
# Max. Min./Amp. JD0 Period
13.360 V 13.950 V 2458378.66340 139.847766200000
ATTENTION: measured mag 9.43 is 3.9 mag brighter than the VSX record maximum brightness 13.36 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:30.55 +59:38:48.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:30.55 +59:38:48.3: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 24 30.55 +59 38 48.3 9.4 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
ASASSN-V J012430.51+593847.9,2461228.7512,9.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012430.51+593847.9 20260707.2512 9.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.09 02:38:48.26 +57:57:35.1
136.79992 -1.99172 galactic Cas Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J039.7144+57.9584 | 02:38:48.32 +57:57:33.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.120+/-0.028 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:38:48.26 +57:57:35.1: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:38:48.26 +57:57:35.1: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 38 48.26 +57 57 35.1 9.1 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 J039.7144+57.9584,2461228.7512,9.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J039.7144+57.9584 20260707.2512 9.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.21 01:14:56.64 +59:42:13.1
125.89674 -3.03273 galactic Cas Second-epoch detections are separated by 0.4" and 5.3 pix
The object was found in VSX 0" NSVS J0114566+594210
Type: SR
# Max. Min./Amp. JD0 Period
13.340 r Y 0.273 r 2458345.86300 105.806803300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:56.64 +59:42:13.1: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:56.64 +59:42:13.1: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 14 56.64 +59 42 13.1 10.2 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
NSVS J0114566+594210,2461228.7512,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0114566+594210 20260707.2512 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.68 02:19:34.20 +58:23:58.5
134.27951 -2.51704 galactic Per Second-epoch detections are separated by 0.5" and 5.9 pix
The object was found in VSX 2" NSVS 1909158
Type: SR
# Max. Min./Amp. JD0 Period
14.589 g Y 0.328 g 2458495.63840 62.731476600000
ATTENTION: measured mag 8.68 is 5.6 mag brighter than the VSX record maximum brightness 14.26 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:34.20 +58:23:58.5: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:34.20 +58:23:58.5: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 19 34.20 +58 23 58.5 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1909158,2461228.7512,8.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1909158 20260707.2512 8.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.78 02:27:22.01 +62:38:26.7
133.70294 1.79236 galactic Cas Second-epoch detections are separated by 2.1" and 5.8 pix
The object was found in VSX 1" V0937 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
13.700 V 14.500 V
ATTENTION: measured mag 9.78 is 3.9 mag brighter than the VSX record maximum brightness 13.70 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:22.01 +62:38:26.7: 10.97 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:22.01 +62:38:26.7: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 27 22.01 +62 38 26.7 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0937 Cas,2461228.7512,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0937 Cas 20260707.2512 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.12 02:30:17.09 +56:38:10.3
136.25130 -3.65758 galactic Per Second-epoch detections are separated by 1.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457587263129458432 | 02:30:17.01 +56:38:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:17.09 +56:38:10.3: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:17.09 +56:38:10.3: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 30 17.09 +56 38 10.3 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457587263129458432,2461228.7512,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457587263129458432 20260707.2512 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.11 02:34:05.62 +56:37:26.6
136.74142 -3.47005 galactic Per Second-epoch detections are separated by 0.8" and 6.1 pix
The object was found in VSX23" Gaia DR3 457763322428148096
Type: ROT
# Max. Min./Amp. JD0 Period
15.220 G 15.260 G K
ATTENTION: measured mag 7.11 is 8.1 mag brighter than the VSX record maximum brightness 15.22 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:05.62 +56:37:26.6: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:05.62 +56:37:26.6: 9.65 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.65 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 34 05.62 +56 37 26.6 7.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457763322428148096,2461228.7512,7.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457763322428148096 20260707.2512 7.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.56 02:10:41.36 +57:16:54.8
133.51382 -3.95260 galactic Per Second-epoch detections are separated by 4.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J032.6766+57.2835 | 02:10:41.36 +57:16:54.8 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:41.36 +57:16:54.8: 13.12 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:41.36 +57:16:54.8: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 10 41.36 +57 16 54.8 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J032.6766+57.2835,2461228.7512,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J032.6766+57.2835 20260707.2512 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 11.04 02:10:01.04 +64:59:04.3
131.11913 3.36932 galactic Cas Second-epoch detections are separated by 1.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:10:01.04 +64:59:04.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:01.04 +64:59:04.3: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:01.04 +64:59:04.3: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 10 01.04 +64 59 04.3 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.42 02:27:52.25 +56:32:26.5
135.97699 -3.86885 galactic Per Second-epoch detections are separated by 0.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:27:52.25 +56:32:26.5 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:52.25 +56:32:26.5: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:52.25 +56:32:26.5: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 27 52.25 +56 32 26.5 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461228.7512,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.48 02:31:32.24 +56:47:59.3
136.34942 -3.44148 galactic Per Second-epoch detections are separated by 1.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457964803634866560 | 02:31:32.30 +56:47:58.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.863+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:32.24 +56:47:59.3: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:32.24 +56:47:59.3: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 32.24 +56 47 59.3 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457964803634866560,2461228.7512,9.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457964803634866560 20260707.2512 9.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.88 02:02:52.76 +63:13:25.1
130.87649 1.45917 galactic Cas Second-epoch detections are separated by 1.4" and 5.3 pix
The object was found in VSX 7" Gaia DR3 514890132679097856
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.100 G 14.130 G A
ATTENTION: measured mag 10.88 is 3.2 mag brighter than the VSX record maximum brightness 14.10 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:52.76 +63:13:25.1: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:52.76 +63:13:25.1: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 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 07 07.2512* 02 02 52.76 +63 13 25.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 514890132679097856,2461228.7512,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 514890132679097856 20260707.2512 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.38 02:09:55.29 +56:59:22.9
133.50242 -4.26260 galactic Per Second-epoch detections are separated by 2.2" and 6.1 pix
The object was found in VSX 2" ASASSN-V J020955.15+565920.6
Type: SR
# Max. Min./Amp. JD0 Period
14.620 V 15.150 V 2458358.04680 150.234053800000
ATTENTION: measured mag 10.38 is 4.2 mag brighter than the VSX record maximum brightness 14.62 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:09:55.29 +56:59:22.9: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:09:55.29 +56:59:22.9: 14.27 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 09 55.29 +56 59 22.9 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J020955.15+565920.6,2461228.7512,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020955.15+565920.6 20260707.2512 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.79 01:50:36.62 +63:53:30.0
129.38652 1.76395 galactic Cas Second-epoch detections are separated by 3.8" and 5.4 pix
The object was found in VSX 5" ASASSN-V J015036.60+635335.1
Type: SR
# Max. Min./Amp. JD0 Period
14.850 V 15.220 V 2458062.97400 59.670000000000
ATTENTION: measured mag 10.79 is 4.1 mag brighter than the VSX record maximum brightness 14.85 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:36.62 +63:53:30.0: 11.42 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:36.62 +63:53:30.0: 14.42 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 50 36.62 +63 53 30.0 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J015036.60+635335.1,2461228.7512,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J015036.60+635335.1 20260707.2512 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.85 02:12:37.92 +61:35:07.5
132.43370 0.22067 galactic Cas Second-epoch detections are separated by 1.4" and 5.4 pix
The object was found in VSX 1" ZTF J021237.80+613507.4
Type: SR
# Max. Min./Amp. JD0 Period
17.093 g Y 0.595 g 2458334.80460 120.561840400000
ATTENTION: measured mag 10.85 is 5.6 mag brighter than the VSX record maximum brightness 16.50 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:12:37.92 +61:35:07.5: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:12:37.92 +61:35:07.5: 14.75 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 12 37.92 +61 35 07.5 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J021237.80+613507.4,2461228.7512,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J021237.80+613507.4 20260707.2512 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.51 01:33:44.66 +60:46:19.2
128.07615 -1.67649 galactic Cas Second-epoch detections are separated by 0.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:33:44.66 +60:46:19.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:44.66 +60:46:19.2: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.66 +60:46:19.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 33 44.66 +60 46 19.2 10.5 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,2461228.7512,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260707.2512 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 7.38 02:37:50.78 +57:54:16.5
136.70543 -2.09319 galactic Cas Second-epoch detections are separated by 0.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457950376842758784 | 02:37:50.90 +57:54:16.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +57 74 J-Ks=0.095+/-0.032 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:50.78 +57:54:16.5: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:50.78 +57:54:16.5: 9.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.97 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 37 50.78 +57 54 16.5 7.4 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 457950376842758784,2461228.7512,7.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457950376842758784 20260707.2512 7.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.84 02:08:59.25 +60:15:03.0
132.41474 -1.18531 galactic Cas Second-epoch detections are separated by 2.2" and 5.4 pix
The object was found in VSX 2" NSVS 1829332
Type: L
# Max. Min./Amp. JD0 Period
12.300 R1 12.750 R1
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:08:59.25 +60:15:03.0: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:08:59.25 +60:15:03.0: 14.70 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 08 59.25 +60 15 03.0 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1829332,2461228.7512,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1829332 20260707.2512 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.35 01:28:36.11 +61:12:07.3
127.39374 -1.34735 galactic Cas Second-epoch detections are separated by 0.4" and 5.3 pix
The object was found in VSX 1" PQ Cas
Type: SR
# Max. Min./Amp. JD0 Period
14.963 g Y 0.540 g 2458436.69130 77.771904400000 S
ATTENTION: measured mag 9.35 is 5.1 mag brighter than the VSX record maximum brightness 14.42 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:36.11 +61:12:07.3: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:36.11 +61:12:07.3: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 28 36.11 +61 12 07.3 9.3 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
PQ Cas,2461228.7512,9.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PQ Cas 20260707.2512 9.35CV 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 07 07.2512 2461228.7512 8.84 01:20:18.26 +64:28:06.1
126.03713 1.77079 galactic Cas Second-epoch detections are separated by 0.3" and 5.1 pix
The object was found in VSX 1" V0898 Cas
Type: SR:
# Max. Min./Amp. JD0 Period
12.800 V 13.800 V
ATTENTION: measured mag 8.84 is 4.0 mag brighter than the VSX record maximum brightness 12.80 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:18.26 +64:28:06.1: 10.35 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:18.26 +64:28:06.1: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 20 18.26 +64 28 06.1 8.8 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
V0898 Cas,2461228.7512,8.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0898 Cas 20260707.2512 8.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 11.03 01:13:00.09 +62:10:43.8
125.44515 -0.58764 galactic Cas Second-epoch detections are separated by 2.8" and 4.7 pix
The object was found in VSX 4" V0418 Cas
Type: M
# Max. Min./Amp. JD0 Period
10.700 V 19.400 V 2453665.00000 478.000000000000 S7/2e
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:00.09 +62:10:43.8: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:00.09 +62:10:43.8: 14.99 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 13 00.09 +62 10 43.8 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0418 Cas,2461228.7512,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0418 Cas 20260707.2512 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.21 02:03:07.44 +57:18:15.2
132.52639 -4.22608 galactic Per Second-epoch detections are separated by 0.7" and 5.7 pix
The object was found in VSX 2" ASASSN-V J020307.46+571813.2
Type: SR
# Max. Min./Amp. JD0 Period
13.470 V 13.900 V 2458312.63550 148.824620900000
ATTENTION: measured mag 9.21 is 4.3 mag brighter than the VSX record maximum brightness 13.47 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:07.44 +57:18:15.2: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:07.44 +57:18:15.2: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 03 07.44 +57 18 15.2 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J020307.46+571813.2,2461228.7512,9.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020307.46+571813.2 20260707.2512 9.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.82 02:31:18.68 +56:20:49.0
136.49154 -3.87268 galactic Per Second-epoch detections are separated by 1.3" 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 | Gaia DR3 457386739697519488 | 02:31:19.13 +56:20:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:18.68 +56:20:49.0: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:18.68 +56:20:49.0: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 18.68 +56 20 49.0 8.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457386739697519488,2461228.7512,8.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457386739697519488 20260707.2512 8.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.71 01:58:48.66 +62:43:31.8
130.56311 0.85623 galactic Cas Second-epoch detections are separated by 1.9" and 5.7 pix
The object was found in VSX 6" NSVS 1820604
Type: SR
# Max. Min./Amp. JD0 Period
13.494 r Y 0.450 R1 2458369.29680 125.813204600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:48.66 +62:43:31.8: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:48.66 +62:43:31.8: 14.28 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 58 48.66 +62 43 31.8 10.7 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
NSVS 1820604,2461228.7512,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1820604 20260707.2512 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.10 01:52:19.59 +57:19:07.0
131.10881 -4.58330 galactic Per Second-epoch detections are separated by 0.5" and 5.6 pix
The object was found in VSX 1" BX Per
Type: LB
# Max. Min./Amp. JD0 Period
14.400 pg 15.000 pg M6
ATTENTION: measured mag 9.10 is 5.3 mag brighter than the VSX record maximum brightness 14.40 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:19.59 +57:19:07.0: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:19.59 +57:19:07.0: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 52 19.59 +57 19 07.0 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BX Per,2461228.7512,9.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BX Per 20260707.2512 9.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.81 01:25:24.78 +62:14:21.4
126.87687 -0.37195 galactic Cas Second-epoch detections are separated by 2.1" and 5.5 pix
The object was found in VSX 1" ASASSN-V J012524.70+621420.4
Type: L:
# Max. Min./Amp. JD0 Period
14.870 V 15.410 V
ATTENTION: measured mag 10.81 is 4.1 mag brighter than the VSX record maximum brightness 14.87 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:24.78 +62:14:21.4: 12.13 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:24.78 +62:14:21.4: 14.48 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 25 24.78 +62 14 21.4 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J012524.70+621420.4,2461228.7512,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J012524.70+621420.4 20260707.2512 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.84 02:03:35.37 +57:58:41.0
132.40043 -3.56115 galactic Per Second-epoch detections are separated by 2.1" and 6.0 pix
The object was found in VSX 1" ASASSN-V J020335.32+575840.4
Type: SR
# Max. Min./Amp. JD0 Period
16.180 g Y 1.090 g 2459278.62900 829.000000000000
ATTENTION: measured mag 10.84 is 4.2 mag brighter than the VSX record maximum brightness 15.09 - 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:35.37 +57:58:41.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:35.37 +57:58:41.0: 14.80 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.80 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 03 35.37 +57 58 41.0 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J020335.32+575840.4,2461228.7512,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J020335.32+575840.4 20260707.2512 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.64 02:31:58.69 +55:59:28.0
136.71245 -4.16708 galactic Per Second-epoch detections are separated by 3.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J037.9924+55.9989 | 02:31:59.30 +55:59:27.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:58.69 +55:59:28.0: 12.95 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:58.69 +55:59:28.0: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 58.69 +55 59 28.0 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J037.9924+55.9989,2461228.7512,9.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J037.9924+55.9989 20260707.2512 9.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.96 02:13:47.66 +63:11:26.5
132.06252 1.78825 galactic Cas Second-epoch detections are separated by 1.8" and 5.8 pix
The object was found in VSX 1" NSVS J0213478+631127
Type: L:
# Max. Min./Amp. JD0 Period
11.122 R1 Y 0.644 R1 355.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:13:47.66 +63:11:26.5: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:13:47.66 +63:11:26.5: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 13 47.66 +63 11 26.5 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0213478+631127,2461228.7512,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0213478+631127 20260707.2512 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 10.27 01:36:47.19 +63:02:42.2
128.04455 0.62434 galactic Cas Second-epoch detections are separated by 2.1" and 5.4 pix
The object was found in VSX 0" NSVS 1806131
Type: L
# Max. Min./Amp. JD0 Period
11.350 R1 11.800 R1
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:47.19 +63:02:42.2: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:47.19 +63:02:42.2: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 36 47.19 +63 02 42.2 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1806131,2461228.7512,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1806131 20260707.2512 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.77 02:31:31.11 +57:22:45.6
136.12822 -2.90568 galactic Per Second-epoch detections are separated by 1.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 458018340407727104 | 02:31:29.87 +57:22:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M3.5 1985ApJS...59..197B LTT 10837
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:31.11 +57:22:45.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:31.11 +57:22:45.6: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 31 31.11 +57 22 45.6 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 458018340407727104,2461228.7512,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 458018340407727104 20260707.2512 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 8.91 02:28:34.97 +56:03:02.6
136.24880 -4.28876 galactic Per Second-epoch detections are separated by 5.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 457539743610843648 | 02:28:35.31 +56:03:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:34.97 +56:03:02.6: 12.82 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:34.97 +56:03:02.6: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 28 34.97 +56 03 02.6 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 457539743610843648,2461228.7512,8.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 457539743610843648 20260707.2512 8.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.81 02:40:38.76 +60:07:56.2
136.13616 0.09047 galactic Cas Second-epoch detections are separated by 0.8" and 5.9 pix
The object was found in VSX 6" NSVS J0240393+600752
Type: L:
# Max. Min./Amp. JD0 Period
11.294 R1 Y 0.308 R1 730.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:40:38.76 +60:07:56.2: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:40:38.76 +60:07:56.2: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 07 07.2512* 02 40 38.76 +60 07 56.2 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0240393+600752,2461228.7512,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0240393+600752 20260707.2512 9.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.33 02:18:22.67 +58:47:10.8
134.00437 -2.20379 galactic Per Second-epoch detections are separated by 1.4" and 6.0 pix
The object was found in VSX 2" NSVS J0218236+584716
Type: SR
# Max. Min./Amp. JD0 Period
12.694 r Y 0.560 r 2458351.79460 241.646383300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:22.67 +58:47:10.8: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:22.67 +58:47:10.8: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 02 18 22.67 +58 47 10.8 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0218236+584716,2461228.7512,9.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0218236+584716 20260707.2512 9.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 07.2512 2461228.7512 9.47 01:35:09.81 +60:17:10.2
128.32914 -2.12657 galactic Cas Second-epoch detections are separated by 1.2" and 5.2 pix
The object was found in VSX 1" Mis V0883
Type: L:
# Max. Min./Amp. JD0 Period
10.600 CR 11.500 CR 188.000000000000 S
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:09.81 +60:17:10.2: 13.10 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:09.81 +60:17:10.2: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 07.2512* 01 35 09.81 +60 17 10.2 9.5 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
Mis V0883,2461228.7512,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V0883 20260707.2512 9.47CV 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
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
SExtractor catalog cache: saved Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461228.75095034
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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits'
wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:42.375 +62:03:20.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:42.375 +62:03:20.28
Angular distance between the image centers 0.0754 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
Image size: 942.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:39.661 +62:02:54.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:39.661 +62:02:54.43
Angular distance between the image centers 0.0668 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 01:42:42.375 +62:03:20.28
Second-epoch second image center 01:42:39.661 +62:02:54.43
Angular distance between the image centers 0.00893 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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.FkOWSBGyMj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.e6HteFLypM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits &> /tmp/tmp.X6QBZaDN1I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits &> /tmp/tmp.AnlyHqGbvj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
Found non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
The reference image (wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat) found
'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat' -> 'wcsmag.cat'
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 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 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 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): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
ERROR: only 24 of 31559 stars detected on the reference image matched the Tycho-2 photometric calibration catalog (0.08%) - the reference image plate solution is likely broken and the magnitude calibration is unreliable
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.937800
a=0.000000 b=1.000000 c=22.937800
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 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 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 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): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.9)
Read 31681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.0659 to 45.7628 deg, Dec +55.3336 to +67.4023 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 7.0659 to 45.7628 deg, Dec 55.3336 to 67.4023 deg
Loaded 26179 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): 14497 out of 16269 total matches.
Matched with Tycho-2 16269 out of 31681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 62 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
3.3 pix fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
3.3 pix fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
2.2 pix wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
14.2 mag. fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
14.2 mag. fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.6 (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.FkOWSBGyMj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.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-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=3786, bad_region=1, passed=31559
Got 31559 stars (including 27743 good ones) from the SExtractor catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat
util/solve_plate_with_UCAC5 got 31559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 280 matched stars entering correct_measured_positions(), 228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 267 matched stars entering correct_measured_positions(), 10048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 336 matched stars entering correct_measured_positions(), 10093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.75"
Excluding outliers - 331 stars left (next iteration limit 293)
WCS_QUALITY_DIAG: file=Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=331 sigma_overall_arcsec=7.291 sigma_q1_arcsec=27.811 sigma_q2_arcsec=12.006 sigma_q3_arcsec=24.661 sigma_q4_arcsec=4.199 n_q1=15 n_q2=98 n_q3=37 n_q4=181 worst_quadrant_to_overall_ratio=3.814
The image catalog is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.e6HteFLypM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.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-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=3692, bad_region=0, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat
util/solve_plate_with_UCAC5 got 31681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=973 sigma_overall_arcsec=0.406 sigma_q1_arcsec=0.531 sigma_q2_arcsec=0.401 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.344 n_q1=119 n_q2=244 n_q3=303 n_q4=307 worst_quadrant_to_overall_ratio=1.308
The image catalog is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.X6QBZaDN1I (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=997, bad_region=0, passed=17056
Got 17056 stars (including 16048 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits.wcscat
util/solve_plate_with_UCAC5 got 17056 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 16630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.7 to 67.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 16630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 16630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits N_match=966 sigma_overall_arcsec=0.370 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.422 sigma_q3_arcsec=0.289 sigma_q4_arcsec=0.406 n_q1=270 n_q2=312 n_q3=222 n_q4=162 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits -region wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AnlyHqGbvj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits.wcscat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=1000, bad_region=0, passed=17018
Got 17018 stars (including 16012 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits.wcscat
util/solve_plate_with_UCAC5 got 17018 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.6'
Seting catalog search parameters based on the expected field of view 942.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013092 (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 0.010473 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 16643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.4)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 16644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 16636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 967 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits N_match=967 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.436 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.416 n_q1=272 n_q2=314 n_q3=224 n_q4=157 worst_quadrant_to_overall_ratio=1.209
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits -region wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=7.291 worst_q_ratio=3.814
ref2=Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.406 worst_q_ratio=1.308
new1=fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits sigma_overall=0.370 worst_q_ratio=1.140
new2=fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits sigma_overall=0.360 worst_q_ratio=1.209
reference average sigma_overall=3.8485 worst_q_ratio=2.561
warn-on-ratio threshold: 2.0x reference
###################################
ERROR: reference image Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a bad plate solution (astrometric residuals 7.291 arcsec while the other reference image of the same field has 0.406 arcsec) - the magnitude calibration relying on it is unreliable
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png (331 matched stars from wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 3.06 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png (973 matched stars from wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206_astrometric_residuals.png (966 matched stars from wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207_astrometric_residuals.png (967 matched stars from wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-01-12_20.00sec_-0.00C_LIGHTs_0206.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-07_CI_Cas-03-Q1b1x1_010238_TTUQ1b1x1_896717_seRmQLOn/wcs_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207.fits'
Preparing the HTML report for the field Cas-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:44.06 +56:06:07.0: 14.01 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:30.18 +55:55:53.1: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:18.02 +56:19:04.5: 13.28 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:25.71 +55:59:07.3: 14.35 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:53.68 +56:14:27.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:34.26 +56:21:55.0: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:31.35 +57:11:40.9: 15.62 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.41 +55:54:24.4: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:25.71 +55:59:07.3: 9.46 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:30.18 +55:55:53.1: 9.73 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:34:30.18 +55:55:53.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:18.02 +56:19:04.5: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 02:33:18.02 +56:19:04.5: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:44.06 +56:06:07.0: 9.67 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:34.26 +56:21:55.0: 9.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.46 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:25.72 +56:07:04.8: 15.69 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 02:31:25.71 +55:59:07.3: ref_mag=9.46 +/- 0.00 new_mean_mag=9.5192 delta=-0.06 (need > 0.90)
Forced photometry reference-image weighted average: 9.67 +/- 0.00
Forced photometry reference-image weighted average: 9.58 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:44.06 +56:06:07.0: ref_mag=9.67 +/- 0.00 new_mean_mag=9.7952 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:34:34.26 +56:21:55.0: ref_mag=9.58 +/- 0.00 new_mean_mag=9.7187 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:31.35 +57:11:40.9: 10.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.11 +/- 0.00
Forced photometry filter REJECTED candidate at 02:36:31.35 +57:11:40.9: ref_mag=10.11 +/- 0.00 new_mean_mag=10.4450 delta=-0.34 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:13.42 +56:15:03.7: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:53.68 +56:14:27.9: 9.92 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.92 +/- 0.00
Forced photometry filter REJECTED candidate at 02:30:53.68 +56:14:27.9: ref_mag=9.92 +/- 0.00 new_mean_mag=9.8202 delta=0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.41 +55:54:24.4: 9.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.71 +/- 0.00
Forced photometry filter REJECTED candidate at 02:33:34.41 +55:54:24.4: ref_mag=9.71 +/- 0.00 new_mean_mag=9.8292 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:25.72 +56:07:04.8: 10.39 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:53.46 +56:34:44.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 10.39 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:26.38 +56:17:10.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 02:31:25.72 +56:07:04.8: ref_mag=10.39 +/- 0.00 new_mean_mag=10.0849 delta=0.31 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:43.09 +56:42:23.3: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:13.42 +56:15:03.7: 9.92 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:35:13.42 +56:15:03.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:30.37 +55:56:58.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:23.15 +56:25:37.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:26.38 +56:17:10.1: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:05.30 +56:25:31.9: 15.68 +/- 0.36 detection
Forced photometry filter REJECTED candidate at 02:36:26.38 +56:17:10.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:53.46 +56:34:44.7: 10.36 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:36:53.46 +56:34:44.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:43.09 +56:42:23.3: 10.33 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:36:43.09 +56:42:23.3: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:16.28 +59:42:59.0: 10.94 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:30.37 +55:56:58.9: 10.39 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:35:30.37 +55:56:58.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:25.80 +55:50:35.0: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:18.27 +56:21:26.6: 15.66 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:23.15 +56:25:37.2: 10.63 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:36:23.15 +56:25:37.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:45.48 +55:57:58.0: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:05.30 +56:25:31.9: 10.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.11 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:05.30 +56:25:31.9: ref_mag=10.11 +/- 0.00 new_mean_mag=10.1032 delta=0.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:16.28 +59:42:59.0: 10.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.75 +/- 0.00
Forced photometry filter REJECTED candidate at 00:52:16.28 +59:42:59.0: ref_mag=10.75 +/- 0.00 new_mean_mag=10.7955 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:25.80 +55:50:35.0: 10.91 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 02:34:25.80 +55:50:35.0: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:28.50 +56:22:24.3: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:18.27 +56:21:26.6: 10.83 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:49.32 +56:11:02.4: 15.38 +/- 0.25 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry filter REJECTED candidate at 02:32:18.27 +56:21:26.6: ref_mag=10.83 +/- 0.00 new_mean_mag=10.8292 delta=0.01 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:45.48 +55:57:58.0: 10.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.01
Forced photometry filter REJECTED candidate at 02:31:45.48 +55:57:58.0: ref_mag=10.98 +/- 0.01 new_mean_mag=10.8720 delta=0.11 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:44.12 +56:11:28.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.14 +56:11:48.0: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:28.50 +56:22:24.3: 11.38 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:18.25 +64:28:06.6: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.01
Forced photometry filter REJECTED candidate at 02:34:28.50 +56:22:24.3: ref_mag=11.38 +/- 0.01 new_mean_mag=10.9339 delta=0.45 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:49.32 +56:11:02.4: 11.00 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:05.12 +56:13:02.2: 15.65 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.00 +/- 0.01
Forced photometry filter REJECTED candidate at 02:30:49.32 +56:11:02.4: ref_mag=11.00 +/- 0.01 new_mean_mag=10.9440 delta=0.06 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:44.12 +56:11:28.4: 11.17 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:26.00 +56:29:14.2: 15.66 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 02:35:44.12 +56:11:28.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.14 +56:11:48.0: 10.89 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.89 +/- 0.00
Forced photometry filter REJECTED candidate at 02:33:34.14 +56:11:48.0: ref_mag=10.89 +/- 0.00 new_mean_mag=10.9932 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:13.95 +55:56:22.7: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.01 +56:12:35.7: 15.51 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:18.25 +64:28:06.6: 12.49 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:28.92 +56:28:21.8: 15.72 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 01:20:18.25 +64:28:06.6: ref_mag=12.56 +/- 0.01 new_mean_mag=11.3491 delta=1.21 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:05.12 +56:13:02.2: 11.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.32 +/- 0.01
Forced photometry filter REJECTED candidate at 02:33:05.12 +56:13:02.2: ref_mag=11.32 +/- 0.01 new_mean_mag=11.0718 delta=0.24 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:26.00 +56:29:14.2: 11.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.01
Forced photometry filter REJECTED candidate at 02:34:26.00 +56:29:14.2: ref_mag=11.13 +/- 0.01 new_mean_mag=11.0836 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:13.95 +55:56:22.7: 11.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.01
Forced photometry filter REJECTED candidate at 02:32:13.95 +55:56:22.7: ref_mag=11.06 +/- 0.01 new_mean_mag=11.0751 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.01 +56:12:35.7: 11.09 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:28.92 +56:28:21.8: 11.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.01
Forced photometry filter REJECTED candidate at 02:34:13.01 +56:12:35.7: ref_mag=11.09 +/- 0.01 new_mean_mag=11.2092 delta=-0.12 (need > 0.90)
Forced photometry reference-image weighted average: 11.12 +/- 0.01
Forced photometry filter REJECTED candidate at 02:35:28.92 +56:28:21.8: ref_mag=11.12 +/- 0.01 new_mean_mag=11.1888 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:58.04 +56:08:50.4: 15.67 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:14.56 +56:20:22.8: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:00.17 +56:00:29.6: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:09.95 +56:56:38.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:39.78 +56:10:16.3: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.64 +56:18:40.7: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:58.04 +56:08:50.4: 11.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.01
Forced photometry filter REJECTED candidate at 02:29:58.04 +56:08:50.4: ref_mag=11.42 +/- 0.01 new_mean_mag=11.2891 delta=0.14 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:14.56 +56:20:22.8: 11.55 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 02:36:14.56 +56:20:22.8: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:00.17 +56:00:29.6: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Forced photometry filter REJECTED candidate at 02:31:00.17 +56:00:29.6: ref_mag=11.25 +/- 0.01 new_mean_mag=11.3164 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:09.95 +56:56:38.2: 11.54 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 02:37:09.95 +56:56:38.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:39.78 +56:10:16.3: 11.34 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 02:35:39.78 +56:10:16.3: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:26.57 +56:00:56.5: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:39.03 +56:11:33.1: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.64 +56:18:40.7: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.01
Forced photometry filter REJECTED candidate at 02:34:13.64 +56:18:40.7: ref_mag=11.61 +/- 0.01 new_mean_mag=11.3972 delta=0.22 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:51.68 +56:11:00.4: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:26.57 +56:00:56.5: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Forced photometry filter REJECTED candidate at 02:29:26.57 +56:00:56.5: ref_mag=11.55 +/- 0.01 new_mean_mag=11.5185 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:39.03 +56:11:33.1: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter REJECTED candidate at 02:29:39.03 +56:11:33.1: ref_mag=11.99 +/- 0.01 new_mean_mag=11.4868 delta=0.50 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:59.43 +56:13:01.4: 13.83 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:51.68 +56:11:00.4: 11.68 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.12 +59:15:33.7: 15.94 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:50.80 +57:54:16.4: 15.75 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 02:33:51.68 +56:11:00.4: ref_mag=11.68 +/- 0.01 new_mean_mag=11.5870 delta=0.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:36.46 +58:48:08.4: 14.72 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:59.43 +56:13:01.4: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.01
Forced photometry filter REJECTED candidate at 02:29:59.43 +56:13:01.4: ref_mag=11.86 +/- 0.01 new_mean_mag=11.5682 delta=0.29 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:50.80 +57:54:16.4: 9.93 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.12 +59:15:33.7: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.93 +/- 0.00
Forced photometry filter REJECTED candidate at 02:37:50.80 +57:54:16.4: ref_mag=9.93 +/- 0.00 new_mean_mag=9.9408 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.12 +59:15:33.7: ref_mag=9.75 +/- 0.00 new_mean_mag=8.5774 delta=1.17 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:29.85 +59:24:31.5: 15.65 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:36.46 +58:48:08.4: 10.22 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:05.63 +56:37:26.5: 15.67 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.22 +/- 0.00
Forced photometry filter KEPT candidate at 01:43:36.46 +58:48:08.4: ref_mag=10.22 +/- 0.00 new_mean_mag=9.2970 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:40.73 +60:54:41.6: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:05.63 +56:37:26.5: 9.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.61 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:05.63 +56:37:26.5: ref_mag=9.61 +/- 0.00 new_mean_mag=9.7520 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:29.85 +59:24:31.5: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter KEPT candidate at 02:24:29.85 +59:24:31.5: ref_mag=11.92 +/- 0.01 new_mean_mag=10.8009 delta=1.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:40.73 +60:54:41.6: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Forced photometry filter KEPT candidate at 02:21:40.73 +60:54:41.6: ref_mag=11.02 +/- 0.00 new_mean_mag=9.5405 delta=1.48 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out52381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out12304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22210.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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: 2s
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Considering the candidate 52171_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52171_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52198_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52198_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52201_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52201_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:36:59.79 +63:08:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52212_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52212_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:34:58.48 +55:58:56.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52216_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52216_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:33:24.21 +56:01:04.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52224_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52224_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52234_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52234_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52240_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52240_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52245_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52245_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52246_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52246_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52252_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52252_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52265_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52265_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52268_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52268_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52270_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52270_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52295_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52295_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52296_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52296_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52301_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52301_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52304_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52304_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:34:26.94 +64:32:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52305_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52305_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52321_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52321_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52330_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52330_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52350_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52350_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52361_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52361_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52362_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52362_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52369_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52369_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52370_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52370_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52372_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52372_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:56:28.45 +60:47:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52377_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52377_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52381_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52381_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:20:18.25 +64:28:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 0.153 524828343402056448 020.07609894905 +64.46853446171 9.8729 8.4133 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52389_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52389_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52395_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52395_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52399_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52399_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52409_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52409_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52424_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52424_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52429_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52429_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52449_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52449_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:18:56.97 +57:10:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52452_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52452_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52453_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52453_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52466_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52466_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:32:19.29 +56:13:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52475_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52475_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52489_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52489_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52490_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52490_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52491_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52491_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52497_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52497_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:11:03.64 +57:20:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52503_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52503_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52507_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52507_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52513_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52513_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 52515_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 52515_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 20109_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 20109_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 02633_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 02633_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:15:23.79 +65:01:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23244_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 23244_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:01:28.15 +58:18:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20736_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 20736_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 22210_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 22210_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 51449_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 51449_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:30:27.34 +62:31:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25035_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 25035_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 17032_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 17032_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 29658_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 29658_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:22:51.61 +57:50:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02782_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 02782_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:33:23.81 +64:24:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12304_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 12304_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 08339_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 08339_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:20:32.78 +62:32:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23703_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 23703_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:54:53.94 +58:33:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21078_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 21078_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:43:07.97 +58:54:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250707_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250707_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250708_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250708_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250716_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250716_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250720_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250720_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250721_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250721_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250725_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250725_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250726_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250726_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:59:46.19 +63:47:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250727_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250727_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:57:03.71 +59:44:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250729_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250729_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250733_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250733_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250734_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250734_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250736_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250736_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:56:39.66 +58:20:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250740_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250740_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250741_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250741_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:01:30.96 +65:05:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250742_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250742_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250743_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250743_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250744_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250744_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 250746_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250746_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250750_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250750_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:31:43.66 +56:27:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250756_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250756_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250757_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250757_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:55:14.60 +59:32:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250759_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250759_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250765_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250765_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250768_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250768_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250794_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250794_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 250809_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250809_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:34:58.41 +55:58:56.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250810_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250810_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:48:46.91 +56:41:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250812_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250812_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:33:24.17 +56:01:04.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 250813_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250813_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 250824_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250824_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250832_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250832_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 250839_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250839_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250843_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250843_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 250844_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250844_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 250846_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250846_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250848_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250848_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250850_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250850_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250866_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250866_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 250869_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250869_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250871_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250871_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250874_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250874_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250876_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250876_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250899_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250899_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250901_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250901_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250903_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250903_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 250904_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250904_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 250905_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250905_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 250906_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250906_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250918_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250918_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250927_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250927_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250931_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250931_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250937_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250937_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250939_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250939_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250959_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250959_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250963_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250963_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250977_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250977_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250979_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250979_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250984_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250984_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250987_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250987_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 250988_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 250988_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 250995_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 250995_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:56:28.42 +60:47:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251000_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251000_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251004_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251004_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251008_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251008_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251010_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251010_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251011_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251011_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251016_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251016_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251017_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251017_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251022_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251022_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251025_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251025_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251034_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251034_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251043_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251043_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251045_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251045_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251053_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251053_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251068_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251068_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251077_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251077_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251083_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251083_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251101_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251101_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251102_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251102_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251110_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251110_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:32:19.25 +56:13:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251113_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251113_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251114_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251114_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251117_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251117_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251125_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251125_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251127_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251127_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251134_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251134_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251135_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251135_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251143_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251143_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251146_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251146_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251147_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251147_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251148_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251148_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251152_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251152_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:48:23.39 +60:58:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251160_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251160_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251163_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251163_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251171_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251171_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251176_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251176_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:56:38.48 +59:13:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251182_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251182_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251191_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251191_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251198_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251198_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251200_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251200_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251201_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251201_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251208_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251208_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251214_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251214_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251218_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251218_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251219_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251219_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251220_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251220_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251227_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251227_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251236_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251236_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251239_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251239_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:53:16.21 +61:08:53.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251240_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251240_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251241_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251241_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251245_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251245_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251246_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251246_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:03:47.01 +61:03:18.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251252_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251252_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251255_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251255_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251256_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251256_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:49:48.22 +65:05:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251271_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251271_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:38:00.55 +57:56:45.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251273_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251273_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251274_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251274_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251295_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251295_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251303_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251303_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:26:41.04 +60:46:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251306_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251306_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251307_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251307_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251308_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251308_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251309_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251309_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251311_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251311_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251319_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251319_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:47:26.01 +63:58:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251321_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251321_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251322_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251322_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251331_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251331_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251337_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251337_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251348_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251348_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251351_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251351_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251353_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251353_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251361_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251361_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251362_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251362_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:17:59.32 +57:47:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251376_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251376_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251377_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251377_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251388_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251388_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251390_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251390_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251396_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251396_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251398_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251398_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251408_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251408_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251410_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251410_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251415_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251415_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251418_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251418_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251420_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251420_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251423_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251423_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251430_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251430_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251431_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251431_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251456_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251456_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251459_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251459_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251466_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251466_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251467_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251467_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251468_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251468_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251474_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251474_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251481_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251481_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251482_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251482_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251483_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251483_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251486_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251486_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:21:50.87 +57:15:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251490_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251490_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251491_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251491_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251494_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251494_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251501_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251501_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:32:45.79 +56:29:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251504_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251504_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251505_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251505_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:16:08.57 +58:49:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251507_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251507_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251508_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251508_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:04:32.60 +57:59:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251514_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251514_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251517_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251517_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:20:13.82 +65:31:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251528_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251528_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251529_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251529_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251530_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251530_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:56:23.12 +59:10:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251531_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251531_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251538_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251538_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251545_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251545_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:35:15.02 +63:00:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251546_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251546_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251548_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251548_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:05:03.74 +64:21:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251552_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251552_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251555_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251555_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251560_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251560_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251566_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251566_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251571_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251571_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251572_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251572_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:31:15.63 +58:01:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251574_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251574_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251590_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251590_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251599_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251599_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251600_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251600_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251601_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251601_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251604_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251604_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251610_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251610_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251614_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251614_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251616_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251616_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251617_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251617_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251622_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251622_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251625_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251625_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251626_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251626_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:40:50.62 +64:17:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251630_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251630_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251633_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251633_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251634_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251634_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251638_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251638_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251640_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251640_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:49:04.03 +57:59:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251641_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251641_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:20:10.74 +58:12:11.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251645_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251645_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251648_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251648_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251649_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251649_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251656_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251656_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:58:01.30 +65:22:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251660_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251660_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251661_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251661_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251665_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251665_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251689_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251689_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:45:43.38 +56:47:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251693_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251693_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251694_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251694_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:23:23.74 +63:36:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251696_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251696_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251698_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251698_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251701_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251701_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251705_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251705_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251712_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251712_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251713_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251713_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251717_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251717_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251719_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251719_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251722_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251722_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251733_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251733_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:08:32.29 +63:35:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251738_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251738_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251739_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251739_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:44:17.55 +61:53:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251757_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251757_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251758_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251758_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251760_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251760_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251765_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251765_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251771_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251771_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251778_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251778_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251781_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251781_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:46:34.49 +63:01:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251782_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251782_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:02:55.19 +64:24:57.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251784_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251784_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251785_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251785_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251795_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251795_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251797_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251797_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251800_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251800_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251809_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251809_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:51:02.75 +64:49:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251813_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251813_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251820_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251820_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251830_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251830_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 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 251837_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251837_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251838_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251838_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:39:56.97 +60:52:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251844_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251844_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:07:40.93 +63:30:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251847_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251847_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251848_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251848_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251850_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251850_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251855_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251855_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:06:45.57 +59:50:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251861_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251861_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:46:33.73 +61:16:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251864_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251864_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251872_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251872_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
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Considering the candidate 251873_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251873_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251875_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251875_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251880_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251880_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:35:21.54 +56:08:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251883_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251883_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251886_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251886_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251895_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251895_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:43:03.55 +58:08:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251899_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251899_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251904_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251904_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251906_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251906_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251908_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251908_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251910_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251910_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:27:52.84 +62:46:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251917_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251917_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:00:35.90 +60:25:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251923_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251923_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:16:39.04 +57:02:20.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251928_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251928_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:36:29.01 +62:40:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251932_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251932_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251935_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251935_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:17:01.05 +61:40:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251936_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251936_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251938_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251938_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251940_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251940_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251945_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251945_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:54:01.10 +63:31:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251946_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251946_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251947_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251947_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:48:23.91 +65:06:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251950_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251950_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251951_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251951_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251952_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251952_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251956_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251956_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 251970_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251970_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251975_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251975_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:02:22.06 +60:42:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251978_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251978_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251989_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251989_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:50:02.70 +57:18:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251991_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 251991_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:04:26.90 +65:05:54.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 251995_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 251995_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252004_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252004_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:36:27.23 +65:08:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252008_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252008_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:33:23.30 +57:44:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252009_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252009_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:29:34.44 +63:19:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252016_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252016_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:04:08.56 +61:47:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252019_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252019_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:16:05.01 +58:49:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252036_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252036_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252039_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252039_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252040_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252040_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252042_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252042_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:00:37.25 +58:30:26.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252044_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252044_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:42:33.26 +63:52:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252045_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252045_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:35:54.55 +60:13:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252050_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252050_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:06:23.73 +62:44:02.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252054_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252054_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:19:12.08 +65:36:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252055_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252055_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252061_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252061_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252062_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252062_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252075_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252075_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252090_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252090_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:19:03.91 +63:57:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252091_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252091_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252094_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252094_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252097_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252097_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252100_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252100_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252102_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252102_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252110_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252110_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252114_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252114_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252118_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252118_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:10:27.42 +60:30:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252126_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252126_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:13:36.09 +57:52:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252127_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252127_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252131_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252131_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252139_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252139_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252150_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252150_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:47:18.56 +63:38:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252155_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252155_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:37:44.87 +64:45:47.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252159_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252159_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:25:50.27 +61:32:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252161_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252161_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:45:14.74 +64:24:34.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252170_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252170_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:35:50.61 +61:27:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252183_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252183_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:13:30.73 +58:34:25.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252184_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252184_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252186_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252186_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:51:09.13 +62:24:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252188_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252188_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252192_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252192_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252202_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252202_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:27:49.84 +62:54:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252203_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252203_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252220_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252220_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252223_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252223_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252224_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252224_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252233_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252233_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:54:18.87 +63:38:05.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252238_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252238_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252242_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252242_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252246_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252246_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252249_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252249_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252253_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252253_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252255_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252255_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:20:49.42 +64:40:21.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252262_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252262_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252269_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252269_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252273_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252273_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:56:05.20 +57:09:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252293_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252293_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:08:33.43 +63:34:27.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252294_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252294_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252299_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252299_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:00:53.39 +63:25:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252301_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252301_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252302_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252302_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252311_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252311_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252318_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252318_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:07:04.01 +59:51:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252321_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252321_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252323_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252323_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252327_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252327_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:01:29.92 +62:28:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252340_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252340_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:34:34.55 +65:48:57.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252342_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252342_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252344_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252344_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252345_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252345_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252354_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252354_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:16:37.47 +64:56:42.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252358_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252358_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252362_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252362_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252363_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252363_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252367_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252367_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:31:32.91 +61:02:19.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252372_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252372_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252382_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252382_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:54:51.49 +60:05:29.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252399_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252399_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252410_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252410_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252412_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252412_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252413_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252413_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252415_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252415_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252434_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252434_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:58:14.02 +60:44:12.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252435_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252435_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:42:55.12 +64:01:46.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252443_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252443_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:49:06.25 +65:23:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252447_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252447_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:43:13.03 +64:00:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252457_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252457_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:01:47.03 +61:46:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252466_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252466_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252469_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252469_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:16:14.14 +66:06:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252470_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252470_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:27:04.15 +64:43:34.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252474_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252474_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:38:12.12 +61:01:26.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252502_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252502_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252507_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252507_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252520_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252520_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252527_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252527_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:58:09.53 +61:55:59.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252543_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252543_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252554_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252554_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252561_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252561_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:18:04.47 +65:36:26.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252565_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252565_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:20:24.81 +64:00:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252570_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252570_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:27:56.48 +62:46:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252571_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252571_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:23:07.72 +61:11:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252577_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252577_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 252581_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252581_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:01:43.92 +63:37:09.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252615_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252615_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 252621_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252621_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 252641_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252641_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252644_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252644_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:03:07.83 +63:43:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252659_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 252659_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 252672_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252672_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:07:29.46 +63:11:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252721_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 252721_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:41:41.17 +57:56:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178605_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 178605_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233881_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 233881_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:28:43.74 +58:25:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168245_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 168245_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186036_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 186036_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:38:44.03 +58:15:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212460_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 212460_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:31:28.24 +57:20:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215315_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 215315_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169758_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 169758_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 64480_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 64480_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 194289_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 194289_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 114460_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 114460_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 214209_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 214209_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220392_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 220392_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104399_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 104399_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:21:40.71 +60:54:41.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 134840_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 134840_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 106568_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 106568_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 26060_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 26060_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198104_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 198104_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 112593_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 112593_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 214314_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 214314_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134816_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 134816_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:24:29.83 +59:24:31.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 62860_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 62860_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:11:58.87 +63:39:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70687_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 70687_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:37:10.04 +61:55:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67097_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 67097_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:36:59.80 +63:08:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21138_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 21138_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:15:23.78 +65:01:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23392_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 23392_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237870_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 237870_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64440_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 64440_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:18:52.31 +62:48:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72532_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 72532_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:45:35.94 +63:07:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211875_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 211875_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:11:03.63 +57:20:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174355_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 174355_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14863_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 14863_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:12:35.16 +65:31:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171906_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 171906_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179696_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 179696_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:29:57.30 +56:45:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197554_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 197554_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:24:17.36 +58:48:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136514_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 136514_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130602_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 130602_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158689_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 158689_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124320_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 124320_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34359_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 34359_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:34:26.97 +64:32:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14315_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 14315_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:50:27.29 +65:55:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137900_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 137900_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213664_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 213664_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166981_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 166981_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218015_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 218015_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235844_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 235844_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 70271_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:20:32.76 +62:32:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184393_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 184393_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178697_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 178697_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:01:20.07 +58:00:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75237_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 75237_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196734_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 196734_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234807_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 234807_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189876_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 189876_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154238_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 154238_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155598_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 155598_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196494_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 196494_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:01:28.12 +58:18:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12954_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 12954_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:13:31.09 +65:37:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152727_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 152727_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 173490_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 173490_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:22:51.62 +57:50:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96078_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 96078_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:43:44.94 +60:25:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162641_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 162641_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 62555_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 62555_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 234312_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 234312_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176794_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 176794_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 180134_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 180134_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 201907_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 201907_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:43:36.46 +58:48:08.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 168042_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 168042_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:09:37.99 +59:05:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39378_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 39378_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:47:55.79 +64:32:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 179380_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 179380_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:27:36.97 +56:48:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177454_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 177454_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 23333_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 23333_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 222553_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 222553_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150407_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 150407_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182351_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 182351_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 233570_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 233570_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 219425_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 219425_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 52771_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 52771_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 93555_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 93555_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 125111_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 125111_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 157757_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 157757_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 123519_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 123519_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 115890_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 115890_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 45963_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 45963_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 95275_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 95275_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 213022_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 213022_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:14:49.88 +57:23:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209662_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 209662_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:31:04.86 +57:13:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156692_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 156692_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:56:38.11 +59:15:33.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178813_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 178813_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:04:41.93 +57:30:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173182_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 173182_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 193780_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 193780_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 00:54:53.89 +58:33:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221536_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 221536_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 76951_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 76951_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 22840_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 22840_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:33:23.79 +64:24:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63215_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 63215_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:30:27.32 +62:31:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218524_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 218524_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 94055_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 94055_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 190235_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 190235_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 213141_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 213141_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 58464_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 58464_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 172650_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 172650_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:11:03.57 +57:47:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76362_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 76362_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 195946_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 195946_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 211642_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 211642_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 172562_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 172562_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:22:06.66 +56:36:16.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 61006_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 61006_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:54:23.63 +63:40:05.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 63240_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 63240_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:37:35.68 +62:13:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146540_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 146540_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:25:50.41 +60:14:05.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 167582_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 167582_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:33:56.03 +59:13:57.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 92255_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 92255_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:00:49.09 +62:16:09.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104341_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 104341_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 187039_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 187039_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:33:25.91 +58:19:40.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 178877_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 178877_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:38:07.67 +57:58:42.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 171363_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 171363_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:08:40.23 +58:25:26.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 153703_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 153703_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 183006_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 183006_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 01:20:05.26 +58:13:56.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 189206_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 189206_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:18:04.33 +57:30:58.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137025_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
Preparing report for the candidate 137025_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
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Considering the candidate 188414_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207
The candidate 188414_fd_Cas-03-Q1b1x1_2026-07-07_01-02-00_20.00sec_-0.00C_LIGHTs_0207 did not pass the final checks
**** FOUND 02:17:59.84 +57:53:59.9 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 21s
make_report_in_HTML.sh TOTAL: 594s
Prepared the HTML report for the field Cas-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:21:40.73 +60:54:41.6
02:24:29.85 +59:24:31.5
01:56:38.12 +59:15:33.7
01:43:36.46 +58:48:08.4
02:40:38.76 +60:07:56.2
02:10:17.96 +60:59:00.3
01:21:54.90 +61:20:55.9
01:14:11.39 +61:16:04.2
01:28:36.11 +61:12:07.3
02:08:59.25 +60:15:03.0
01:25:43.56 +60:50:05.6
01:33:44.66 +60:46:19.2
02:19:16.58 +59:42:22.1
02:38:01.93 +58:50:39.9
01:46:47.71 +60:09:41.2
01:35:09.81 +60:17:10.2
02:11:29.16 +59:35:35.7
01:14:56.64 +59:42:13.1
02:18:22.67 +58:47:10.8
01:24:30.55 +59:38:48.3
02:38:48.26 +57:57:35.1
02:37:50.78 +57:54:16.5
02:24:41.36 +58:22:34.6
02:19:34.20 +58:23:58.5
02:24:52.10 +58:00:24.5
01:58:35.42 +58:39:55.9
02:33:58.86 +57:33:07.0
02:37:21.05 +57:19:39.0
02:03:07.44 +57:18:15.2
02:31:45.74 +56:26:46.2
02:30:17.09 +56:38:10.3
02:10:41.36 +57:16:54.8
02:27:39.96 +56:48:08.2
02:34:05.62 +56:37:26.6
02:31:32.24 +56:47:59.3
02:22:56.66 +57:11:45.2
01:28:07.88 +58:27:03.1
02:03:35.37 +57:58:41.0
02:14:38.60 +57:52:11.6
02:31:31.11 +57:22:45.6
01:26:54.02 +58:45:08.8
02:05:05.79 +58:16:24.3
02:28:34.97 +56:03:02.6
02:31:58.69 +55:59:28.0
02:19:47.96 +56:25:10.1
02:33:59.56 +55:56:25.8
02:27:56.18 +56:10:22.0
02:34:12.75 +56:03:48.5
01:52:19.59 +57:19:07.0
02:09:55.29 +56:59:22.9
02:29:11.49 +56:22:46.6
02:31:18.68 +56:20:49.0
02:27:52.25 +56:32:26.5
02:10:01.04 +64:59:04.3
02:02:52.76 +63:13:25.1
02:28:12.03 +64:31:53.4
02:23:49.46 +56:41:26.7
02:32:02.00 +57:03:30.7
01:02:45.67 +63:46:46.0
01:55:33.43 +62:51:23.2
01:32:27.31 +64:14:12.8
02:04:53.86 +64:12:10.7
01:26:06.09 +59:01:11.0
01:51:44.29 +60:38:43.1
01:09:25.27 +64:35:19.7
01:13:07.51 +58:55:53.3
01:40:55.21 +57:55:17.8
02:18:13.88 +57:38:00.5
01:11:45.03 +61:13:57.5
00:56:47.64 +60:38:48.7
01:13:51.48 +58:12:20.1
00:54:31.45 +59:24:01.9
01:17:48.27 +57:17:35.1
02:25:56.68 +56:38:22.1
02:01:40.01 +58:27:27.8
00:52:55.14 +58:28:53.1
00:59:04.64 +61:08:53.8
01:01:40.14 +58:50:23.6
02:23:04.39 +56:30:08.5
02:33:52.47 +57:01:39.2
02:36:31.33 +57:11:40.8
02:31:25.68 +55:59:07.1
02:34:34.26 +56:21:55.4
02:34:43.98 +56:06:06.6
02:30:53.66 +56:14:27.7
02:33:34.37 +55:54:24.4
02:34:05.29 +56:25:32.0
02:31:25.68 +56:07:04.6
02:32:15.41 +56:38:50.3
02:29:11.88 +56:17:58.5
02:31:06.52 +56:30:41.9
02:32:55.20 +56:39:40.3
02:34:03.63 +56:30:43.3
02:30:12.38 +56:11:25.1
02:28:50.73 +56:20:49.0
02:31:37.61 +56:33:36.4
02:32:18.25 +56:21:26.4
02:31:45.44 +55:57:57.8
02:30:49.34 +56:11:02.2
02:30:37.31 +56:22:57.8
02:34:28.50 +56:22:24.5
02:33:34.12 +56:11:47.9
02:35:42.61 +56:44:19.7
02:29:40.94 +56:20:04.5
02:34:04.59 +56:42:29.8
02:34:26.00 +56:29:14.3
02:33:05.10 +56:13:02.1
02:28:49.03 +56:07:35.6
02:32:13.91 +55:56:22.5
02:34:13.00 +56:12:36.6
02:35:28.90 +56:28:21.8
02:30:03.66 +56:22:33.4
02:34:43.49 +56:34:06.4
02:29:58.04 +56:08:50.1
02:31:00.12 +56:00:29.2
02:34:13.62 +56:18:40.6
02:30:59.13 +56:08:43.7
02:28:34.90 +56:13:02.9
02:32:19.08 +56:15:24.4
02:29:39.02 +56:11:32.8
02:27:59.59 +56:09:19.5
02:34:12.75 +56:11:54.4
02:29:26.60 +56:00:56.3
02:29:59.42 +56:13:01.1
02:31:29.57 +56:26:21.8
02:33:51.65 +56:11:00.3
02:35:00.16 +56:43:10.0
02:30:43.88 +55:58:11.5
02:33:48.69 +55:57:06.6
02:30:00.30 +56:17:42.9
02:33:50.75 +55:59:56.4
02:28:41.03 +56:12:03.3
02:34:03.12 +56:00:34.9
02:28:56.63 +56:11:03.7
02:36:27.29 +56:56:50.8
02:34:09.50 +56:41:03.1
02:35:40.34 +56:37:58.5
02:34:34.53 +56:36:41.0
02:35:12.53 +56:50:10.0
02:33:28.33 +56:18:30.9
02:30:38.35 +56:11:55.5
02:34:37.65 +56:32:36.9
02:33:57.85 +56:36:42.0
02:34:43.75 +56:51:49.3
02:34:13.66 +56:19:36.9
02:34:22.42 +56:20:28.4
02:35:16.02 +56:26:20.3
02:28:10.75 +56:06:42.8
02:32:37.23 +56:00:39.2
02:29:46.43 +56:03:52.1
02:29:43.15 +56:05:11.6
02:29:39.10 +56:20:59.6
02:33:06.27 +56:00:33.3
02:35:22.31 +56:48:50.7
02:36:27.90 +56:50:29.8
02:31:43.40 +56:14:44.1
02:33:30.82 +56:43:01.2
02:36:18.23 +56:52:16.6
02:32:49.98 +56:14:33.6
02:33:02.07 +56:26:23.7
02:29:40.37 +56:13:41.1
02:33:07.80 +56:14:49.7
02:34:06.45 +56:06:18.8
02:29:33.63 +56:09:09.1
02:31:12.76 +56:27:39.4
02:30:38.96 +56:15:15.0
02:33:40.00 +56:00:07.2
02:31:04.55 +56:05:04.2
02:31:32.20 +56:41:26.6
02:34:20.44 +56:29:01.4
02:35:35.89 +56:45:06.5
01:18:14.29 +61:44:37.2
02:34:31.65 +56:11:10.4
02:30:49.94 +56:26:29.6
02:34:41.02 +56:11:01.2
01:58:16.33 +59:38:58.0
00:58:55.96 +58:04:06.0
02:36:20.12 +56:57:28.9
02:34:07.76 +56:29:06.5
01:20:56.93 +62:03:29.7
02:30:26.95 +56:10:13.2
02:32:54.24 +56:43:29.3
02:37:19.18 +57:14:52.0
02:34:09.77 +56:06:36.9
02:34:27.75 +56:43:25.0
02:29:16.26 +56:06:17.5
00:36:55.88 +62:32:57.4
02:32:36.04 +56:17:21.3
02:33:10.79 +56:00:07.1
02:34:25.23 +56:10:43.9
02:34:50.44 +56:14:15.1
02:35:36.46 +56:50:34.4
02:34:18.67 +56:07:36.4
01:29:33.01 +61:46:26.5
02:32:56.64 +56:40:53.9
02:29:17.29 +56:14:27.8
02:34:14.18 +56:14:09.6
02:33:48.88 +56:37:03.6
02:33:06.38 +56:40:26.3
02:30:25.27 +56:22:03.9
02:33:21.47 +56:24:37.7
02:30:31.77 +56:03:29.5
02:36:24.29 +56:49:27.5
01:22:23.94 +61:13:51.6
02:31:05.38 +56:00:31.6
02:32:31.70 +56:04:31.5
02:32:32.91 +56:21:52.5
02:32:29.84 +55:59:08.6
02:31:57.79 +56:05:41.6
00:52:12.50 +64:57:21.6
02:34:01.32 +56:28:57.2
02:24:56.80 +56:48:21.5
02:34:29.42 +56:26:00.5
02:34:22.66 +56:27:54.2
02:27:24.27 +56:18:01.8
02:33:00.93 +56:09:31.2
02:31:09.24 +56:03:13.3
02:30:43.64 +56:25:16.2
02:31:06.56 +56:11:58.4
02:29:37.98 +56:28:56.4
02:31:42.63 +56:28:20.1
02:35:20.59 +56:30:28.5
02:30:09.49 +56:13:06.4
02:34:14.15 +56:41:49.8
02:32:08.77 +55:55:37.5
02:30:43.84 +56:23:45.5
02:36:19.80 +56:48:29.7
02:26:52.95 +56:05:48.3
02:30:10.17 +56:16:14.7
00:51:32.84 +59:59:12.6
00:47:11.57 +58:29:06.7
02:31:28.87 +56:18:16.5
02:30:53.06 +56:31:32.6
02:27:18.79 +56:05:55.8
02:33:06.79 +56:01:45.3
02:31:41.25 +56:32:00.9
02:30:31.12 +56:33:56.5
01:19:41.75 +62:51:05.3
02:31:35.16 +56:11:21.0
01:13:12.83 +60:19:03.4
02:32:40.03 +56:36:59.2
02:32:47.85 +56:09:08.3
00:45:38.04 +56:46:39.0
02:36:38.41 +57:22:31.7
01:41:54.61 +62:34:04.7
02:34:49.29 +56:45:55.6
00:54:25.48 +60:12:30.6
02:29:02.28 +56:16:34.5
00:41:56.47 +63:42:31.2
02:31:41.77 +56:00:50.9
02:36:51.36 +57:09:36.5
02:30:46.17 +56:43:56.8
02:35:58.60 +56:46:23.5
02:32:16.64 +56:27:15.9
02:27:39.64 +56:13:54.9
02:35:00.66 +56:49:39.3
02:10:24.12 +60:01:13.6
02:35:30.82 +56:47:10.6
01:18:36.81 +58:41:39.1
01:38:33.84 +60:47:25.3
00:39:40.06 +61:06:36.3
02:32:40.73 +56:57:45.9
01:59:33.54 +60:01:44.6
02:31:36.56 +56:43:54.7
01:31:48.39 +64:21:55.8
02:36:01.82 +56:57:52.5
02:31:05.41 +56:13:06.4
02:32:56.45 +56:04:07.6
01:29:32.94 +63:19:37.2
01:18:48.37 +64:12:21.1
01:56:32.59 +59:56:29.5
02:01:39.11 +61:45:17.0
02:01:03.64 +64:43:31.2
02:02:54.02 +60:15:41.6
02:32:36.48 +56:53:27.0
01:55:53.21 +64:15:24.7
02:21:38.41 +65:44:30.3
01:38:06.02 +58:10:36.7
01:59:06.11 +59:55:34.4
01:31:48.54 +64:22:27.8
02:35:15.89 +56:49:40.2
02:34:25.60 +56:19:16.4
01:06:55.51 +59:18:57.7
02:33:21.63 +56:36:57.4
02:33:15.69 +56:38:32.9
01:23:08.00 +63:07:27.6
02:26:25.60 +56:08:18.7
02:14:27.88 +64:44:14.1
01:20:18.26 +64:28:06.1
01:50:36.62 +63:53:30.0
02:13:47.66 +63:11:26.5
02:27:22.01 +62:38:26.7
02:19:03.95 +62:47:34.1
02:14:40.15 +62:26:25.5
01:36:47.19 +63:02:42.2
01:58:48.66 +62:43:31.8
02:12:37.92 +61:35:07.5
01:25:24.78 +62:14:21.4
01:13:00.09 +62:10:43.8
########### Completed Cas-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:56:38.12 +59:15:33.7
01:43:36.46 +58:48:08.4
02:24:29.85 +59:24:31.5
02:21:40.73 +60:54:41.6
01:02:45.67 +63:46:46.0
01:55:33.43 +62:51:23.2
01:32:27.31 +64:14:12.8
02:04:53.86 +64:12:10.7
01:26:06.09 +59:01:11.0
01:51:44.29 +60:38:43.1
01:09:25.27 +64:35:19.7
01:13:07.51 +58:55:53.3
01:40:55.21 +57:55:17.8
02:18:13.88 +57:38:00.5
01:11:45.03 +61:13:57.5
00:56:47.64 +60:38:48.7
01:13:51.48 +58:12:20.1
00:54:31.45 +59:24:01.9
01:17:48.27 +57:17:35.1
02:25:56.68 +56:38:22.1
02:01:40.01 +58:27:27.8
00:52:55.14 +58:28:53.1
00:59:04.64 +61:08:53.8
01:01:40.14 +58:50:23.6
02:23:04.39 +56:30:08.5
02:33:52.47 +57:01:39.2
02:36:31.33 +57:11:40.8
02:31:25.68 +55:59:07.1
02:34:34.26 +56:21:55.4
02:34:43.98 +56:06:06.6
02:30:53.66 +56:14:27.7
02:33:34.37 +55:54:24.4
02:34:05.29 +56:25:32.0
02:31:25.68 +56:07:04.6
02:32:15.41 +56:38:50.3
02:29:11.88 +56:17:58.5
02:31:06.52 +56:30:41.9
02:32:55.20 +56:39:40.3
02:34:03.63 +56:30:43.3
02:30:12.38 +56:11:25.1
02:28:50.73 +56:20:49.0
02:31:37.61 +56:33:36.4
02:32:18.25 +56:21:26.4
02:31:45.44 +55:57:57.8
02:30:49.34 +56:11:02.2
02:30:37.31 +56:22:57.8
02:34:28.50 +56:22:24.5
02:33:34.12 +56:11:47.9
02:35:42.61 +56:44:19.7
02:29:40.94 +56:20:04.5
02:34:04.59 +56:42:29.8
02:34:26.00 +56:29:14.3
02:33:05.10 +56:13:02.1
02:28:49.03 +56:07:35.6
02:32:13.91 +55:56:22.5
02:34:13.00 +56:12:36.6
02:35:28.90 +56:28:21.8
02:30:03.66 +56:22:33.4
02:34:43.49 +56:34:06.4
02:29:58.04 +56:08:50.1
02:31:00.12 +56:00:29.2
02:34:13.62 +56:18:40.6
02:30:59.13 +56:08:43.7
02:28:34.90 +56:13:02.9
02:32:19.08 +56:15:24.4
02:29:39.02 +56:11:32.8
02:27:59.59 +56:09:19.5
02:34:12.75 +56:11:54.4
02:29:26.60 +56:00:56.3
02:29:59.42 +56:13:01.1
02:31:29.57 +56:26:21.8
02:33:51.65 +56:11:00.3
02:35:00.16 +56:43:10.0
02:30:43.88 +55:58:11.5
02:33:48.69 +55:57:06.6
02:30:00.30 +56:17:42.9
02:33:50.75 +55:59:56.4
02:28:41.03 +56:12:03.3
02:34:03.12 +56:00:34.9
02:28:56.63 +56:11:03.7
02:36:27.29 +56:56:50.8
02:34:09.50 +56:41:03.1
02:35:40.34 +56:37:58.5
02:34:34.53 +56:36:41.0
02:35:12.53 +56:50:10.0
02:33:28.33 +56:18:30.9
02:30:38.35 +56:11:55.5
02:34:37.65 +56:32:36.9
02:33:57.85 +56:36:42.0
02:34:43.75 +56:51:49.3
02:34:13.66 +56:19:36.9
02:34:22.42 +56:20:28.4
02:35:16.02 +56:26:20.3
02:28:10.75 +56:06:42.8
02:32:37.23 +56:00:39.2
02:29:46.43 +56:03:52.1
02:29:43.15 +56:05:11.6
02:29:39.10 +56:20:59.6
02:33:06.27 +56:00:33.3
02:35:22.31 +56:48:50.7
02:36:27.90 +56:50:29.8
02:31:43.40 +56:14:44.1
02:33:30.82 +56:43:01.2
02:36:18.23 +56:52:16.6
02:32:49.98 +56:14:33.6
02:33:02.07 +56:26:23.7
02:29:40.37 +56:13:41.1
02:33:07.80 +56:14:49.7
02:34:06.45 +56:06:18.8
02:29:33.63 +56:09:09.1
02:31:12.76 +56:27:39.4
02:30:38.96 +56:15:15.0
02:33:40.00 +56:00:07.2
02:31:04.55 +56:05:04.2
02:31:32.20 +56:41:26.6
02:34:20.44 +56:29:01.4
02:35:35.89 +56:45:06.5
01:18:14.29 +61:44:37.2
02:34:31.65 +56:11:10.4
02:30:49.94 +56:26:29.6
02:34:41.02 +56:11:01.2
01:58:16.33 +59:38:58.0
00:58:55.96 +58:04:06.0
02:36:20.12 +56:57:28.9
02:34:07.76 +56:29:06.5
01:20:56.93 +62:03:29.7
02:30:26.95 +56:10:13.2
02:32:54.24 +56:43:29.3
02:37:19.18 +57:14:52.0
02:34:09.77 +56:06:36.9
02:34:27.75 +56:43:25.0
02:29:16.26 +56:06:17.5
00:36:55.88 +62:32:57.4
02:32:36.04 +56:17:21.3
02:33:10.79 +56:00:07.1
02:34:25.23 +56:10:43.9
02:34:50.44 +56:14:15.1
02:35:36.46 +56:50:34.4
02:34:18.67 +56:07:36.4
01:29:33.01 +61:46:26.5
02:32:56.64 +56:40:53.9
02:29:17.29 +56:14:27.8
02:34:14.18 +56:14:09.6
02:33:48.88 +56:37:03.6
02:33:06.38 +56:40:26.3
02:30:25.27 +56:22:03.9
02:33:21.47 +56:24:37.7
02:30:31.77 +56:03:29.5
02:36:24.29 +56:49:27.5
01:22:23.94 +61:13:51.6
02:31:05.38 +56:00:31.6
02:32:31.70 +56:04:31.5
02:32:32.91 +56:21:52.5
02:32:29.84 +55:59:08.6
02:31:57.79 +56:05:41.6
00:52:12.50 +64:57:21.6
02:34:01.32 +56:28:57.2
02:24:56.80 +56:48:21.5
02:34:29.42 +56:26:00.5
02:34:22.66 +56:27:54.2
02:27:24.27 +56:18:01.8
02:33:00.93 +56:09:31.2
02:31:09.24 +56:03:13.3
02:30:43.64 +56:25:16.2
02:31:06.56 +56:11:58.4
02:29:37.98 +56:28:56.4
02:31:42.63 +56:28:20.1
02:35:20.59 +56:30:28.5
02:30:09.49 +56:13:06.4
02:34:14.15 +56:41:49.8
02:32:08.77 +55:55:37.5
02:30:43.84 +56:23:45.5
02:36:19.80 +56:48:29.7
02:26:52.95 +56:05:48.3
02:30:10.17 +56:16:14.7
00:51:32.84 +59:59:12.6
00:47:11.57 +58:29:06.7
02:31:28.87 +56:18:16.5
02:30:53.06 +56:31:32.6
02:27:18.79 +56:05:55.8
02:33:06.79 +56:01:45.3
02:31:41.25 +56:32:00.9
02:30:31.12 +56:33:56.5
01:19:41.75 +62:51:05.3
02:31:35.16 +56:11:21.0
01:13:12.83 +60:19:03.4
02:32:40.03 +56:36:59.2
02:32:47.85 +56:09:08.3
00:45:38.04 +56:46:39.0
02:36:38.41 +57:22:31.7
01:41:54.61 +62:34:04.7
02:34:49.29 +56:45:55.6
00:54:25.48 +60:12:30.6
02:29:02.28 +56:16:34.5
00:41:56.47 +63:42:31.2
02:31:41.77 +56:00:50.9
02:36:51.36 +57:09:36.5
02:30:46.17 +56:43:56.8
02:35:58.60 +56:46:23.5
02:32:16.64 +56:27:15.9
02:27:39.64 +56:13:54.9
02:35:00.66 +56:49:39.3
02:10:24.12 +60:01:13.6
02:35:30.82 +56:47:10.6
01:18:36.81 +58:41:39.1
01:38:33.84 +60:47:25.3
00:39:40.06 +61:06:36.3
02:32:40.73 +56:57:45.9
01:59:33.54 +60:01:44.6
02:31:36.56 +56:43:54.7
01:31:48.39 +64:21:55.8
02:36:01.82 +56:57:52.5
02:31:05.41 +56:13:06.4
02:32:56.45 +56:04:07.6
01:29:32.94 +63:19:37.2
01:18:48.37 +64:12:21.1
01:56:32.59 +59:56:29.5
02:01:39.11 +61:45:17.0
02:01:03.64 +64:43:31.2
02:02:54.02 +60:15:41.6
02:32:36.48 +56:53:27.0
01:55:53.21 +64:15:24.7
02:21:38.41 +65:44:30.3
01:38:06.02 +58:10:36.7
01:59:06.11 +59:55:34.4
01:31:48.54 +64:22:27.8
02:35:15.89 +56:49:40.2
02:34:25.60 +56:19:16.4
01:06:55.51 +59:18:57.7
02:33:21.63 +56:36:57.4
02:33:15.69 +56:38:32.9
01:23:08.00 +63:07:27.6
02:26:25.60 +56:08:18.7
02:27:39.96 +56:48:08.2
01:58:35.42 +58:39:55.9
02:33:58.86 +57:33:07.0
02:19:03.95 +62:47:34.1
02:14:38.60 +57:52:11.6
01:14:11.39 +61:16:04.2
02:33:59.56 +55:56:25.8
02:29:11.49 +56:22:46.6
02:38:01.93 +58:50:39.9
02:10:17.96 +60:59:00.3
02:14:27.88 +64:44:14.1
02:05:05.79 +58:16:24.3
01:21:54.90 +61:20:55.9
02:27:56.18 +56:10:22.0
02:28:12.03 +64:31:53.4
02:31:45.74 +56:26:46.2
02:37:21.05 +57:19:39.0
01:46:47.71 +60:09:41.2
02:19:16.58 +59:42:22.1
02:24:41.36 +58:22:34.6
01:25:43.56 +60:50:05.6
02:11:29.16 +59:35:35.7
02:19:47.96 +56:25:10.1
02:24:52.10 +58:00:24.5
02:34:12.75 +56:03:48.5
02:32:02.00 +57:03:30.7
02:22:56.66 +57:11:45.2
02:14:40.15 +62:26:25.5
01:26:54.02 +58:45:08.8
02:23:49.46 +56:41:26.7
01:28:07.88 +58:27:03.1
01:24:30.55 +59:38:48.3
02:38:48.26 +57:57:35.1
01:14:56.64 +59:42:13.1
02:19:34.20 +58:23:58.5
02:27:22.01 +62:38:26.7
02:30:17.09 +56:38:10.3
02:34:05.62 +56:37:26.6
02:10:41.36 +57:16:54.8
02:10:01.04 +64:59:04.3
02:27:52.25 +56:32:26.5
02:31:32.24 +56:47:59.3
02:02:52.76 +63:13:25.1
02:09:55.29 +56:59:22.9
01:50:36.62 +63:53:30.0
02:12:37.92 +61:35:07.5
01:33:44.66 +60:46:19.2
02:37:50.78 +57:54:16.5
02:08:59.25 +60:15:03.0
01:28:36.11 +61:12:07.3
01:20:18.26 +64:28:06.1
01:13:00.09 +62:10:43.8
02:03:07.44 +57:18:15.2
02:31:18.68 +56:20:49.0
01:58:48.66 +62:43:31.8
01:52:19.59 +57:19:07.0
01:25:24.78 +62:14:21.4
02:03:35.37 +57:58:41.0
02:31:58.69 +55:59:28.0
02:13:47.66 +63:11:26.5
01:36:47.19 +63:02:42.2
02:31:31.11 +57:22:45.6
02:28:34.97 +56:03:02.6
02:40:38.76 +60:07:56.2
02:18:22.67 +58:47:10.8
01:35:09.81 +60:17:10.2
###################################################################################
01:56:38.12 +59:15:33.7 -- not an asteroid (will add it to exclusion list)
01:43:36.46 +58:48:08.4 -- not an asteroid (will add it to exclusion list)
02:24:29.85 +59:24:31.5 -- not an asteroid (will add it to exclusion list)
02:21:40.73 +60:54:41.6 -- not an asteroid (will add it to exclusion list)
01:02:45.67 +63:46:46.0 -- not an asteroid (will add it to exclusion list)
01:55:33.43 +62:51:23.2 -- not an asteroid (will add it to exclusion list)
01:32:27.31 +64:14:12.8 -- not an asteroid (will add it to exclusion list)
02:04:53.86 +64:12:10.7 -- not an asteroid (will add it to exclusion list)
01:26:06.09 +59:01:11.0 -- not an asteroid (will add it to exclusion list)
01:51:44.29 +60:38:43.1 -- not an asteroid (will add it to exclusion list)
01:09:25.27 +64:35:19.7 -- not an asteroid (will add it to exclusion list)
01:13:07.51 +58:55:53.3 -- not an asteroid (will add it to exclusion list)
01:40:55.21 +57:55:17.8 -- not an asteroid (will add it to exclusion list)
02:18:13.88 +57:38:00.5 -- not an asteroid (will add it to exclusion list)
01:11:45.03 +61:13:57.5 -- not an asteroid (will add it to exclusion list)
00:56:47.64 +60:38:48.7 -- not an asteroid (will add it to exclusion list)
01:13:51.48 +58:12:20.1 -- not an asteroid (will add it to exclusion list)
00:54:31.45 +59:24:01.9 -- not an asteroid (will add it to exclusion list)
01:17:48.27 +57:17:35.1 -- not an asteroid (will add it to exclusion list)
02:25:56.68 +56:38:22.1 -- not an asteroid (will add it to exclusion list)
02:01:40.01 +58:27:27.8 -- not an asteroid (will add it to exclusion list)
00:52:55.14 +58:28:53.1 -- not an asteroid (will add it to exclusion list)
00:59:04.64 +61:08:53.8 -- not an asteroid (will add it to exclusion list)
01:01:40.14 +58:50:23.6 -- not an asteroid (will add it to exclusion list)
02:23:04.39 +56:30:08.5 -- not an asteroid (will add it to exclusion list)
02:33:52.47 +57:01:39.2 -- not an asteroid (will add it to exclusion list)
02:36:31.33 +57:11:40.8 -- not an asteroid (will add it to exclusion list)
02:31:25.68 +55:59:07.1 -- not an asteroid (will add it to exclusion list)
02:34:34.26 +56:21:55.4 -- not an asteroid (will add it to exclusion list)
02:34:43.98 +56:06:06.6 -- not an asteroid (will add it to exclusion list)
02:30:53.66 +56:14:27.7 -- not an asteroid (will add it to exclusion list)
02:33:34.37 +55:54:24.4 -- not an asteroid (will add it to exclusion list)
02:34:05.29 +56:25:32.0 -- not an asteroid (will add it to exclusion list)
02:31:25.68 +56:07:04.6 -- not an asteroid (will add it to exclusion list)
02:32:15.41 +56:38:50.3 -- not an asteroid (will add it to exclusion list)
02:29:11.88 +56:17:58.5 -- not an asteroid (will add it to exclusion list)
02:31:06.52 +56:30:41.9 -- not an asteroid (will add it to exclusion list)
02:32:55.20 +56:39:40.3 -- not an asteroid (will add it to exclusion list)
02:34:03.63 +56:30:43.3 -- not an asteroid (will add it to exclusion list)
02:30:12.38 +56:11:25.1 -- not an asteroid (will add it to exclusion list)
02:28:50.73 +56:20:49.0 -- not an asteroid (will add it to exclusion list)
02:31:37.61 +56:33:36.4 -- not an asteroid (will add it to exclusion list)
02:32:18.25 +56:21:26.4 -- not an asteroid (will add it to exclusion list)
02:31:45.44 +55:57:57.8 -- not an asteroid (will add it to exclusion list)
02:30:49.34 +56:11:02.2 -- not an asteroid (will add it to exclusion list)
02:30:37.31 +56:22:57.8 -- not an asteroid (will add it to exclusion list)
02:34:28.50 +56:22:24.5 -- not an asteroid (will add it to exclusion list)
02:33:34.12 +56:11:47.9 -- not an asteroid (will add it to exclusion list)
02:35:42.61 +56:44:19.7 -- not an asteroid (will add it to exclusion list)
02:29:40.94 +56:20:04.5 -- not an asteroid (will add it to exclusion list)
02:34:04.59 +56:42:29.8 -- not an asteroid (will add it to exclusion list)
02:34:26.00 +56:29:14.3 -- not an asteroid (will add it to exclusion list)
02:33:05.10 +56:13:02.1 -- not an asteroid (will add it to exclusion list)
02:28:49.03 +56:07:35.6 -- not an asteroid (will add it to exclusion list)
02:32:13.91 +55:56:22.5 -- not an asteroid (will add it to exclusion list)
02:34:13.00 +56:12:36.6 -- not an asteroid (will add it to exclusion list)
02:35:28.90 +56:28:21.8 -- not an asteroid (will add it to exclusion list)
02:30:03.66 +56:22:33.4 -- not an asteroid (will add it to exclusion list)
02:34:43.49 +56:34:06.4 -- not an asteroid (will add it to exclusion list)
02:29:58.04 +56:08:50.1 -- not an asteroid (will add it to exclusion list)
02:31:00.12 +56:00:29.2 -- not an asteroid (will add it to exclusion list)
02:34:13.62 +56:18:40.6 -- not an asteroid (will add it to exclusion list)
02:30:59.13 +56:08:43.7 -- not an asteroid (will add it to exclusion list)
02:28:34.90 +56:13:02.9 -- not an asteroid (will add it to exclusion list)
02:32:19.08 +56:15:24.4 -- not an asteroid (will add it to exclusion list)
02:29:39.02 +56:11:32.8 -- not an asteroid (will add it to exclusion list)
02:27:59.59 +56:09:19.5 -- not an asteroid (will add it to exclusion list)
02:34:12.75 +56:11:54.4 -- not an asteroid (will add it to exclusion list)
02:29:26.60 +56:00:56.3 -- not an asteroid (will add it to exclusion list)
02:29:59.42 +56:13:01.1 -- not an asteroid (will add it to exclusion list)
02:31:29.57 +56:26:21.8 -- not an asteroid (will add it to exclusion list)
02:33:51.65 +56:11:00.3 -- not an asteroid (will add it to exclusion list)
02:35:00.16 +56:43:10.0 -- not an asteroid (will add it to exclusion list)
02:30:43.88 +55:58:11.5 -- not an asteroid (will add it to exclusion list)
02:33:48.69 +55:57:06.6 -- not an asteroid (will add it to exclusion list)
02:30:00.30 +56:17:42.9 -- not an asteroid (will add it to exclusion list)
02:33:50.75 +55:59:56.4 -- not an asteroid (will add it to exclusion list)
02:28:41.03 +56:12:03.3 -- not an asteroid (will add it to exclusion list)
02:34:03.12 +56:00:34.9 -- not an asteroid (will add it to exclusion list)
02:28:56.63 +56:11:03.7 -- not an asteroid (will add it to exclusion list)
02:36:27.29 +56:56:50.8 -- not an asteroid (will add it to exclusion list)
02:34:09.50 +56:41:03.1 -- not an asteroid (will add it to exclusion list)
02:35:40.34 +56:37:58.5 -- not an asteroid (will add it to exclusion list)
02:34:34.53 +56:36:41.0 -- not an asteroid (will add it to exclusion list)
02:35:12.53 +56:50:10.0 -- not an asteroid (will add it to exclusion list)
02:33:28.33 +56:18:30.9 -- not an asteroid (will add it to exclusion list)
02:30:38.35 +56:11:55.5 -- not an asteroid (will add it to exclusion list)
02:34:37.65 +56:32:36.9 -- not an asteroid (will add it to exclusion list)
02:33:57.85 +56:36:42.0 -- not an asteroid (will add it to exclusion list)
02:34:43.75 +56:51:49.3 -- not an asteroid (will add it to exclusion list)
02:34:13.66 +56:19:36.9 -- not an asteroid (will add it to exclusion list)
02:34:22.42 +56:20:28.4 -- not an asteroid (will add it to exclusion list)
02:35:16.02 +56:26:20.3 -- not an asteroid (will add it to exclusion list)
02:28:10.75 +56:06:42.8 -- not an asteroid (will add it to exclusion list)
02:32:37.23 +56:00:39.2 -- not an asteroid (will add it to exclusion list)
02:29:46.43 +56:03:52.1 -- not an asteroid (will add it to exclusion list)
02:29:43.15 +56:05:11.6 -- not an asteroid (will add it to exclusion list)
02:29:39.10 +56:20:59.6 -- not an asteroid (will add it to exclusion list)
02:33:06.27 +56:00:33.3 -- not an asteroid (will add it to exclusion list)
02:35:22.31 +56:48:50.7 -- not an asteroid (will add it to exclusion list)
02:36:27.90 +56:50:29.8 -- not an asteroid (will add it to exclusion list)
02:31:43.40 +56:14:44.1 -- not an asteroid (will add it to exclusion list)
02:33:30.82 +56:43:01.2 -- not an asteroid (will add it to exclusion list)
02:36:18.23 +56:52:16.6 -- not an asteroid (will add it to exclusion list)
02:32:49.98 +56:14:33.6 -- not an asteroid (will add it to exclusion list)
02:33:02.07 +56:26:23.7 -- not an asteroid (will add it to exclusion list)
02:29:40.37 +56:13:41.1 -- not an asteroid (will add it to exclusion list)
02:33:07.80 +56:14:49.7 -- not an asteroid (will add it to exclusion list)
02:34:06.45 +56:06:18.8 -- not an asteroid (will add it to exclusion list)
02:29:33.63 +56:09:09.1 -- not an asteroid (will add it to exclusion list)
02:31:12.76 +56:27:39.4 -- not an asteroid (will add it to exclusion list)
02:30:38.96 +56:15:15.0 -- not an asteroid (will add it to exclusion list)
02:33:40.00 +56:00:07.2 -- not an asteroid (will add it to exclusion list)
02:31:04.55 +56:05:04.2 -- not an asteroid (will add it to exclusion list)
02:31:32.20 +56:41:26.6 -- not an asteroid (will add it to exclusion list)
02:34:20.44 +56:29:01.4 -- not an asteroid (will add it to exclusion list)
02:35:35.89 +56:45:06.5 -- not an asteroid (will add it to exclusion list)
01:18:14.29 +61:44:37.2 -- not an asteroid (will add it to exclusion list)
02:34:31.65 +56:11:10.4 -- not an asteroid (will add it to exclusion list)
02:30:49.94 +56:26:29.6 -- not an asteroid (will add it to exclusion list)
02:34:41.02 +56:11:01.2 -- not an asteroid (will add it to exclusion list)
01:58:16.33 +59:38:58.0 -- not an asteroid (will add it to exclusion list)
00:58:55.96 +58:04:06.0 -- not an asteroid (will add it to exclusion list)
02:36:20.12 +56:57:28.9 -- not an asteroid (will add it to exclusion list)
02:34:07.76 +56:29:06.5 -- not an asteroid (will add it to exclusion list)
01:20:56.93 +62:03:29.7 -- not an asteroid (will add it to exclusion list)
02:30:26.95 +56:10:13.2 -- not an asteroid (will add it to exclusion list)
02:32:54.24 +56:43:29.3 -- not an asteroid (will add it to exclusion list)
02:37:19.18 +57:14:52.0 -- not an asteroid (will add it to exclusion list)
02:34:09.77 +56:06:36.9 -- not an asteroid (will add it to exclusion list)
02:34:27.75 +56:43:25.0 -- not an asteroid (will add it to exclusion list)
02:29:16.26 +56:06:17.5 -- not an asteroid (will add it to exclusion list)
00:36:55.88 +62:32:57.4 -- not an asteroid (will add it to exclusion list)
02:32:36.04 +56:17:21.3 -- not an asteroid (will add it to exclusion list)
02:33:10.79 +56:00:07.1 -- not an asteroid (will add it to exclusion list)
02:34:25.23 +56:10:43.9 -- not an asteroid (will add it to exclusion list)
02:34:50.44 +56:14:15.1 -- not an asteroid (will add it to exclusion list)
02:35:36.46 +56:50:34.4 -- not an asteroid (will add it to exclusion list)
02:34:18.67 +56:07:36.4 -- not an asteroid (will add it to exclusion list)
01:29:33.01 +61:46:26.5 -- not an asteroid (will add it to exclusion list)
02:32:56.64 +56:40:53.9 -- not an asteroid (will add it to exclusion list)
02:29:17.29 +56:14:27.8 -- not an asteroid (will add it to exclusion list)
02:34:14.18 +56:14:09.6 -- not an asteroid (will add it to exclusion list)
02:33:48.88 +56:37:03.6 -- not an asteroid (will add it to exclusion list)
02:33:06.38 +56:40:26.3 -- not an asteroid (will add it to exclusion list)
02:30:25.27 +56:22:03.9 -- not an asteroid (will add it to exclusion list)
02:33:21.47 +56:24:37.7 -- not an asteroid (will add it to exclusion list)
02:30:31.77 +56:03:29.5 -- not an asteroid (will add it to exclusion list)
02:36:24.29 +56:49:27.5 -- not an asteroid (will add it to exclusion list)
01:22:23.94 +61:13:51.6 -- not an asteroid (will add it to exclusion list)
02:31:05.38 +56:00:31.6 -- not an asteroid (will add it to exclusion list)
02:32:31.70 +56:04:31.5 -- not an asteroid (will add it to exclusion list)
02:32:32.91 +56:21:52.5 -- not an asteroid (will add it to exclusion list)
02:32:29.84 +55:59:08.6 -- not an asteroid (will add it to exclusion list)
02:31:57.79 +56:05:41.6 -- not an asteroid (will add it to exclusion list)
00:52:12.50 +64:57:21.6 -- not an asteroid (will add it to exclusion list)
02:34:01.32 +56:28:57.2 -- not an asteroid (will add it to exclusion list)
02:24:56.80 +56:48:21.5 -- not an asteroid (will add it to exclusion list)
02:34:29.42 +56:26:00.5 -- not an asteroid (will add it to exclusion list)
02:34:22.66 +56:27:54.2 -- not an asteroid (will add it to exclusion list)
02:27:24.27 +56:18:01.8 -- not an asteroid (will add it to exclusion list)
02:33:00.93 +56:09:31.2 -- not an asteroid (will add it to exclusion list)
02:31:09.24 +56:03:13.3 -- not an asteroid (will add it to exclusion list)
02:30:43.64 +56:25:16.2 -- not an asteroid (will add it to exclusion list)
02:31:06.56 +56:11:58.4 -- not an asteroid (will add it to exclusion list)
02:29:37.98 +56:28:56.4 -- not an asteroid (will add it to exclusion list)
02:31:42.63 +56:28:20.1 -- not an asteroid (will add it to exclusion list)
02:35:20.59 +56:30:28.5 -- not an asteroid (will add it to exclusion list)
02:30:09.49 +56:13:06.4 -- not an asteroid (will add it to exclusion list)
02:34:14.15 +56:41:49.8 -- not an asteroid (will add it to exclusion list)
02:32:08.77 +55:55:37.5 -- not an asteroid (will add it to exclusion list)
02:30:43.84 +56:23:45.5 -- not an asteroid (will add it to exclusion list)
02:36:19.80 +56:48:29.7 -- not an asteroid (will add it to exclusion list)
02:26:52.95 +56:05:48.3 -- not an asteroid (will add it to exclusion list)
02:30:10.17 +56:16:14.7 -- not an asteroid (will add it to exclusion list)
00:51:32.84 +59:59:12.6 -- not an asteroid (will add it to exclusion list)
00:47:11.57 +58:29:06.7 -- not an asteroid (will add it to exclusion list)
02:31:28.87 +56:18:16.5 -- not an asteroid (will add it to exclusion list)
02:30:53.06 +56:31:32.6 -- not an asteroid (will add it to exclusion list)
02:27:18.79 +56:05:55.8 -- not an asteroid (will add it to exclusion list)
02:33:06.79 +56:01:45.3 -- not an asteroid (will add it to exclusion list)
02:31:41.25 +56:32:00.9 -- not an asteroid (will add it to exclusion list)
02:30:31.12 +56:33:56.5 -- not an asteroid (will add it to exclusion list)
01:19:41.75 +62:51:05.3 -- not an asteroid (will add it to exclusion list)
02:31:35.16 +56:11:21.0 -- not an asteroid (will add it to exclusion list)
01:13:12.83 +60:19:03.4 -- not an asteroid (will add it to exclusion list)
02:32:40.03 +56:36:59.2 -- not an asteroid (will add it to exclusion list)
02:32:47.85 +56:09:08.3 -- not an asteroid (will add it to exclusion list)
00:45:38.04 +56:46:39.0 -- not an asteroid (will add it to exclusion list)
02:36:38.41 +57:22:31.7 -- not an asteroid (will add it to exclusion list)
01:41:54.61 +62:34:04.7 -- not an asteroid (will add it to exclusion list)
02:34:49.29 +56:45:55.6 -- not an asteroid (will add it to exclusion list)
00:54:25.48 +60:12:30.6 -- not an asteroid (will add it to exclusion list)
02:29:02.28 +56:16:34.5 -- not an asteroid (will add it to exclusion list)
00:41:56.47 +63:42:31.2 -- not an asteroid (will add it to exclusion list)
02:31:41.77 +56:00:50.9 -- not an asteroid (will add it to exclusion list)
02:36:51.36 +57:09:36.5 -- not an asteroid (will add it to exclusion list)
02:30:46.17 +56:43:56.8 -- not an asteroid (will add it to exclusion list)
02:35:58.60 +56:46:23.5 -- not an asteroid (will add it to exclusion list)
02:32:16.64 +56:27:15.9 -- not an asteroid (will add it to exclusion list)
02:27:39.64 +56:13:54.9 -- not an asteroid (will add it to exclusion list)
02:35:00.66 +56:49:39.3 -- not an asteroid (will add it to exclusion list)
02:10:24.12 +60:01:13.6 -- not an asteroid (will add it to exclusion list)
02:35:30.82 +56:47:10.6 -- not an asteroid (will add it to exclusion list)
01:18:36.81 +58:41:39.1 -- not an asteroid (will add it to exclusion list)
01:38:33.84 +60:47:25.3 -- not an asteroid (will add it to exclusion list)
00:39:40.06 +61:06:36.3 -- not an asteroid (will add it to exclusion list)
02:32:40.73 +56:57:45.9 -- not an asteroid (will add it to exclusion list)
01:59:33.54 +60:01:44.6 -- not an asteroid (will add it to exclusion list)
02:31:36.56 +56:43:54.7 -- not an asteroid (will add it to exclusion list)
01:31:48.39 +64:21:55.8 -- not an asteroid (will add it to exclusion list)
02:36:01.82 +56:57:52.5 -- not an asteroid (will add it to exclusion list)
02:31:05.41 +56:13:06.4 -- not an asteroid (will add it to exclusion list)
02:32:56.45 +56:04:07.6 -- not an asteroid (will add it to exclusion list)
01:29:32.94 +63:19:37.2 -- not an asteroid (will add it to exclusion list)
01:18:48.37 +64:12:21.1 -- not an asteroid (will add it to exclusion list)
01:56:32.59 +59:56:29.5 -- not an asteroid (will add it to exclusion list)
02:01:39.11 +61:45:17.0 -- not an asteroid (will add it to exclusion list)
02:01:03.64 +64:43:31.2 -- not an asteroid (will add it to exclusion list)
02:02:54.02 +60:15:41.6 -- not an asteroid (will add it to exclusion list)
02:32:36.48 +56:53:27.0 -- not an asteroid (will add it to exclusion list)
01:55:53.21 +64:15:24.7 -- not an asteroid (will add it to exclusion list)
02:21:38.41 +65:44:30.3 -- not an asteroid (will add it to exclusion list)
01:38:06.02 +58:10:36.7 -- not an asteroid (will add it to exclusion list)
01:59:06.11 +59:55:34.4 -- not an asteroid (will add it to exclusion list)
01:31:48.54 +64:22:27.8 -- not an asteroid (will add it to exclusion list)
02:35:15.89 +56:49:40.2 -- not an asteroid (will add it to exclusion list)
02:34:25.60 +56:19:16.4 -- not an asteroid (will add it to exclusion list)
01:06:55.51 +59:18:57.7 -- not an asteroid (will add it to exclusion list)
02:33:21.63 +56:36:57.4 -- not an asteroid (will add it to exclusion list)
02:33:15.69 +56:38:32.9 -- not an asteroid (will add it to exclusion list)
01:23:08.00 +63:07:27.6 -- not an asteroid (will add it to exclusion list)
02:26:25.60 +56:08:18.7 -- not an asteroid (will add it to exclusion list)
02:27:39.96 +56:48:08.2 -- not an asteroid (will add it to exclusion list)
01:58:35.42 +58:39:55.9 -- not an asteroid (will add it to exclusion list)
02:33:58.86 +57:33:07.0 -- not an asteroid (will add it to exclusion list)
02:19:03.95 +62:47:34.1 -- not an asteroid (will add it to exclusion list)
02:14:38.60 +57:52:11.6 -- not an asteroid (will add it to exclusion list)
01:14:11.39 +61:16:04.2 -- not an asteroid (will add it to exclusion list)
02:33:59.56 +55:56:25.8 -- not an asteroid (will add it to exclusion list)
02:29:11.49 +56:22:46.6 -- not an asteroid (will add it to exclusion list)
02:38:01.93 +58:50:39.9 -- not an asteroid (will add it to exclusion list)
02:10:17.96 +60:59:00.3 -- not an asteroid (will add it to exclusion list)
02:14:27.88 +64:44:14.1 -- not an asteroid (will add it to exclusion list)
02:05:05.79 +58:16:24.3 -- not an asteroid (will add it to exclusion list)
01:21:54.90 +61:20:55.9 -- not an asteroid (will add it to exclusion list)
02:27:56.18 +56:10:22.0 -- not an asteroid (will add it to exclusion list)
02:28:12.03 +64:31:53.4 -- not an asteroid (will add it to exclusion list)
02:31:45.74 +56:26:46.2 -- not an asteroid (will add it to exclusion list)
02:37:21.05 +57:19:39.0 -- not an asteroid (will add it to exclusion list)
01:46:47.71 +60:09:41.2 -- not an asteroid (will add it to exclusion list)
02:19:16.58 +59:42:22.1 -- not an asteroid (will add it to exclusion list)
02:24:41.36 +58:22:34.6 -- not an asteroid (will add it to exclusion list)
01:25:43.56 +60:50:05.6 -- not an asteroid (will add it to exclusion list)
02:11:29.16 +59:35:35.7 -- not an asteroid (will add it to exclusion list)
02:19:47.96 +56:25:10.1 -- not an asteroid (will add it to exclusion list)
02:24:52.10 +58:00:24.5 -- not an asteroid (will add it to exclusion list)
02:34:12.75 +56:03:48.5 -- not an asteroid (will add it to exclusion list)
02:32:02.00 +57:03:30.7 -- not an asteroid (will add it to exclusion list)
02:22:56.66 +57:11:45.2 -- not an asteroid (will add it to exclusion list)
02:14:40.15 +62:26:25.5 -- not an asteroid (will add it to exclusion list)
01:26:54.02 +58:45:08.8 -- not an asteroid (will add it to exclusion list)
02:23:49.46 +56:41:26.7 -- not an asteroid (will add it to exclusion list)
01:28:07.88 +58:27:03.1 -- not an asteroid (will add it to exclusion list)
01:24:30.55 +59:38:48.3 -- not an asteroid (will add it to exclusion list)
02:38:48.26 +57:57:35.1 -- not an asteroid (will add it to exclusion list)
01:14:56.64 +59:42:13.1 -- not an asteroid (will add it to exclusion list)
02:19:34.20 +58:23:58.5 -- not an asteroid (will add it to exclusion list)
02:27:22.01 +62:38:26.7 -- not an asteroid (will add it to exclusion list)
02:30:17.09 +56:38:10.3 -- not an asteroid (will add it to exclusion list)
02:34:05.62 +56:37:26.6 -- not an asteroid (will add it to exclusion list)
02:10:41.36 +57:16:54.8 -- not an asteroid (will add it to exclusion list)
02:10:01.04 +64:59:04.3 -- not an asteroid (will add it to exclusion list)
02:27:52.25 +56:32:26.5 -- not an asteroid (will add it to exclusion list)
02:31:32.24 +56:47:59.3 -- not an asteroid (will add it to exclusion list)
02:02:52.76 +63:13:25.1 -- not an asteroid (will add it to exclusion list)
02:09:55.29 +56:59:22.9 -- not an asteroid (will add it to exclusion list)
01:50:36.62 +63:53:30.0 -- not an asteroid (will add it to exclusion list)
02:12:37.92 +61:35:07.5 -- not an asteroid (will add it to exclusion list)
01:33:44.66 +60:46:19.2 -- not an asteroid (will add it to exclusion list)
02:37:50.78 +57:54:16.5 -- not an asteroid (will add it to exclusion list)
02:08:59.25 +60:15:03.0 -- not an asteroid (will add it to exclusion list)
01:28:36.11 +61:12:07.3 -- not an asteroid (will add it to exclusion list)
01:20:18.26 +64:28:06.1 -- not an asteroid (will add it to exclusion list)
01:13:00.09 +62:10:43.8 -- not an asteroid (will add it to exclusion list)
02:03:07.44 +57:18:15.2 -- not an asteroid (will add it to exclusion list)
02:31:18.68 +56:20:49.0 -- not an asteroid (will add it to exclusion list)
01:58:48.66 +62:43:31.8 -- not an asteroid (will add it to exclusion list)
01:52:19.59 +57:19:07.0 -- not an asteroid (will add it to exclusion list)
01:25:24.78 +62:14:21.4 -- not an asteroid (will add it to exclusion list)
02:03:35.37 +57:58:41.0 -- not an asteroid (will add it to exclusion list)
02:31:58.69 +55:59:28.0 -- not an asteroid (will add it to exclusion list)
02:13:47.66 +63:11:26.5 -- not an asteroid (will add it to exclusion list)
01:36:47.19 +63:02:42.2 -- not an asteroid (will add it to exclusion list)
02:31:31.11 +57:22:45.6 -- not an asteroid (will add it to exclusion list)
02:28:34.97 +56:03:02.6 -- not an asteroid (will add it to exclusion list)
02:40:38.76 +60:07:56.2 -- not an asteroid (will add it to exclusion list)
02:18:22.67 +58:47:10.8 -- not an asteroid (will add it to exclusion list)
01:35:09.81 +60:17:10.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:36:55.88 +62:32:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:40.06 +61:06:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:56.47 +63:42:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:38.04 +56:46:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:11.57 +58:29:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:32.84 +59:59:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:12.50 +64:57:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:55.14 +58:28:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:25.48 +60:12:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:31.45 +59:24:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:47.64 +60:38:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:55.96 +58:04:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:04.64 +61:08:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:40.14 +58:50:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:45.67 +63:46:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:55.51 +59:18:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:25.27 +64:35:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:45.03 +61:13:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:00.09 +62:10:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:07.51 +58:55:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:12.83 +60:19:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:51.48 +58:12:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:11.39 +61:16:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:56.64 +59:42:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:48.27 +57:17:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:14.29 +61:44:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:36.81 +58:41:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:48.37 +64:12:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:41.75 +62:51:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:18.26 +64:28:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:56.93 +62:03:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:54.90 +61:20:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:23.94 +61:13:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:08.00 +63:07:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:30.55 +59:38:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:24.78 +62:14:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:43.56 +60:50:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:06.09 +59:01:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:54.02 +58:45:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:07.88 +58:27:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:36.11 +61:12:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:32.94 +63:19:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:33.01 +61:46:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.39 +64:21:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.54 +64:22:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:27.31 +64:14:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:44.66 +60:46:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:09.81 +60:17:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:47.19 +63:02:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:06.02 +58:10:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:33.84 +60:47:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:55.21 +57:55:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:54.61 +62:34:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:36.46 +58:48:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:47.71 +60:09:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:36.62 +63:53:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:44.29 +60:38:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:19.59 +57:19:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:33.43 +62:51:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:53.21 +64:15:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:32.59 +59:56:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.12 +59:15:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:16.33 +59:38:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:35.42 +58:39:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:48.66 +62:43:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:06.11 +59:55:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:33.54 +60:01:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:03.64 +64:43:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:39.11 +61:45:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:40.01 +58:27:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:52.76 +63:13:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:54.02 +60:15:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:07.44 +57:18:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:35.37 +57:58:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:53.86 +64:12:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:05.79 +58:16:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:59.25 +60:15:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:09:55.29 +56:59:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:01.04 +64:59:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:17.96 +60:59:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:24.12 +60:01:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:41.36 +57:16:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:29.16 +59:35:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:37.92 +61:35:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:47.66 +63:11:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:27.88 +64:44:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:38.60 +57:52:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:14:40.15 +62:26:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:13.88 +57:38:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:22.67 +58:47:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:03.95 +62:47:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:16.58 +59:42:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:34.20 +58:23:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:47.96 +56:25:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:38.41 +65:44:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:40.73 +60:54:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:56.66 +57:11:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:04.39 +56:30:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:49.46 +56:41:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:29.85 +59:24:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:41.36 +58:22:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:52.10 +58:00:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:56.80 +56:48:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:56.68 +56:38:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:25.60 +56:08:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:52.95 +56:05:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:18.79 +56:05:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:22.01 +62:38:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:24.27 +56:18:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:39.64 +56:13:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:39.96 +56:48:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:52.25 +56:32:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:56.18 +56:10:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:59.59 +56:09:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:10.75 +56:06:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:12.03 +64:31:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:34.90 +56:13:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:34.97 +56:03:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:41.03 +56:12:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:49.03 +56:07:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:50.73 +56:20:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:56.63 +56:11:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:02.28 +56:16:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:11.49 +56:22:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:11.88 +56:17:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:16.26 +56:06:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:17.29 +56:14:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:26.60 +56:00:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:33.63 +56:09:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:37.98 +56:28:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:39.02 +56:11:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:39.10 +56:20:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:40.37 +56:13:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:40.94 +56:20:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:43.15 +56:05:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:46.43 +56:03:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:58.04 +56:08:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:59.42 +56:13:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:00.30 +56:17:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:03.66 +56:22:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:09.49 +56:13:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:10.17 +56:16:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:12.38 +56:11:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:17.09 +56:38:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:25.27 +56:22:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:26.95 +56:10:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:31.12 +56:33:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:31.77 +56:03:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:37.31 +56:22:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:38.35 +56:11:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:38.96 +56:15:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:43.64 +56:25:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:43.84 +56:23:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:43.88 +55:58:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:46.17 +56:43:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:49.34 +56:11:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:49.94 +56:26:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:53.06 +56:31:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:53.66 +56:14:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:59.13 +56:08:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:00.12 +56:00:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:04.55 +56:05:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:05.38 +56:00:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:05.41 +56:13:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:06.52 +56:30:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:06.56 +56:11:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:09.24 +56:03:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:12.76 +56:27:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:18.68 +56:20:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:25.68 +55:59:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:25.68 +56:07:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:28.87 +56:18:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:29.57 +56:26:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:31.11 +57:22:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:32.20 +56:41:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:32.24 +56:47:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:35.16 +56:11:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:36.56 +56:43:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:37.61 +56:33:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:41.25 +56:32:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:41.77 +56:00:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:42.63 +56:28:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:43.40 +56:14:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:45.44 +55:57:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:45.74 +56:26:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:57.79 +56:05:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:58.69 +55:59:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:02.00 +57:03:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:08.77 +55:55:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:13.91 +55:56:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:15.41 +56:38:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:16.64 +56:27:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:18.25 +56:21:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:19.08 +56:15:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:29.84 +55:59:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:31.70 +56:04:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:32.91 +56:21:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:36.04 +56:17:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:36.48 +56:53:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:37.23 +56:00:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:40.03 +56:36:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:40.73 +56:57:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:47.85 +56:09:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:49.98 +56:14:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:54.24 +56:43:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:55.20 +56:39:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:56.45 +56:04:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:56.64 +56:40:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:00.93 +56:09:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:02.07 +56:26:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:05.10 +56:13:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:06.27 +56:00:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:06.38 +56:40:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:06.79 +56:01:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:07.80 +56:14:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:10.79 +56:00:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:15.69 +56:38:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:21.47 +56:24:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:21.63 +56:36:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:28.33 +56:18:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:30.82 +56:43:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:34.12 +56:11:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:34.37 +55:54:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:40.00 +56:00:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:48.69 +55:57:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:48.88 +56:37:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:50.75 +55:59:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:51.65 +56:11:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:52.47 +57:01:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:57.85 +56:36:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:58.86 +57:33:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:59.56 +55:56:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:01.32 +56:28:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:03.12 +56:00:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:03.63 +56:30:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:04.59 +56:42:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:05.29 +56:25:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:05.62 +56:37:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:06.45 +56:06:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:07.76 +56:29:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:09.50 +56:41:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:09.77 +56:06:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:12.75 +56:03:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:12.75 +56:11:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:13.00 +56:12:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:13.62 +56:18:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:13.66 +56:19:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:14.15 +56:41:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:14.18 +56:14:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:18.67 +56:07:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:20.44 +56:29:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:22.42 +56:20:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:22.66 +56:27:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:25.23 +56:10:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:25.60 +56:19:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:26.00 +56:29:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:27.75 +56:43:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:28.50 +56:22:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:29.42 +56:26:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:31.65 +56:11:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:34.26 +56:21:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:34.53 +56:36:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:37.65 +56:32:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:41.02 +56:11:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:43.49 +56:34:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:43.75 +56:51:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:43.98 +56:06:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:49.29 +56:45:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:50.44 +56:14:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:00.16 +56:43:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:00.66 +56:49:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:12.53 +56:50:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:15.89 +56:49:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:16.02 +56:26:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:20.59 +56:30:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:22.31 +56:48:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:28.90 +56:28:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:30.82 +56:47:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:35.89 +56:45:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:36.46 +56:50:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:40.34 +56:37:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:42.61 +56:44:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:58.60 +56:46:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:01.82 +56:57:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:18.23 +56:52:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:19.80 +56:48:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:20.12 +56:57:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:24.29 +56:49:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:27.29 +56:56:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:27.90 +56:50:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:31.33 +57:11:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:38.41 +57:22:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:51.36 +57:09:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:19.18 +57:14:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:21.05 +57:19:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:50.78 +57:54:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:01.93 +58:50:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:48.26 +57:57:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:40:38.76 +60:07:56.2 -- 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)
00:36:55.88 +62:32:57.4 -- not a known variable star
00:39:40.06 +61:06:36.3 -- a known variable star
00:41:56.47 +63:42:31.2 -- a known variable star
00:45:38.04 +56:46:39.0 -- not a known variable star
00:47:11.57 +58:29:06.7 -- not a known variable star
00:51:32.84 +59:59:12.6 -- not a known variable star
00:52:12.50 +64:57:21.6 -- not a known variable star
00:52:55.14 +58:28:53.1 -- not a known variable star
00:54:25.48 +60:12:30.6 -- not a known variable star
00:54:31.45 +59:24:01.9 -- a known variable star
00:56:47.64 +60:38:48.7 -- not a known variable star
00:58:55.96 +58:04:06.0 -- not a known variable star
00:59:04.64 +61:08:53.8 -- not a known variable star
01:01:40.14 +58:50:23.6 -- not a known variable star
01:02:45.67 +63:46:46.0 -- not a known variable star
01:06:55.51 +59:18:57.7 -- not a known variable star
01:09:25.27 +64:35:19.7 -- not a known variable star
01:11:45.03 +61:13:57.5 -- a known variable star
01:13:00.09 +62:10:43.8 -- a known variable star
01:13:07.51 +58:55:53.3 -- a known variable star
01:13:12.83 +60:19:03.4 -- a known variable star
01:13:51.48 +58:12:20.1 -- not a known variable star
01:14:11.39 +61:16:04.2 -- a known variable star
01:14:56.64 +59:42:13.1 -- a known variable star
01:17:48.27 +57:17:35.1 -- not a known variable star
01:18:14.29 +61:44:37.2 -- not a known variable star
01:18:36.81 +58:41:39.1 -- a known variable star
01:18:48.37 +64:12:21.1 -- not a known variable star
01:19:41.75 +62:51:05.3 -- not a known variable star
01:20:18.26 +64:28:06.1 -- a known variable star
01:20:56.93 +62:03:29.7 -- not a known variable star
01:21:54.90 +61:20:55.9 -- a known variable star
01:22:23.94 +61:13:51.6 -- a known variable star
01:23:08.00 +63:07:27.6 -- not a known variable star
01:24:30.55 +59:38:48.3 -- a known variable star
01:25:24.78 +62:14:21.4 -- a known variable star
01:25:43.56 +60:50:05.6 -- a known variable star
01:26:06.09 +59:01:11.0 -- not a known variable star
01:26:54.02 +58:45:08.8 -- a known variable star
01:28:07.88 +58:27:03.1 -- a known variable star
01:28:36.11 +61:12:07.3 -- a known variable star
01:29:32.94 +63:19:37.2 -- a known variable star
01:29:33.01 +61:46:26.5 -- not a known variable star
01:31:48.39 +64:21:55.8 -- not a known variable star
01:31:48.54 +64:22:27.8 -- not a known variable star
01:32:27.31 +64:14:12.8 -- not a known variable star
01:33:44.66 +60:46:19.2 -- not a known variable star
01:35:09.81 +60:17:10.2 -- a known variable star
01:36:47.19 +63:02:42.2 -- a known variable star
01:38:06.02 +58:10:36.7 -- a known variable star
01:38:33.84 +60:47:25.3 -- not a known variable star
01:40:55.21 +57:55:17.8 -- not a known variable star
01:41:54.61 +62:34:04.7 -- a known variable star
01:43:36.46 +58:48:08.4 -- a known variable star
01:46:47.71 +60:09:41.2 -- a known variable star
01:50:36.62 +63:53:30.0 -- a known variable star
01:51:44.29 +60:38:43.1 -- a known variable star
01:52:19.59 +57:19:07.0 -- a known variable star
01:55:33.43 +62:51:23.2 -- a known variable star
01:55:53.21 +64:15:24.7 -- not a known variable star
01:56:32.59 +59:56:29.5 -- a known variable star
01:56:38.12 +59:15:33.7 -- a known variable star
01:58:16.33 +59:38:58.0 -- not a known variable star
01:58:35.42 +58:39:55.9 -- a known variable star
01:58:48.66 +62:43:31.8 -- a known variable star
01:59:06.11 +59:55:34.4 -- not a known variable star
01:59:33.54 +60:01:44.6 -- a known variable star
02:01:03.64 +64:43:31.2 -- not a known variable star
02:01:39.11 +61:45:17.0 -- not a known variable star
02:01:40.01 +58:27:27.8 -- a known variable star
02:02:52.76 +63:13:25.1 -- a known variable star
02:02:54.02 +60:15:41.6 -- not a known variable star
02:03:07.44 +57:18:15.2 -- a known variable star
02:03:35.37 +57:58:41.0 -- a known variable star
02:04:53.86 +64:12:10.7 -- not a known variable star
02:05:05.79 +58:16:24.3 -- a known variable star
02:08:59.25 +60:15:03.0 -- a known variable star
02:09:55.29 +56:59:22.9 -- a known variable star
02:10:01.04 +64:59:04.3 -- not a known variable star
02:10:17.96 +60:59:00.3 -- a known variable star
02:10:24.12 +60:01:13.6 -- not a known variable star
02:10:41.36 +57:16:54.8 -- not a known variable star
02:11:29.16 +59:35:35.7 -- a known variable star
02:12:37.92 +61:35:07.5 -- a known variable star
02:13:47.66 +63:11:26.5 -- a known variable star
02:14:27.88 +64:44:14.1 -- a known variable star
02:14:38.60 +57:52:11.6 -- a known variable star
02:14:40.15 +62:26:25.5 -- a known variable star
02:18:13.88 +57:38:00.5 -- not a known variable star
02:18:22.67 +58:47:10.8 -- a known variable star
02:19:03.95 +62:47:34.1 -- a known variable star
02:19:16.58 +59:42:22.1 -- a known variable star
02:19:34.20 +58:23:58.5 -- a known variable star
02:19:47.96 +56:25:10.1 -- not a known variable star
02:21:38.41 +65:44:30.3 -- not a known variable star
02:21:40.73 +60:54:41.6 -- a known variable star
02:22:56.66 +57:11:45.2 -- not a known variable star
02:23:04.39 +56:30:08.5 -- not a known variable star
02:23:49.46 +56:41:26.7 -- not a known variable star
02:24:29.85 +59:24:31.5 -- a known variable star
02:24:41.36 +58:22:34.6 -- a known variable star
02:24:52.10 +58:00:24.5 -- a known variable star
02:24:56.80 +56:48:21.5 -- not a known variable star
02:25:56.68 +56:38:22.1 -- not a known variable star
02:26:25.60 +56:08:18.7 -- a known variable star
02:26:52.95 +56:05:48.3 -- not a known variable star
02:27:18.79 +56:05:55.8 -- not a known variable star
02:27:22.01 +62:38:26.7 -- a known variable star
02:27:24.27 +56:18:01.8 -- not a known variable star
02:27:39.64 +56:13:54.9 -- not a known variable star
02:27:39.96 +56:48:08.2 -- not a known variable star
02:27:52.25 +56:32:26.5 -- not a known variable star
02:27:56.18 +56:10:22.0 -- not a known variable star
02:27:59.59 +56:09:19.5 -- not a known variable star
02:28:10.75 +56:06:42.8 -- not a known variable star
02:28:12.03 +64:31:53.4 -- a known variable star
02:28:34.90 +56:13:02.9 -- not a known variable star
02:28:34.97 +56:03:02.6 -- not a known variable star
02:28:41.03 +56:12:03.3 -- a known variable star
02:28:49.03 +56:07:35.6 -- a known variable star
02:28:50.73 +56:20:49.0 -- not a known variable star
02:28:56.63 +56:11:03.7 -- a known variable star
02:29:02.28 +56:16:34.5 -- not a known variable star
02:29:11.49 +56:22:46.6 -- not a known variable star
02:29:11.88 +56:17:58.5 -- not a known variable star
02:29:16.26 +56:06:17.5 -- not a known variable star
02:29:17.29 +56:14:27.8 -- not a known variable star
02:29:26.60 +56:00:56.3 -- not a known variable star
02:29:33.63 +56:09:09.1 -- not a known variable star
02:29:37.98 +56:28:56.4 -- a known variable star
02:29:39.02 +56:11:32.8 -- a known variable star
02:29:39.10 +56:20:59.6 -- not a known variable star
02:29:40.37 +56:13:41.1 -- not a known variable star
02:29:40.94 +56:20:04.5 -- not a known variable star
02:29:43.15 +56:05:11.6 -- not a known variable star
02:29:46.43 +56:03:52.1 -- not a known variable star
02:29:58.04 +56:08:50.1 -- not a known variable star
02:29:59.42 +56:13:01.1 -- not a known variable star
02:30:00.30 +56:17:42.9 -- not a known variable star
02:30:03.66 +56:22:33.4 -- not a known variable star
02:30:09.49 +56:13:06.4 -- not a known variable star
02:30:10.17 +56:16:14.7 -- not a known variable star
02:30:12.38 +56:11:25.1 -- a known variable star
02:30:17.09 +56:38:10.3 -- not a known variable star
02:30:25.27 +56:22:03.9 -- a known variable star
02:30:26.95 +56:10:13.2 -- not a known variable star
02:30:31.12 +56:33:56.5 -- not a known variable star
02:30:31.77 +56:03:29.5 -- not a known variable star
02:30:37.31 +56:22:57.8 -- a known variable star
02:30:38.35 +56:11:55.5 -- not a known variable star
02:30:38.96 +56:15:15.0 -- not a known variable star
02:30:43.64 +56:25:16.2 -- not a known variable star
02:30:43.84 +56:23:45.5 -- not a known variable star
02:30:43.88 +55:58:11.5 -- not a known variable star
02:30:46.17 +56:43:56.8 -- not a known variable star
02:30:49.34 +56:11:02.2 -- not a known variable star
02:30:49.94 +56:26:29.6 -- not a known variable star
02:30:53.06 +56:31:32.6 -- not a known variable star
02:30:53.66 +56:14:27.7 -- not a known variable star
02:30:59.13 +56:08:43.7 -- not a known variable star
02:31:00.12 +56:00:29.2 -- not a known variable star
02:31:04.55 +56:05:04.2 -- a known variable star
02:31:05.38 +56:00:31.6 -- not a known variable star
02:31:05.41 +56:13:06.4 -- a known variable star
02:31:06.52 +56:30:41.9 -- not a known variable star
02:31:06.56 +56:11:58.4 -- not a known variable star
02:31:09.24 +56:03:13.3 -- not a known variable star
02:31:12.76 +56:27:39.4 -- a known variable star
02:31:18.68 +56:20:49.0 -- not a known variable star
02:31:25.68 +55:59:07.1 -- a known variable star
02:31:25.68 +56:07:04.6 -- not a known variable star
02:31:28.87 +56:18:16.5 -- not a known variable star
02:31:29.57 +56:26:21.8 -- not a known variable star
02:31:31.11 +57:22:45.6 -- not a known variable star
02:31:32.20 +56:41:26.6 -- not a known variable star
02:31:32.24 +56:47:59.3 -- not a known variable star
02:31:35.16 +56:11:21.0 -- a known variable star
02:31:36.56 +56:43:54.7 -- not a known variable star
02:31:37.61 +56:33:36.4 -- a known variable star
02:31:41.25 +56:32:00.9 -- not a known variable star
02:31:41.77 +56:00:50.9 -- a known variable star
02:31:42.63 +56:28:20.1 -- not a known variable star
02:31:43.40 +56:14:44.1 -- not a known variable star
02:31:45.44 +55:57:57.8 -- not a known variable star
02:31:45.74 +56:26:46.2 -- not a known variable star
02:31:57.79 +56:05:41.6 -- not a known variable star
02:31:58.69 +55:59:28.0 -- not a known variable star
02:32:02.00 +57:03:30.7 -- not a known variable star
02:32:08.77 +55:55:37.5 -- not a known variable star
02:32:13.91 +55:56:22.5 -- a known variable star
02:32:15.41 +56:38:50.3 -- not a known variable star
02:32:16.64 +56:27:15.9 -- not a known variable star
02:32:18.25 +56:21:26.4 -- not a known variable star
02:32:19.08 +56:15:24.4 -- a known variable star
02:32:29.84 +55:59:08.6 -- not a known variable star
02:32:31.70 +56:04:31.5 -- a known variable star
02:32:32.91 +56:21:52.5 -- a known variable star
02:32:36.04 +56:17:21.3 -- not a known variable star
02:32:36.48 +56:53:27.0 -- a known variable star
02:32:37.23 +56:00:39.2 -- not a known variable star
02:32:40.03 +56:36:59.2 -- not a known variable star
02:32:40.73 +56:57:45.9 -- not a known variable star
02:32:47.85 +56:09:08.3 -- not a known variable star
02:32:49.98 +56:14:33.6 -- a known variable star
02:32:54.24 +56:43:29.3 -- not a known variable star
02:32:55.20 +56:39:40.3 -- not a known variable star
02:32:56.45 +56:04:07.6 -- not a known variable star
02:32:56.64 +56:40:53.9 -- not a known variable star
02:33:00.93 +56:09:31.2 -- not a known variable star
02:33:02.07 +56:26:23.7 -- not a known variable star
02:33:05.10 +56:13:02.1 -- not a known variable star
02:33:06.27 +56:00:33.3 -- not a known variable star
02:33:06.38 +56:40:26.3 -- not a known variable star
02:33:06.79 +56:01:45.3 -- not a known variable star
02:33:07.80 +56:14:49.7 -- not a known variable star
02:33:10.79 +56:00:07.1 -- not a known variable star
02:33:15.69 +56:38:32.9 -- not a known variable star
02:33:21.47 +56:24:37.7 -- not a known variable star
02:33:21.63 +56:36:57.4 -- not a known variable star
02:33:28.33 +56:18:30.9 -- not a known variable star
02:33:30.82 +56:43:01.2 -- not a known variable star
02:33:34.12 +56:11:47.9 -- a known variable star
02:33:34.37 +55:54:24.4 -- not a known variable star
02:33:40.00 +56:00:07.2 -- not a known variable star
02:33:48.69 +55:57:06.6 -- not a known variable star
02:33:48.88 +56:37:03.6 -- not a known variable star
02:33:50.75 +55:59:56.4 -- not a known variable star
02:33:51.65 +56:11:00.3 -- not a known variable star
02:33:52.47 +57:01:39.2 -- a known variable star
02:33:57.85 +56:36:42.0 -- not a known variable star
02:33:58.86 +57:33:07.0 -- not a known variable star
02:33:59.56 +55:56:25.8 -- a known variable star
02:34:01.32 +56:28:57.2 -- not a known variable star
02:34:03.12 +56:00:34.9 -- not a known variable star
02:34:03.63 +56:30:43.3 -- not a known variable star
02:34:04.59 +56:42:29.8 -- a known variable star
02:34:05.29 +56:25:32.0 -- not a known variable star
02:34:05.62 +56:37:26.6 -- a known variable star
02:34:06.45 +56:06:18.8 -- a known variable star
02:34:07.76 +56:29:06.5 -- not a known variable star
02:34:09.50 +56:41:03.1 -- a known variable star
02:34:09.77 +56:06:36.9 -- a known variable star
02:34:12.75 +56:03:48.5 -- not a known variable star
02:34:12.75 +56:11:54.4 -- not a known variable star
02:34:13.00 +56:12:36.6 -- a known variable star
02:34:13.62 +56:18:40.6 -- not a known variable star
02:34:13.66 +56:19:36.9 -- a known variable star
02:34:14.15 +56:41:49.8 -- not a known variable star
02:34:14.18 +56:14:09.6 -- not a known variable star
02:34:18.67 +56:07:36.4 -- not a known variable star
02:34:20.44 +56:29:01.4 -- not a known variable star
02:34:22.42 +56:20:28.4 -- not a known variable star
02:34:22.66 +56:27:54.2 -- not a known variable star
02:34:25.23 +56:10:43.9 -- not a known variable star
02:34:25.60 +56:19:16.4 -- not a known variable star
02:34:26.00 +56:29:14.3 -- not a known variable star
02:34:27.75 +56:43:25.0 -- not a known variable star
02:34:28.50 +56:22:24.5 -- not a known variable star
02:34:29.42 +56:26:00.5 -- not a known variable star
02:34:31.65 +56:11:10.4 -- not a known variable star
02:34:34.26 +56:21:55.4 -- not a known variable star
02:34:34.53 +56:36:41.0 -- not a known variable star
02:34:37.65 +56:32:36.9 -- not a known variable star
02:34:41.02 +56:11:01.2 -- not a known variable star
02:34:43.49 +56:34:06.4 -- a known variable star
02:34:43.75 +56:51:49.3 -- not a known variable star
02:34:43.98 +56:06:06.6 -- not a known variable star
02:34:49.29 +56:45:55.6 -- not a known variable star
02:34:50.44 +56:14:15.1 -- a known variable star
02:35:00.16 +56:43:10.0 -- not a known variable star
02:35:00.66 +56:49:39.3 -- a known variable star
02:35:12.53 +56:50:10.0 -- not a known variable star
02:35:15.89 +56:49:40.2 -- not a known variable star
02:35:16.02 +56:26:20.3 -- not a known variable star
02:35:20.59 +56:30:28.5 -- not a known variable star
02:35:22.31 +56:48:50.7 -- a known variable star
02:35:28.90 +56:28:21.8 -- a known variable star
02:35:30.82 +56:47:10.6 -- a known variable star
02:35:35.89 +56:45:06.5 -- not a known variable star
02:35:36.46 +56:50:34.4 -- not a known variable star
02:35:40.34 +56:37:58.5 -- not a known variable star
02:35:42.61 +56:44:19.7 -- a known variable star
02:35:58.60 +56:46:23.5 -- not a known variable star
02:36:01.82 +56:57:52.5 -- not a known variable star
02:36:18.23 +56:52:16.6 -- not a known variable star
02:36:19.80 +56:48:29.7 -- not a known variable star
02:36:20.12 +56:57:28.9 -- a known variable star
02:36:24.29 +56:49:27.5 -- not a known variable star
02:36:27.29 +56:56:50.8 -- not a known variable star
02:36:27.90 +56:50:29.8 -- not a known variable star
02:36:31.33 +57:11:40.8 -- not a known variable star
02:36:38.41 +57:22:31.7 -- not a known variable star
02:36:51.36 +57:09:36.5 -- not a known variable star
02:37:19.18 +57:14:52.0 -- not a known variable star
02:37:21.05 +57:19:39.0 -- not a known variable star
02:37:50.78 +57:54:16.5 -- not a known variable star
02:38:01.93 +58:50:39.9 -- not a known variable star
02:38:48.26 +57:57:35.1 -- not a known variable star
02:40:38.76 +60:07:56.2 -- a known variable star
Found 199 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
299 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 299 (excluding asteroids and hot pixels, 199 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)2461228.75095034 -observatory V36
07:39:57.86 +17:22:37.2 Mercury (4.0mag)
09:58:30.72 +14:01:03.9 Venus (-4.1mag)
04:14:59.03 +21:00:53.0 Mars (1.3mag)
08:13:51.95 +20:20:14.6 Jupiter (-1.8mag)
00:55:28.67 +03:19:05.1 Saturn (0.7mag)
04:06:37.77 +20:43:25.2 Uranus (5.8mag)
00:17:01.74 +00:20:53.5 Neptune (7.8mag)
20:31:11.80 -23:16:38.6 Pluto (14.4mag)
00:26:56.51 +05:27:53.3 Moon (-10.5mag)
-rw-r--r-- 1 apache apache 362 Jul 7 04:24 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461228.75095034:
08:13:56.86 +20:19:56.1 Io (6.1mag)
08:14:01.60 +20:19:40.6 Europa (6.3mag)
08:13:37.35 +20:21:09.1 Ganymede (5.6mag)
08:14:14.23 +20:18:58.9 Callisto (6.8mag)
08:12:32.29 +20:03:10.2 Himalia (15.7mag)
08:13:56.49 +20:19:58.2 Thebe (16.6mag)
08:11:54.81 +20:08:25.1 Elara (17.6mag)
08:17:18.09 +20:16:04.8 Pasiphae (17.8mag)
08:19:00.24 +20:24:54.0 Carme (19.0mag)
00:55:19.51 +03:19:28.8 Titan (8.5mag)
00:55:30.71 +03:18:51.5 Rhea (9.8mag)
00:55:02.69 +03:18:50.9 Iapetus (11.2mag)
00:55:44.18 +03:18:56.7 Hyperion (14.5mag)
00:55:33.54 +03:16:46.1 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jul 7 04:24 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461228.75095034:
17:42:54.23 -33:37:16.0 JWST
13:49:46.20 +56:47:02.8 Chandra
09:07:55.64 -51:44:42.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jul 7 04:24 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461228.75095034 -observatory V36
02:31:48.62 +14:03:01.5 17.9mag P/1996 R2 (Lagerkvist)
18:20:23.19 -34:15:55.1 13.7mag P/2010 H2 (Vales)
06:22:33.72 -68:05:47.1 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:59:42.87 +32:23:43.0 17.6mag C/2017 K2 (PANSTARRS)
17:04:02.05 +16:03:25.5 18.0mag C/2021 G2 (ATLAS)
01:28:51.00 +01:29:33.8 15.3mag P/2021 N1 (ZTF)
23:01:18.90 +32:16:44.3 17.2mag C/2022 E2 (ATLAS)
06:08:49.86 +26:57:02.8 16.6mag C/2022 N2 (PANSTARRS)
09:52:50.25 +29:55:05.6 16.8mag C/2022 QE78 (ATLAS)
09:07:44.98 +04:56:03.7 17.8mag C/2022 R6 (PANSTARRS)
18:09:08.46 +21:24:05.7 17.9mag C/2023 A3 (Tsuchinshan-ATLAS)
15:11:57.56 -11:19:17.7 17.7mag P/2023 B1 (PANSTARRS)
21:52:49.74 +67:37:13.5 17.8mag C/2023 H5 (Lemmon)
16:37:12.85 -09:45:04.4 13.9mag C/2023 R1 (PANSTARRS)
07:55:20.61 +65:32:46.7 17.9mag C/2024 A1 (ATLAS)
07:28:42.24 +29:50:24.9 14.5mag C/2024 E1 (Wierzchos)
15:17:54.00 +15:14:08.7 17.5mag C/2024 G6 (ATLAS)
19:45:10.09 +38:45:22.5 13.8mag C/2024 J3 (ATLAS)
21:50:38.81 +45:31:17.9 17.9mag C/2024 R4 (PANSTARRS)
04:46:41.22 -13:56:43.9 15.8mag C/2024 T5 (ATLAS)
06:31:58.08 +29:35:10.7 18.0mag C/2025 J1 (Borisov)
07:12:05.48 -12:37:39.5 16.3mag C/2025 R3 (PANSTARRS)
09:52:33.60 +22:33:49.4 17.7mag C/2025 V2 (Rankin)
12:43:39.19 +04:03:45.9 17.1mag C/2025 Y1 (ATLAS)
17:00:57.00 +79:01:03.3 17.4mag C/2026 A2 (Bok)
02:42:49.25 +45:05:59.1 16.6mag C/2026 B2 (Sun-Gao)
11:23:36.15 +03:57:58.3 16.9mag A/2026 E1
21:14:04.61 -14:01:56.2 7.4mag 10P/Tempel
11:12:02.61 -01:45:37.6 16.1mag 29P/Schwassmann-Wachmann
03:55:39.66 +29:12:37.0 17.8mag 47P/Ashbrook-Jackson
10:01:34.78 +14:59:40.5 17.0mag 63P/Wild
00:46:54.35 -05:08:29.7 15.6mag 65P/Gunn
08:17:12.38 +34:20:33.9 17.8mag 76P/West-Kohoutek-Ikemura
04:19:52.35 +19:59:59.4 13.7mag 78P/Gehrels
02:17:10.20 +10:09:46.6 16.2mag 88P/Howell
06:26:11.76 +30:41:31.8 15.6mag 93P/Lovas
04:10:59.59 +30:57:38.9 16.9mag 114P/Wiseman-Skiff
08:01:06.21 +31:01:56.0 15.3mag 123P/West-Hartley
10:42:22.38 +02:27:15.9 16.8mag 124P/Mrkos
04:46:43.13 +20:42:54.7 16.3mag 128P/Shoemaker-Holt
05:30:21.83 +19:43:35.9 17.8mag 131P/Mueller
00:00:36.26 +02:48:11.6 18.0mag 139P/Vaisala-Oterma
07:01:48.38 +17:40:21.2 15.1mag 141P-D/Machholz
03:15:26.06 -21:22:36.7 15.6mag 161P/Hartley-IRAS
05:21:54.90 +33:14:09.7 15.3mag 162P/SidingSpring
19:11:27.55 +13:17:39.5 15.0mag 169P/NEAT
01:33:30.86 +07:13:34.4 17.7mag 220P/McNaught
16:36:33.74 -08:16:41.2 16.9mag 235P/LINEAR
08:38:41.92 +33:34:36.0 17.9mag 240P/NEAT
20:43:14.04 -48:51:08.3 17.8mag 259P/Garradd
01:50:39.80 +10:38:33.2 15.7mag 260P/McNaught
05:27:51.23 +36:34:06.4 17.4mag 295P/LINEAR
15:06:52.19 +06:19:26.4 17.6mag 391P/Kowalski
08:31:49.83 +19:47:59.0 17.9mag 450P/LONEOS
07:46:52.11 +39:28:17.1 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jul 7 04:24 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.80 AT2026lxf 2026-05-8.34 13.72
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
16:41:15.63 +39:17:14.70 2026-06-26.38 16.07
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
16:41:15.63 +39:17:14.70 2026-06-26.38 16.07
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
-rw-r--r-- 1 apache apache 5.6K Jul 7 04:24 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
-rw-r--r-- 1 apache apache 189K Jul 7 04:24 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
20:43:31.883 -06:33:13.40 AT 2026rme 2026-06-22.44 21.69
09:40:14.549 -04:56:19.06 AT 2026rmd 2026-02-14.41 21.59
13:59:57.150 -09:03:11.62 AT 2026rmc 2026-02-17.61 20.73
12:25:30.012 -26:12:13.68 AT 2026rmb 2026-01-27.58 21.09
03:21:09.438 +39:25:53.03 AT 2026rma 2026-01-13.29 20.19
13:07:11.418 +13:39:38.85 AT 2026rlz 2026-02-25.47 20.51
03:01:07.569 -26:13:29.83 AT 2026rly 2026-01-09.24 20.54
17:01:46.968 -17:03:38.47 AT 2026rlx 2026-07-04.18 18.537
15:04:30.380 -39:18:48.60 AT 2026rlw 2026-07-04.31 18.9
21:26:04.454 -52:53:31.58 AT 2026rlv 2026-07-04.01 18.538
09:44:11.615 +04:40:29.15 AT 2026rlu 2026-04-19.27 20.88
12:57:25.723 -07:44:47.85 AT 2026rlt 2026-04-22.35 20.53
11:52:32.131 -13:45:09.94 AT 2026rls 2026-04-22.31 21.02
16:41:34.520 +44:47:03.76 AT 2026rlr 2026-04-23.49 21.03
11:22:02.700 -24:23:51.28 AT 2026rlq 2026-05-07.27 20.73
13:17:29.523 +09:10:51.61 AT 2026rlp 2026-05-21.26 20.85
20:21:54.334 -21:13:51.37 AT 2026rlo 2026-05-20.57 19.91
20:13:59.295 -23:24:43.54 AT 2026rln 2026-05-20.56 20.51
20:30:30.579 -12:41:46.85 AT 2026rlm 2026-05-21.56 19.73
20:43:01.499 -03:15:22.31 AT 2026rll 2026-05-24.58 20.5
-rw-r--r-- 1 apache apache 29K Jul 7 04:24 tns_transients_list.txt
