This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM
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 05 25.3690 2461185.8690 8.83 01:56:38.06 +59:15:33.8
131.18810 -2.56326 galactic Cas Second-epoch detections are separated by 0.3" and 2.7 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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.06 +59:15:33.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.06 +59:15:33.8: 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 05 25.3690* 01 56 38.06 +59 15 33.8 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
X Cas,2461185.8690,8.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
X Cas 20260525.3690 8.83CV 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 05 25.3690 2461185.8690 11.43 01:37:05.49 +62:54:32.1
128.10255 0.49640 galactic Cas Second-epoch detections are separated by 1.3" and 2.9 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 | 01:37:05.49 +62:54:32.1 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:05.49 +62:54:32.1: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:05.49 +62:54:32.1: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 05 25.3690* 01 37 05.49 +62 54 32.1 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,2461185.8690,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.43CV 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 05 25.3690 2461185.8690 11.53 01:11:20.02 +61:17:54.5
125.31912 -1.48102 galactic Cas Second-epoch detections are separated by 3.4" and 2.7 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 | 01:11:20.02 +61:17:54.5 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.029 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:20.02 +61:17:54.5: 13.07 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:20.02 +61:17:54.5: 14.08 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 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 05 25.3690* 01 11 20.02 +61 17 54.5 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.37 01:36:18.66 +64:32:20.3
127.73266 2.08630 galactic Cas Second-epoch detections are separated by 3.9" and 2.0 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 | 01:36:18.66 +64:32:20.3 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.037 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:18.66 +64:32:20.3: 11.70 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:18.66 +64:32:20.3: 14.55 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.04 +/- 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 05 25.3690* 01 36 18.66 +64 32 20.3 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,2461185.8690,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.29 01:41:22.16 +58:11:36.2
129.48971 -4.04119 galactic Cas Second-epoch detections are separated by 3.2" and 2.8 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 J025.3435+58.1901 | 01:41:22.16 +58:11:36.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.012+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:41:22.16 +58:11:36.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:41:22.16 +58:11:36.2: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 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 05 25.3690* 01 41 22.16 +58 11 36.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.3435+58.1901,2461185.8690,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.3435+58.1901 20260525.3690 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.32 01:12:00.87 +64:42:19.2
125.12870 1.92139 galactic Cas Second-epoch detections are separated by 2.2" and 3.1 pix
The object was found in VSX 2" ZTF J011201.03+644221.2
Type: RS
# Max. Min./Amp. JD0 Period
14.762 g Y 0.263 g 2458343.85900 3.018403700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:00.87 +64:42:19.2: 11.87 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:00.87 +64:42:19.2: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 05 25.3690* 01 12 00.87 +64 42 19.2 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 J011201.03+644221.2,2461185.8690,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011201.03+644221.2 20260525.3690 11.32CV 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 05 25.3690 2461185.8690 11.35 01:34:57.74 +61:00:14.2
128.18385 -1.42320 galactic Cas Second-epoch detections are separated by 2.1" and 2.5 pix
The object was found in VSX 9" Gaia DR3 509967443017642624
Type: RS
# Max. Min./Amp. JD0 Period
17.430 G 17.560 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:57.74 +61:00:14.2: 12.41 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:57.74 +61:00:14.2: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 05 25.3690* 01 34 57.74 +61 00 14.2 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
Gaia DR3 509967443017642624,2461185.8690,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509967443017642624 20260525.3690 11.35CV 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 05 25.3690 2461185.8690 11.16 01:17:47.95 +57:25:42.1
126.48928 -5.26120 galactic Cas Second-epoch detections are separated by 2.2" and 3.2 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 J019.4502+57.4284 | 01:17:47.95 +57:25:42.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.500+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:47.95 +57:25:42.1: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:47.95 +57:25:42.1: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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 05 25.3690* 01 17 47.95 +57 25 42.1 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
ATO J019.4502+57.4284,2461185.8690,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.4502+57.4284 20260525.3690 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.16 01:59:58.42 +60:14:10.3
131.34455 -1.51133 galactic Cas Second-epoch detections are separated by 4.0" and 2.2 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 | 01:59:58.42 +60:14:10.3 (user input) | T | P | (position from user input) J-Ks=0.911+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:58.42 +60:14:10.3: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:58.42 +60:14:10.3: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 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 05 25.3690* 01 59 58.42 +60 14 10.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.13 01:27:41.37 +59:04:45.6
127.58310 -3.46465 galactic Cas Second-epoch detections are separated by 0.2" and 3.2 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 | 01:27:41.37 +59:04:45.6 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:41.37 +59:04:45.6: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:41.37 +59:04:45.6: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 05 25.3690* 01 27 41.37 +59 04 45.6 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,2461185.8690,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.33 01:11:16.57 +58:55:54.2
125.49476 -3.84127 galactic Cas Second-epoch detections are separated by 2.1" and 3.1 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 J017.8423+58.9300 | 01:11:16.57 +58:55:54.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.465+/-0.043 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:16.57 +58:55:54.2: 12.07 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:16.57 +58:55:54.2: 14.06 +/- 0.06 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 05 25.3690* 01 11 16.57 +58 55 54.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.8423+58.9300,2461185.8690,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.8423+58.9300 20260525.3690 11.33CV 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 05 25.3690 2461185.8690 11.32 01:07:01.83 +59:46:18.7
124.89605 -3.04041 galactic Cas Second-epoch detections are separated by 3.4" and 2.7 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 | 01:07:01.83 +59:46:18.7 (user input) | T | P | (position from user input) J-Ks=0.500+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:01.83 +59:46:18.7: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:01.83 +59:46:18.7: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 05 25.3690* 01 07 01.83 +59 46 18.7 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.32CV 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 05 25.3690 2461185.8690 11.33 01:06:15.91 +57:53:23.8
124.90858 -4.92489 galactic Cas Second-epoch detections are separated by 1.1" and 3.5 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 J016.5720+57.8855 | 01:06:15.91 +57:53:23.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.781+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:15.91 +57:53:23.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:15.91 +57:53:23.8: 14.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 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 05 25.3690* 01 06 15.91 +57 53 23.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J016.5720+57.8855,2461185.8690,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J016.5720+57.8855 20260525.3690 11.33CV 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 05 25.3690 2461185.8690 10.99 01:25:45.62 +59:01:19.9
127.34476 -3.55516 galactic Cas Second-epoch detections are separated by 0.8" and 3.3 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 | 01:25:45.62 +59:01:19.9 (user input) | T | P | (position from user input) J-Ks=0.769+/- (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:45.62 +59:01:19.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:45.62 +59:01:19.9: 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 05 25.3690* 01 25 45.62 +59 01 19.9 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,2461185.8690,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 11.04 01:10:04.96 +57:48:01.6
125.42317 -4.98109 galactic Cas Second-epoch detections are separated by 3.0" and 3.4 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 | 01:10:04.96 +57:48:01.6 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:04.96 +57:48:01.6: 12.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:04.96 +57:48:01.6: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.82 +/- 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 05 25.3690* 01 10 04.96 +57 48 01.6 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,2461185.8690,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 11.17 01:37:01.65 +62:19:20.0
128.19857 -0.08243 galactic Cas Second-epoch detections are separated by 2.1" and 2.6 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 | 01:37:01.65 +62:19:20.0 (user input) | T | P | (position from user input) J-Ks=0.825+/-0.036 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:01.65 +62:19:20.0: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:01.65 +62:19:20.0: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 05 25.3690* 01 37 01.65 +62 19 20.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.17CV 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 05 25.3690 2461185.8690 11.23 01:04:37.03 +62:52:11.1
124.43375 0.03644 galactic Cas Second-epoch detections are separated by 1.4" and 3.0 pix
The object was not found in VSX
The object was found in ASASSN-V18" ASASSN-V J010437.17+625229.1
Type: ROT:
MeanMag 13.26 m Amp. 0.06 m Period d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:04:37.03 +62:52:11.1: 11.42 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:37.03 +62:52:11.1: 13.65 +/- 0.04 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 05 25.3690* 01 04 37.03 +62 52 11.1 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
VARIABLE_NAME,2461185.8690,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260525.3690 11.23CV 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 05 25.3690 2461185.8690 11.10 01:12:09.68 +58:47:53.2
125.61965 -3.96545 galactic Cas Second-epoch detections are separated by 1.1" and 3.4 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 | 01:12:09.68 +58:47:53.2 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:09.68 +58:47:53.2: 13.29 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:09.68 +58:47:53.2: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 05 25.3690* 01 12 09.68 +58 47 53.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.10CV 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 05 25.3690 2461185.8690 11.11 01:32:46.75 +60:59:11.0
127.92557 -1.48390 galactic Cas Second-epoch detections are separated by 1.4" and 2.7 pix
The object was found in VSX 2" Gaia DR3 509888213771256832
Type: ROT
# Max. Min./Amp. JD0 Period
16.910 G 17.020 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:46.75 +60:59:11.0: 12.15 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:46.75 +60:59:11.0: 13.95 +/- 0.06 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 05 25.3690* 01 32 46.75 +60 59 11.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509888213771256832,2461185.8690,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509888213771256832 20260525.3690 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.13 01:08:39.13 +60:32:39.6
125.04833 -2.25666 galactic Cas Second-epoch detections are separated by 0.9" and 3.1 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 | 01:08:39.13 +60:32:39.6 (user input) | T | P | (position from user input) J-Ks=0.751+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:39.13 +60:32:39.6: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:39.13 +60:32:39.6: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 05 25.3690* 01 08 39.13 +60 32 39.6 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,2461185.8690,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.06 01:36:48.85 +62:28:28.5
128.14750 0.06323 galactic Cas Second-epoch detections are separated by 2.6" and 3.1 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 | 01:36:48.85 +62:28:28.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:48.85 +62:28:28.5: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:48.85 +62:28:28.5: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 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 05 25.3690* 01 36 48.85 +62 28 28.5 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,2461185.8690,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.06CV 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 05 25.3690 2461185.8690 11.09 01:26:05.58 +59:01:14.6
127.38746 -3.55090 galactic Cas Second-epoch detections are separated by 1.7" and 3.0 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 J021.5231+59.0209 | 01:26:05.58 +59:01:14.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.314+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:05.58 +59:01:14.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:05.58 +59:01:14.6: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 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 05 25.3690* 01 26 05.58 +59 01 14.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.5231+59.0209,2461185.8690,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.5231+59.0209 20260525.3690 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 05 25.3690 2461185.8690 11.15 01:39:59.26 +60:24:41.5
128.89428 -1.89697 galactic Cas Second-epoch detections are separated by 1.6" and 2.9 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 | 01:39:59.26 +60:24:41.5 (user input) | T | P | (position from user input) J-Ks=0.197+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:59.26 +60:24:41.5: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:59.26 +60:24:41.5: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 05 25.3690* 01 39 59.26 +60 24 41.5 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,2461185.8690,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.15CV 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 05 25.3690 2461185.8690 11.02 01:07:39.11 +59:59:17.8
124.96056 -2.81959 galactic Cas Second-epoch detections are separated by 1.1" and 3.2 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 | 01:07:39.11 +59:59:17.8 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.11 +59:59:17.8: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.11 +59:59:17.8: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 05 25.3690* 01 07 39.11 +59 59 17.8 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,2461185.8690,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.02CV 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 05 25.3690 2461185.8690 11.01 01:43:07.95 +58:54:09.0
129.57635 -3.30075 galactic Cas Second-epoch detections are separated by 3.4" and 2.8 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 J025.7736+58.9016 | 01:43:07.95 +58:54:09.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.275+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:07.95 +58:54:09.0: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:07.95 +58:54:09.0: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 05 25.3690* 01 43 07.95 +58 54 09.0 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
ATO J025.7736+58.9016,2461185.8690,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.7736+58.9016 20260525.3690 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 05 25.3690 2461185.8690 10.87 02:00:06.49 +59:00:32.6
131.68347 -2.69093 galactic Cas Second-epoch detections are separated by 1.8" and 2.6 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 507781618204489856 | 02:00:05.90 +59:00:52.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.381+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:06.49 +59:00:32.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:06.49 +59:00:32.6: 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 05 25.3690* 02 00 06.49 +59 00 32.6 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 507781618204489856,2461185.8690,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507781618204489856 20260525.3690 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 05 25.3690 2461185.8690 11.07 01:25:27.57 +59:27:13.6
127.24931 -3.13248 galactic Cas Second-epoch detections are separated by 4.3" and 2.9 pix
The object was found in VSX 6" Gaia DR3 510073344036983552
Type: ROT
# Max. Min./Amp. JD0 Period
14.460 G 14.520 G 1.820050000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:27.57 +59:27:13.6: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:27.57 +59:27:13.6: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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 05 25.3690* 01 25 27.57 +59 27 13.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510073344036983552,2461185.8690,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510073344036983552 20260525.3690 11.07CV 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 05 25.3690 2461185.8690 10.88 01:12:59.67 +57:34:05.9
125.83090 -5.18206 galactic Cas Second-epoch detections are separated by 1.8" and 3.6 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 | 01:12:59.67 +57:34:05.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:59.67 +57:34:05.9: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:59.67 +57:34:05.9: 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 05 25.3690* 01 12 59.67 +57 34 05.9 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,2461185.8690,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 11.01 01:25:00.93 +62:50:50.8
126.75196 0.22501 galactic Cas Second-epoch detections are separated by 2.3" and 2.4 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 | 01:25:00.93 +62:50:50.8 (user input) | T | P | (position from user input) J-Ks=0.981+/-0.026 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:00.93 +62:50:50.8: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:00.93 +62:50:50.8: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 05 25.3690* 01 25 00.93 +62 50 50.8 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,2461185.8690,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 11.07 01:26:37.96 +60:38:03.7
127.23621 -1.94292 galactic Cas Second-epoch detections are separated by 2.9" and 2.7 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 | 01:26:37.96 +60:38:03.7 (user input) | T | P | (position from user input) J-Ks=0.456+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:37.96 +60:38:03.7: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:37.96 +60:38:03.7: 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 05 25.3690* 01 26 37.96 +60 38 03.7 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,2461185.8690,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.07CV 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 05 25.3690 2461185.8690 11.13 02:20:45.34 +63:43:07.2
132.62621 2.54077 galactic Cas Second-epoch detections are separated by 4.5" and 1.8 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 | 02:20:45.34 +63:43:07.2 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:45.34 +63:43:07.2: 13.39 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:45.34 +63:43:07.2: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.82 +/- 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 05 25.3690* 02 20 45.34 +63 43 07.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 10.95 01:33:08.64 +61:46:15.7
127.84283 -0.70241 galactic Cas Second-epoch detections are separated by 3.8" and 2.3 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 | 01:33:08.64 +61:46:15.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:08.64 +61:46:15.7: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:08.64 +61:46:15.7: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 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 05 25.3690* 01 33 08.64 +61 46 15.7 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,2461185.8690,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.15 01:10:43.69 +60:59:20.5
125.26978 -1.79513 galactic Cas Second-epoch detections are separated by 4.2" and 2.7 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 | 01:10:43.69 +60:59:20.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:43.69 +60:59:20.5: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:43.69 +60:59:20.5: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 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 05 25.3690* 01 10 43.69 +60 59 20.5 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,2461185.8690,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.15CV 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 05 25.3690 2461185.8690 10.95 01:13:40.87 +60:51:24.9
125.63823 -1.89790 galactic Cas Second-epoch detections are separated by 2.5" and 2.7 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 | 01:13:40.87 +60:51:24.9 (user input) | T | P | (position from user input) J-Ks=1.576+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:40.87 +60:51:24.9: 12.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:40.87 +60:51:24.9: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 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 05 25.3690* 01 13 40.87 +60 51 24.9 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,2461185.8690,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.02 01:24:55.02 +59:41:45.6
127.14941 -2.90132 galactic Cas Second-epoch detections are separated by 1.1" and 3.1 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 | 01:24:55.02 +59:41:45.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:55.02 +59:41:45.6: 12.77 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:55.02 +59:41:45.6: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 05 25.3690* 01 24 55.02 +59 41 45.6 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,2461185.8690,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.02CV 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 05 25.3690 2461185.8690 10.93 01:08:15.57 +61:15:06.2
124.95390 -1.55397 galactic Cas Second-epoch detections are separated by 2.4" and 2.8 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 | 01:08:15.57 +61:15:06.2 (user input) | T | P | (position from user input) J-Ks=0.814+/-0.026 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:15.57 +61:15:06.2: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:15.57 +61:15:06.2: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 05 25.3690* 01 08 15.57 +61 15 06.2 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,2461185.8690,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 10.84 01:13:27.21 +59:57:16.6
125.68775 -2.79928 galactic Cas Second-epoch detections are separated by 1.8" and 3.0 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 | 01:13:27.21 +59:57:16.6 (user input) | T | P | (position from user input) J-Ks=0.257+/-0.049 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:27.21 +59:57:16.6: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:27.21 +59:57:16.6: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 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 05 25.3690* 01 13 27.21 +59 57 16.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 10.79 01:34:39.57 +59:40:47.6
128.36887 -2.73482 galactic Cas Second-epoch detections are separated by 1.2" and 3.0 pix
The object was found in VSX20" Gaia DR3 509378860698091520
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.120 G 12.150 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:39.57 +59:40:47.6: 12.86 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:39.57 +59:40:47.6: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 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 05 25.3690* 01 34 39.57 +59 40 47.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509378860698091520,2461185.8690,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509378860698091520 20260525.3690 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 05 25.3690 2461185.8690 10.88 01:24:49.24 +59:47:14.7
127.12550 -2.81224 galactic Cas Second-epoch detections are separated by 1.8" and 2.9 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 510095677857790080 | 01:24:49.88 +59:46:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1960IzKry..24..160B [B60] +59 160 J-Ks=0.149+/-0.051 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:49.24 +59:47:14.7: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:49.24 +59:47:14.7: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 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 05 25.3690* 01 24 49.24 +59 47 14.7 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 510095677857790080,2461185.8690,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510095677857790080 20260525.3690 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 05 25.3690 2461185.8690 10.84 01:08:59.39 +60:47:21.1
125.07308 -2.00956 galactic Cas Second-epoch detections are separated by 4.0" and 2.8 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 522440066710315904 | 01:08:58.80 +60:47:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.504+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:59.39 +60:47:21.1: 13.11 +/- 0.36 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:59.39 +60:47:21.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 05 25.3690* 01 08 59.39 +60 47 21.1 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 522440066710315904,2461185.8690,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522440066710315904 20260525.3690 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 05 25.3690 2461185.8690 10.87 01:11:44.66 +61:13:56.5
125.37351 -1.54308 galactic Cas Second-epoch detections are separated by 0.5" and 3.1 pix
The object was found in VSX 1" 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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:44.66 +61:13:56.5: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:44.66 +61:13:56.5: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 05 25.3690* 01 11 44.66 +61 13 56.5 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
ZTF J011144.73+611356.9,2461185.8690,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011144.73+611356.9 20260525.3690 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 05 25.3690 2461185.8690 10.65 01:07:31.77 +61:28:27.5
124.85237 -1.33743 galactic Cas Second-epoch detections are separated by 3.3" and 2.7 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 | 01:07:31.77 +61:28:27.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:31.77 +61:28:27.5: 12.79 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:31.77 +61:28:27.5: 13.25 +/- 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 05 25.3690* 01 07 31.77 +61 28 27.5 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
target,2461185.8690,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 10.74 01:26:36.35 +59:41:33.3
127.36129 -2.87638 galactic Cas Second-epoch detections are separated by 6.4" and 3.2 pix
The object was found in VSX 4" Gaia DR3 510083239641443712
Type: ROT
# Max. Min./Amp. JD0 Period
13.540 G 13.590 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:36.35 +59:41:33.3: 12.85 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:36.35 +59:41:33.3: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 05 25.3690* 01 26 36.35 +59 41 33.3 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
Gaia DR3 510083239641443712,2461185.8690,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510083239641443712 20260525.3690 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 05 25.3690 2461185.8690 10.63 01:20:45.02 +57:55:08.6
126.82967 -4.73069 galactic Cas Second-epoch detections are separated by 0.7" and 3.5 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 413797116609704704 | 01:20:41.29 +57:55:17.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.023+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:45.02 +57:55:08.6: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:45.02 +57:55:08.6: 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 05 25.3690* 01 20 45.02 +57 55 08.6 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 413797116609704704,2461185.8690,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413797116609704704 20260525.3690 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 05 25.3690 2461185.8690 10.48 01:56:43.74 +58:07:02.6
131.48633 -3.66582 galactic Cas Second-epoch detections are separated by 3.5" and 2.5 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 | 01:56:43.74 +58:07:02.6 (user input) | T | P | (position from user input) J-Ks=0.270+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:43.74 +58:07:02.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:43.74 +58:07:02.6: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 05 25.3690* 01 56 43.74 +58 07 02.6 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,2461185.8690,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 10.56 01:19:08.61 +60:33:57.4
126.33174 -2.12279 galactic Cas Second-epoch detections are separated by 3.0" and 2.7 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 510378080556092032 | 01:19:06.00 +60:34:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:08.61 +60:33:57.4: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:08.61 +60:33:57.4: 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 05 25.3690* 01 19 08.61 +60 33 57.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510378080556092032,2461185.8690,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510378080556092032 20260525.3690 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 05 25.3690 2461185.8690 10.53 01:49:15.81 +59:14:38.1
130.27534 -2.80088 galactic Cas Second-epoch detections are separated by 0.8" and 2.9 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 506536352570768768 | 01:49:14.31 +59:14:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.811+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:15.81 +59:14:38.1: 13.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:15.81 +59:14:38.1: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 05 25.3690* 01 49 15.81 +59 14 38.1 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 506536352570768768,2461185.8690,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506536352570768768 20260525.3690 10.53CV 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 05 25.3690 2461185.8690 10.48 01:22:28.28 +61:07:37.1
126.67072 -1.51929 galactic Cas Second-epoch detections are separated by 1.2" and 2.8 pix
The object was found in VSX22" Gaia DR3 510501328936368640
Type: RS
# Max. Min./Amp. JD0 Period
13.970 G 14.040 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:28.28 +61:07:37.1: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:28.28 +61:07:37.1: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 05 25.3690* 01 22 28.28 +61 07 37.1 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 510501328936368640,2461185.8690,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510501328936368640 20260525.3690 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 05 25.3690 2461185.8690 10.48 01:25:51.85 +61:17:11.7
127.05586 -1.30921 galactic Cas Second-epoch detections are separated by 1.2" and 2.8 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 510682782716801920 | 01:25:53.57 +61:16:58.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.356+/-0.029 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:51.85 +61:17:11.7: 11.63 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:51.85 +61:17:11.7: 13.06 +/- 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 05 25.3690* 01 25 51.85 +61 17 11.7 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
Gaia DR3 510682782716801920,2461185.8690,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510682782716801920 20260525.3690 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 05 25.3690 2461185.8690 10.40 01:30:10.15 +59:36:19.1
127.81986 -2.89836 galactic Cas Second-epoch detections are separated by 0.2" and 3.1 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 | 01:30:10.15 +59:36:19.1 (user input) | T | P | (position from user input) J-Ks=0.144+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:10.15 +59:36:19.1: 11.58 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:10.15 +59:36:19.1: 13.10 +/- 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 05 25.3690* 01 30 10.15 +59 36 19.1 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,2461185.8690,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 10.38 01:31:23.03 +59:33:42.0
127.97866 -2.91809 galactic Cas Second-epoch detections are separated by 0.5" and 3.1 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 J022.8294+59.5638 | 01:31:23.03 +59:33:42.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.833+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:23.03 +59:33:42.0: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:23.03 +59:33:42.0: 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 05 25.3690* 01 31 23.03 +59 33 42.0 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
ATO J022.8294+59.5638,2461185.8690,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.8294+59.5638 20260525.3690 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 05 25.3690 2461185.8690 10.40 01:31:45.26 +59:35:57.1
128.01921 -2.87374 galactic Cas Second-epoch detections are separated by 1.7" and 2.8 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 | 01:31:45.26 +59:35:57.1 (user input) | T | P | (position from user input) J-Ks=0.145+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:45.26 +59:35:57.1: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:45.26 +59:35:57.1: 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 05 25.3690* 01 31 45.26 +59 35 57.1 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,2461185.8690,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 10.04 01:35:24.95 +60:39:14.8
128.29746 -1.75867 galactic Cas Second-epoch detections are separated by 1.3" and 3.1 pix
The object was found in VSX 6" Gaia DR3 509819081975016960
Type: S
# Max. Min./Amp. JD0 Period
17.140 G 17.450 G O
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:24.95 +60:39:14.8: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:24.95 +60:39:14.8: 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 05 25.3690* 01 35 24.95 +60 39 14.8 10.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 509819081975016960,2461185.8690,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509819081975016960 20260525.3690 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 05 25.3690 2461185.8690 9.99 01:45:34.95 +59:18:09.5
129.80297 -2.84487 galactic Cas Second-epoch detections are separated by 0.3" and 3.0 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 J026.3995+59.3029 | 01:45:34.95 +59:18:09.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:34.95 +59:18:09.5: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:34.95 +59:18:09.5: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 05 25.3690* 01 45 34.95 +59 18 09.5 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
ATO J026.3995+59.3029,2461185.8690,9.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.3995+59.3029 20260525.3690 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 05 25.3690 2461185.8690 9.89 01:25:26.59 +60:57:43.6
127.04845 -1.63755 galactic Cas Second-epoch detections are separated by 1.1" and 2.8 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 510670688089089920 | 01:25:28.22 +60:57:27.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +60 212 J-Ks=0.332+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:26.59 +60:57:43.6: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:26.59 +60:57:43.6: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 05 25.3690* 01 25 26.59 +60 57 43.6 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
Gaia DR3 510670688089089920,2461185.8690,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510670688089089920 20260525.3690 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 05 25.3690 2461185.8690 9.34 01:48:51.09 +59:35:49.5
130.14583 -2.46811 galactic Cas Second-epoch detections are separated by 1.6" and 2.8 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 506595038995541376 | 01:48:49.64 +59:36:01.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.406+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:51.09 +59:35:49.5: 12.64 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:51.09 +59:35:49.5: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 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 05 25.3690* 01 48 51.09 +59 35 49.5 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
Gaia DR3 506595038995541376,2461185.8690,9.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506595038995541376 20260525.3690 9.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 9.31 01:25:56.67 +59:35:11.9
127.29270 -2.99263 galactic Cas Second-epoch detections are separated by 0.7" and 3.1 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 510075336901717632 | 01:25:55.70 +59:34:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +59 169 J-Ks=0.194+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:56.67 +59:35:11.9: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:56.67 +59:35:11.9: 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 05 25.3690* 01 25 56.67 +59 35 11.9 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
Gaia DR3 510075336901717632,2461185.8690,9.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510075336901717632 20260525.3690 9.31CV 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 05 25.3690 2461185.8690 8.93 01:44:58.49 +57:57:47.5
130.00400 -4.17156 galactic Cas Second-epoch detections are separated by 0.1" and 3.2 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 J026.2565+57.9569 | 01:44:59.53 +57:57:33.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.812+/-0.026 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:58.49 +57:57:47.5: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:58.49 +57:57:47.5: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 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 05 25.3690* 01 44 58.49 +57 57 47.5 8.9 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 J026.2565+57.9569,2461185.8690,8.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.2565+57.9569 20260525.3690 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 05 25.3690 2461185.8690 8.14 01:47:13.05 +57:44:18.9
130.34393 -4.32822 galactic Cas Second-epoch detections are separated by 0.7" and 3.1 pix
The object was found in VSX 4" Gaia DR3 505962471920178944
Type: VAR
# Max. Min./Amp. JD0 Period
13.440 G 13.470 G 0.024984900000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:13.05 +57:44:18.9: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:13.05 +57:44:18.9: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.71 +/- 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 05 25.3690* 01 47 13.05 +57 44 18.9 8.1 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 505962471920178944,2461185.8690,8.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505962471920178944 20260525.3690 8.14CV 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 05 25.3690 2461185.8690 7.73 01:35:37.48 +61:16:48.8
128.21584 -1.13738 galactic Cas Second-epoch detections are separated by 0.2" and 2.8 pix
The object was found in VSX 8" Gaia DR3 509978579881384704
Type: E
# Max. Min./Amp. JD0 Period
12.390 G 12.580 G 1.177150000000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:37.48 +61:16:48.8: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:37.48 +61:16:48.8: 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 05 25.3690* 01 35 37.48 +61 16 48.8 7.7 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 509978579881384704,2461185.8690,7.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509978579881384704 20260525.3690 7.73CV 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 05 25.3690 2461185.8690 9.14 01:28:00.44 +61:19:58.1
127.30436 -1.22810 galactic Cas Second-epoch detections are separated by 1.2" and 2.7 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 510703497331624576 | 01:28:01.22 +61:19:29.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0V 1928MeUpp..37....1S BD+60 240 J-Ks=0.169+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:00.44 +61:19:58.1: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:00.44 +61:19:58.1: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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 05 25.3690* 01 28 00.44 +61 19 58.1 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
Gaia DR3 510703497331624576,2461185.8690,9.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510703497331624576 20260525.3690 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 05 25.3690 2461185.8690 9.92 01:23:52.89 +60:48:43.7
126.87929 -1.81071 galactic Cas Second-epoch detections are separated by 0.9" and 2.9 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 510299637275996288 | 01:23:47.99 +60:48:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1956PMcCO..13a....B AG+60 152 J-Ks=0.337+/-0.027 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:23:52.89 +60:48:43.7: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:23:52.89 +60:48:43.7: 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 05 25.3690* 01 23 52.89 +60 48 43.7 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 510299637275996288,2461185.8690,9.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510299637275996288 20260525.3690 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 05 25.3690 2461185.8690 10.30 01:26:15.45 +60:37:28.6
127.19193 -1.95881 galactic Cas Second-epoch detections are separated by 1.0" and 3.0 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 510240779041994240 | 01:26:11.56 +60:37:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.182+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:15.45 +60:37:28.6: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:15.45 +60:37:28.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 05 25.3690* 01 26 15.45 +60 37 28.6 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 510240779041994240,2461185.8690,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510240779041994240 20260525.3690 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 05 25.3690 2461185.8690 10.45 01:31:09.00 +59:34:13.0
127.94803 -2.91415 galactic Cas Second-epoch detections are separated by 0.7" and 3.0 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 J022.7886+59.5702 | 01:31:07.89 +59:33:48.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1955ApJS....2..123F LF 5 +59 28 J-Ks=0.831+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:09.00 +59:34:13.0: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:09.00 +59:34:13.0: 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 05 25.3690* 01 31 09.00 +59 34 13.0 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
ATO J022.7886+59.5702,2461185.8690,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.7886+59.5702 20260525.3690 10.45CV 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 05 25.3690 2461185.8690 10.37 01:29:33.38 +63:19:30.8
127.19462 0.76940 galactic Cas Second-epoch detections are separated by 7.1" and 4.1 pix
The object was found in VSX16" Gaia DR3 512422828587465216
Type: S
# Max. Min./Amp. JD0 Period
14.920 G 15.600 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:33.38 +63:19:30.8: 12.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:33.38 +63:19:30.8: 13.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.21 +/- 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 05 25.3690* 01 29 33.38 +63 19 30.8 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 512422828587465216,2461185.8690,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512422828587465216 20260525.3690 10.37CV 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 05 25.3690 2461185.8690 10.59 01:18:37.02 +58:41:37.3
126.46510 -3.99148 galactic Cas Second-epoch detections are separated by 3.1" and 3.0 pix
The object was found in VSX23" Gaia DR3 413902596701682816
Type: ROT
# Max. Min./Amp. JD0 Period
15.180 G 15.220 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:37.02 +58:41:37.3: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:37.02 +58:41:37.3: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 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 05 25.3690* 01 18 37.02 +58 41 37.3 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
Gaia DR3 413902596701682816,2461185.8690,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413902596701682816 20260525.3690 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 05 25.3690 2461185.8690 10.62 02:00:21.87 +64:56:36.8
130.14941 3.04212 galactic Cas Second-epoch detections are separated by 1.9" and 2.4 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 518139017740687360 | 02:00:16.12 +64:56:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9IV/V 1928MeUpp..37....1S BD+64 275 J-Ks=1.311+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:21.87 +64:56:36.8: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:21.87 +64:56:36.8: 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 05 25.3690* 02 00 21.87 +64 56 36.8 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 518139017740687360,2461185.8690,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518139017740687360 20260525.3690 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 05 25.3690 2461185.8690 10.72 01:07:03.66 +59:18:15.9
124.92832 -3.50676 galactic Cas Second-epoch detections are separated by 2.8" and 3.6 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 | 01:07:03.66 +59:18:15.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:03.66 +59:18:15.9: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:03.66 +59:18:15.9: 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 05 25.3690* 01 07 03.66 +59 18 15.9 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
target,2461185.8690,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 10.69 01:51:09.35 +64:52:46.5
129.21811 2.73921 galactic Cas Second-epoch detections are separated by 4.0" and 1.8 pix
The object was found in VSX 3" Gaia DR3 518229967963921664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.740 G 13.780 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:09.35 +64:52:46.5: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:09.35 +64:52:46.5: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 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 05 25.3690* 01 51 09.35 +64 52 46.5 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
Gaia DR3 518229967963921664,2461185.8690,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 518229967963921664 20260525.3690 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 05 25.3690 2461185.8690 10.71 01:29:21.55 +61:44:13.4
127.40555 -0.80487 galactic Cas Second-epoch detections are separated by 1.7" and 2.6 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 | 01:29:21.55 +61:44:13.4 (user input) | T | P | (position from user input) J-Ks=0.512+/-0.037 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:21.55 +61:44:13.4: 12.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:21.55 +61:44:13.4: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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 05 25.3690* 01 29 21.55 +61 44 13.4 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,2461185.8690,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 10.73 01:36:16.25 +60:12:26.3
128.47809 -2.18078 galactic Cas Second-epoch detections are separated by 1.2" and 3.3 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 509768332640107392 | 01:36:16.56 +60:11:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:16.25 +60:12:26.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:16.25 +60:12:26.3: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 05 25.3690* 01 36 16.25 +60 12 26.3 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
Gaia DR3 509768332640107392,2461185.8690,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509768332640107392 20260525.3690 10.73CV 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 05 25.3690 2461185.8690 10.82 01:34:53.35 +60:45:26.6
128.21649 -1.66775 galactic Cas Second-epoch detections are separated by 2.1" and 2.8 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 | 01:34:53.35 +60:45:26.6 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.054 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:53.35 +60:45:26.6: 12.78 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:53.35 +60:45:26.6: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.57 +/- 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 05 25.3690* 01 34 53.35 +60 45 26.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 10.84 01:29:10.32 +59:39:16.1
127.68777 -2.86839 galactic Cas Second-epoch detections are separated by 1.4" and 3.0 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 J022.3180+59.6407 | 01:29:11.26 +59:38:43.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K0 1960IzKry..24..160B [B60] +59 214 J-Ks=0.903+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:10.32 +59:39:16.1: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:10.32 +59:39:16.1: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 05 25.3690* 01 29 10.32 +59 39 16.1 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
ATO J022.3180+59.6407,2461185.8690,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.3180+59.6407 20260525.3690 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 05 25.3690 2461185.8690 10.95 01:18:48.35 +64:12:22.5
125.90436 1.49257 galactic Cas Second-epoch detections are separated by 1.6" and 2.5 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 | 01:18:48.35 +64:12:22.5 (user input) | T | P | (position from user input) J-Ks=0.908+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:48.35 +64:12:22.5: 11.66 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:48.35 +64:12:22.5: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 05 25.3690* 01 18 48.35 +64 12 22.5 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,2461185.8690,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 10.94 01:38:05.76 +61:04:11.3
128.54606 -1.29233 galactic Cas Second-epoch detections are separated by 4.7" and 2.3 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 | 01:38:05.76 +61:04:11.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:05.76 +61:04:11.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:05.76 +61:04:11.3: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 05 25.3690* 01 38 05.76 +61 04 11.3 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
target,2461185.8690,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 10.94CV 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 05 25.3690 2461185.8690 11.00 01:19:28.60 +59:54:38.2
126.44377 -2.76981 galactic Cas Second-epoch detections are separated by 3.3" and 2.8 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 510323036254643328 | 01:19:24.22 +59:54:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B6 1935BSD...C01....0S BSD 8- 782
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:28.60 +59:54:38.2: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:28.60 +59:54:38.2: 13.92 +/- 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 05 25.3690* 01 19 28.60 +59 54 38.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510323036254643328,2461185.8690,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510323036254643328 20260525.3690 11.00CV 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 05 25.3690 2461185.8690 10.91 02:16:37.80 +64:56:45.6
131.79704 3.55085 galactic Cas Second-epoch detections are separated by 1.5" and 2.1 pix
The object was found in VSX13" Gaia DR3 515428274899734784
Type: ROT
# Max. Min./Amp. JD0 Period
15.360 G 15.390 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:16:37.80 +64:56:45.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:16:37.80 +64:56:45.6: 13.90 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 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 05 25.3690* 02 16 37.80 +64 56 45.6 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 515428274899734784,2461185.8690,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 515428274899734784 20260525.3690 10.91CV 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 05 25.3690 2461185.8690 10.87 01:58:13.79 +60:03:14.7
131.18205 -1.74345 galactic Cas Second-epoch detections are separated by 3.7" and 2.9 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 | 01:58:13.79 +60:03:14.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:13.79 +60:03:14.7: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:13.79 +60:03:14.7: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 05 25.3690* 01 58 13.79 +60 03 14.7 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,2461185.8690,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 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 05 25.3690 2461185.8690 10.94 01:22:11.14 +59:09:02.7
126.87221 -3.48556 galactic Cas Second-epoch detections are separated by 0.7" and 3.2 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 413976852405588480 | 01:22:13.31 +59:08:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1960IzKry..24..160B [B60] +58 184
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:11.14 +59:09:02.7: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:11.14 +59:09:02.7: 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 05 25.3690* 01 22 11.14 +59 09 02.7 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 413976852405588480,2461185.8690,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413976852405588480 20260525.3690 10.94CV 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 05 25.3690 2461185.8690 11.05 01:11:56.65 +58:41:02.0
125.60067 -4.08156 galactic Cas Second-epoch detections are separated by 4.5" and 3.7 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 J017.9933+58.6776 | 01:11:56.65 +58:41:02.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:56.65 +58:41:02.0: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:56.65 +58:41:02.0: 13.87 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 05 25.3690* 01 11 56.65 +58 41 02.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.9933+58.6776,2461185.8690,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.9933+58.6776 20260525.3690 11.05CV 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 05 25.3690 2461185.8690 11.01 01:17:48.33 +58:35:16.1
126.37088 -4.10777 galactic Cas Second-epoch detections are separated by 3.6" and 3.3 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 413895419824765696 | 01:17:45.89 +58:35:00.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:48.33 +58:35:16.1: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:48.33 +58:35:16.1: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 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 05 25.3690* 01 17 48.33 +58 35 16.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 413895419824765696,2461185.8690,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413895419824765696 20260525.3690 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 05 25.3690 2461185.8690 11.00 01:31:48.40 +64:21:55.3
127.28197 1.83510 galactic Cas Second-epoch detections are separated by 1.3" and 2.5 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 | 01:31:48.40 +64:21:55.3 (user input) | T | P | (position from user input) J-Ks=0.974+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.40 +64:21:55.3: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.40 +64:21:55.3: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 05 25.3690* 01 31 48.40 +64 21 55.3 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,2461185.8690,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.00CV 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 05 25.3690 2461185.8690 10.92 02:17:05.29 +64:01:02.3
132.14567 2.68846 galactic Cas Second-epoch detections are separated by 3.1" and 1.7 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 515173119485547392 | 02:17:01.60 +64:01:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.393+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:17:05.29 +64:01:02.3: 12.50 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:17:05.29 +64:01:02.3: 13.55 +/- 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 05 25.3690* 02 17 05.29 +64 01 02.3 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 515173119485547392,2461185.8690,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 515173119485547392 20260525.3690 10.92CV 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 05 25.3690 2461185.8690 11.06 01:14:41.50 +58:46:44.7
125.94866 -3.95639 galactic Cas Second-epoch detections are separated by 1.8" and 3.3 pix
The object was found in VSX24" Gaia DR3 414091266028390144
Type: ROT
# Max. Min./Amp. JD0 Period
18.000 G 18.140 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:41.50 +58:46:44.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:41.50 +58:46:44.7: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 05 25.3690* 01 14 41.50 +58 46 44.7 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
Gaia DR3 414091266028390144,2461185.8690,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 414091266028390144 20260525.3690 11.06CV 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 05 25.3690 2461185.8690 10.88 02:00:32.82 +59:40:05.7
131.56348 -2.04032 galactic Cas Second-epoch detections are separated by 3.0" and 2.5 pix
The object was found in VSX 4" ZTF J020033.07+594008.7
Type: SR
# Max. Min./Amp. JD0 Period
13.621 r Y 0.477 r 2458342.93970 344.838134100000 C
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:00:32.82 +59:40:05.7: 11.54 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:00:32.82 +59:40:05.7: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.91 +/- 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 05 25.3690* 02 00 32.82 +59 40 05.7 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
ZTF J020033.07+594008.7,2461185.8690,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J020033.07+594008.7 20260525.3690 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 05 25.3690 2461185.8690 11.00 01:31:48.47 +64:22:27.8
127.28069 1.84404 galactic Cas Second-epoch detections are separated by 1.0" and 2.5 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 | 01:31:48.47 +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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:48.47 +64:22:27.8: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:48.47 +64:22:27.8: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 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 05 25.3690* 01 31 48.47 +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,2461185.8690,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.00CV 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 05 25.3690 2461185.8690 10.85 02:21:38.50 +65:44:29.5
132.02542 4.47502 galactic Cas Second-epoch detections are separated by 2.6" and 1.8 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 517069845756285184 | 02:21:38.42 +65:45:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.045+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:38.50 +65:44:29.5: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:38.50 +65:44:29.5: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 05 25.3690* 02 21 38.50 +65 44 29.5 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
Gaia DR3 517069845756285184,2461185.8690,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 517069845756285184 20260525.3690 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 05 25.3690 2461185.8690 10.88 02:20:32.64 +62:45:43.0
132.92735 1.63230 galactic Cas Second-epoch detections are separated by 2.0" and 2.1 pix
The object was found in VSX15" ZTF J022034.82+624545.5
Type: SR
# Max. Min./Amp. JD0 Period
14.855 r Y 0.593 r 2458302.30000 111.117252300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:32.64 +62:45:43.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:32.64 +62:45:43.0: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 05 25.3690* 02 20 32.64 +62 45 43.0 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
ZTF J022034.82+624545.5,2461185.8690,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J022034.82+624545.5 20260525.3690 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 05 25.3690 2461185.8690 11.02 02:01:03.52 +64:43:32.9
130.27849 2.85175 galactic Cas Second-epoch detections are separated by 1.4" and 2.2 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 | 02:01:03.52 +64:43:32.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:01:03.52 +64:43:32.9: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:01:03.52 +64:43:32.9: 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 05 25.3690* 02 01 03.52 +64 43 32.9 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,2461185.8690,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.02CV 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 05 25.3690 2461185.8690 11.07 01:44:03.41 +61:54:43.1
129.08317 -0.32972 galactic Cas Second-epoch detections are separated by 2.0" and 3.0 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 511486800591720192 | 01:44:01.89 +61:55:16.8 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B1V 1999A&AS..136..313S Cl* NGC 654 Sto 94 J-Ks=12.609+/- (unrealisitic color!)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:03.41 +61:54:43.1: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:03.41 +61:54:43.1: 13.95 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 05 25.3690* 01 44 03.41 +61 54 43.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511486800591720192,2461185.8690,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511486800591720192 20260525.3690 11.07CV 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 05 25.3690 2461185.8690 11.04 01:13:39.07 +58:10:51.0
125.86585 -4.56432 galactic Cas Second-epoch detections are separated by 1.8" and 3.8 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 J018.4234+58.1762 | 01:13:41.63 +58:10:34.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.593+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:39.07 +58:10:51.0: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:39.07 +58:10:51.0: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 05 25.3690* 01 13 39.07 +58 10 51.0 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
ATO J018.4234+58.1762,2461185.8690,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.4234+58.1762 20260525.3690 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 05 25.3690 2461185.8690 11.00 01:50:39.98 +62:00:55.2
129.81943 -0.06179 galactic Cas Second-epoch detections are separated by 1.2" and 2.6 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 511356332360621440 | 01:50:34.89 +62:00:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1955ApJS....2..123F LF 5 +61 158 J-Ks=1.202+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:39.98 +62:00:55.2: 13.28 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:39.98 +62:00:55.2: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 05 25.3690* 01 50 39.98 +62 00 55.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511356332360621440,2461185.8690,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511356332360621440 20260525.3690 11.00CV 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 05 25.3690 2461185.8690 11.19 01:29:39.14 +63:18:44.3
127.20719 0.75821 galactic Cas Second-epoch detections are separated by 2.6" and 2.5 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 512422794227736704 | 01:29:32.93 +63:18:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8Ib 1987ApJS...64..241S NGC 559 14
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:39.14 +63:18:44.3: 12.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:39.14 +63:18:44.3: 14.09 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.09 +/- 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 05 25.3690* 01 29 39.14 +63 18 44.3 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512422794227736704,2461185.8690,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512422794227736704 20260525.3690 11.19CV 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 05 25.3690 2461185.8690 11.10 01:07:29.45 +63:11:00.7
124.74128 0.36819 galactic Cas Second-epoch detections are separated by 3.6" and 2.9 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 | 01:07:29.45 +63:11:00.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:29.45 +63:11:00.7: 11.40 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:29.45 +63:11:00.7: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.84 +/- 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 05 25.3690* 01 07 29.45 +63 11 00.7 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,2461185.8690,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.10CV 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 05 25.3690 2461185.8690 11.12 01:48:29.48 +60:27:38.2
129.91174 -1.63566 galactic Cas Second-epoch detections are separated by 1.3" and 2.7 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 | 01:48:29.48 +60:27:38.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:29.48 +60:27:38.2: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:29.48 +60:27:38.2: 13.81 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 05 25.3690* 01 48 29.48 +60 27 38.2 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.07 01:25:25.24 +58:19:59.4
127.39237 -4.24397 galactic Cas Second-epoch detections are separated by 3.7" and 3.0 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 J021.3568+58.3360 | 01:25:26.64 +58:19:32.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +58 215 J-Ks=0.486+/-0.036 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:25.24 +58:19:59.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:25.24 +58:19:59.4: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 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 05 25.3690* 01 25 25.24 +58 19 59.4 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J021.3568+58.3360,2461185.8690,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.3568+58.3360 20260525.3690 11.07CV 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 05 25.3690 2461185.8690 11.21 01:59:34.12 +63:37:06.6
130.41403 1.74084 galactic Cas Second-epoch detections are separated by 0.9" and 2.4 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 | 01:59:34.12 +63:37:06.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:34.12 +63:37:06.6: 13.51 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:34.12 +63:37:06.6: 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 05 25.3690* 01 59 34.12 +63 37 06.6 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,2461185.8690,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.18 01:38:11.29 +61:01:59.0
128.56366 -1.32647 galactic Cas Second-epoch detections are separated by 3.9" and 2.3 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 | 01:38:11.29 +61:01:59.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:11.29 +61:01:59.0: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:11.29 +61:01:59.0: 14.11 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.11 +/- 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 05 25.3690* 01 38 11.29 +61 01 59.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.18CV 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 05 25.3690 2461185.8690 11.13 01:31:55.99 +59:26:39.6
128.06588 -3.02315 galactic Cas Second-epoch detections are separated by 3.8" and 2.9 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 J023.0100+59.4551 | 01:31:59.23 +59:26:47.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1955ApJS....2..123F LF 5 +59 42 J-Ks=0.314+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:55.99 +59:26:39.6: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:55.99 +59:26:39.6: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.13 +/- 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 05 25.3690* 01 31 55.99 +59 26 39.6 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.0100+59.4551,2461185.8690,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J023.0100+59.4551 20260525.3690 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.12 02:02:25.68 +64:38:22.6
130.44288 2.80812 galactic Cas Second-epoch detections are separated by 2.8" and 2.0 pix
The object was found in VSX 2" ASASSN-V J020225.96+643822.9
Type: SR
# Max. Min./Amp. JD0 Period
14.090 V 14.200 V 2457555.11300 70.630000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:25.68 +64:38:22.6: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:25.68 +64:38:22.6: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 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 05 25.3690* 02 02 25.68 +64 38 22.6 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
ASASSN-V J020225.96+643822.9,2461185.8690,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J020225.96+643822.9 20260525.3690 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.28 01:45:26.42 +60:36:32.8
129.51333 -1.57073 galactic Cas Second-epoch detections are separated by 3.9" and 2.3 pix
The object was found in VSX 2" ZTF J014526.32+603634.2
Type: RS
# Max. Min./Amp. JD0 Period
14.440 r Y 0.055 r 2458351.88120 3.435017200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:26.42 +60:36:32.8: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:26.42 +60:36:32.8: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.19 +/- 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 05 25.3690* 01 45 26.42 +60 36 32.8 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 J014526.32+603634.2,2461185.8690,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J014526.32+603634.2 20260525.3690 11.28CV 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 05 25.3690 2461185.8690 11.37 01:22:24.00 +61:13:49.6
126.64976 -1.41760 galactic Cas Second-epoch detections are separated by 3.0" and 3.2 pix
The object was found in VSX 2" 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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:24.00 +61:13:49.6: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:24.00 +61:13:49.6: 15.75 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.75 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 25.3690* 01 22 24.00 +61 13 49.6 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
NSVS J0122238+611352,2461185.8690,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0122238+611352 20260525.3690 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.42 01:13:18.74 +63:56:03.6
125.33238 1.16458 galactic Cas Second-epoch detections are separated by 2.9" and 2.8 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 | 01:13:18.74 +63:56:03.6 (user input) | T | P | (position from user input) J-Ks=0.838+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:18.74 +63:56:03.6: 11.57 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:18.74 +63:56:03.6: 14.47 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.83 +/- 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 05 25.3690* 01 13 18.74 +63 56 03.6 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,2461185.8690,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.42CV 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 05 25.3690 2461185.8690 11.44 01:44:29.97 +65:09:24.5
128.47103 2.85727 galactic Cas Second-epoch detections are separated by 2.4" and 2.1 pix
The object was found in VSX 6" Gaia DR3 519045973088246784
Type: ROT
# Max. Min./Amp. JD0 Period
15.090 G 15.140 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:29.97 +65:09:24.5: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:29.97 +65:09:24.5: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 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 05 25.3690* 01 44 29.97 +65 09 24.5 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
Gaia DR3 519045973088246784,2461185.8690,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 519045973088246784 20260525.3690 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 05 25.3690 2461185.8690 11.55 01:24:36.09 +61:08:54.9
126.92319 -1.46590 galactic Cas Second-epoch detections are separated by 3.0" and 2.5 pix
The object was found in VSX 1" Gaia DR3 510685394056841344
Type: ROT
# Max. Min./Amp. JD0 Period
14.210 G 14.240 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:36.09 +61:08:54.9: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:36.09 +61:08:54.9: 14.38 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 25.3690* 01 24 36.09 +61 08 54.9 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510685394056841344,2461185.8690,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510685394056841344 20260525.3690 11.55CV 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 05 25.3690 2461185.8690 11.32 01:30:50.85 +60:06:03.2
127.82915 -2.39560 galactic Cas Second-epoch detections are separated by 1.1" and 3.0 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 | IL Cas | 01:30:46.78 +60:06:02.4 (Gaia DR3) | EA/SD (local) | 3.451726000000 (local) | Gaia3var=VARIABLE SpType: B5 1955ApJS....2..123F LF 5 +59 22
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:50.85 +60:06:03.2: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:50.85 +60:06:03.2: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 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 05 25.3690* 01 30 50.85 +60 06 03.2 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
IL Cas,2461185.8690,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IL Cas 20260525.3690 11.32CV 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 05 25.3690 2461185.8690 11.28 01:13:13.57 +57:53:06.1
125.83502 -4.86385 galactic Cas Second-epoch detections are separated by 2.8" and 3.1 pix
The object was found in VSX24" Gaia DR3 413643769095819136
Type: E
# Max. Min./Amp. JD0 Period
17.840 G 18.210 G 30.570000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:13.57 +57:53:06.1: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:13.57 +57:53:06.1: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 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 05 25.3690* 01 13 13.57 +57 53 06.1 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
Gaia DR3 413643769095819136,2461185.8690,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413643769095819136 20260525.3690 11.28CV 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 05 25.3690 2461185.8690 11.18 02:15:16.83 +59:21:33.6
133.44181 -1.79076 galactic Cas Second-epoch detections are separated by 2.4" and 2.5 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 507242582628346368 | 02:15:20.62 +59:22:07.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.718+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:16.83 +59:21:33.6: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:16.83 +59:21:33.6: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 05 25.3690* 02 15 16.83 +59 21 33.6 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
Gaia DR3 507242582628346368,2461185.8690,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507242582628346368 20260525.3690 11.18CV 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 05 25.3690 2461185.8690 11.38 01:37:59.74 +61:04:02.6
128.53456 -1.29689 galactic Cas Second-epoch detections are separated by 1.3" and 2.7 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 | 01:37:59.74 +61:04:02.6 (user input) | T | P | (position from user input) J-Ks=0.241+/-0.044 (F)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:37:59.74 +61:04:02.6: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:37:59.74 +61:04:02.6: 14.28 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 25.3690* 01 37 59.74 +61 04 02.6 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,2461185.8690,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.38CV 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 05 25.3690 2461185.8690 11.37 01:08:11.52 +62:14:22.7
124.88156 -0.56867 galactic Cas Second-epoch detections are separated by 3.3" and 2.9 pix
The object was found in VSX 2" Gaia DR3 522685876279259136
Type: ROT
# Max. Min./Amp. JD0 Period
14.350 G 14.370 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:11.52 +62:14:22.7: 12.19 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:11.52 +62:14:22.7: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 05 25.3690* 01 08 11.52 +62 14 22.7 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
Gaia DR3 522685876279259136,2461185.8690,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522685876279259136 20260525.3690 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 11.51 01:22:13.56 +59:52:25.2
126.79092 -2.76720 galactic Cas Second-epoch detections are separated by 0.4" and 3.1 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 | 01:22:13.56 +59:52:25.2 (user input) | T | P | (position from user input) J-Ks=1.005+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:13.56 +59:52:25.2: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:13.56 +59:52:25.2: 14.36 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.36 +/- 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 05 25.3690* 01 22 13.56 +59 52 25.2 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.51CV 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 05 25.3690 2461185.8690 11.59 01:21:55.54 +63:45:18.9
126.29499 1.08276 galactic Cas Second-epoch detections are separated by 2.8" and 2.5 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 | 01:21:55.54 +63:45:18.9 (user input) | T | P | (position from user input) J-Ks=1.195+/- (M)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:55.54 +63:45:18.9: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:55.54 +63:45:18.9: 14.28 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 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 05 25.3690* 01 21 55.54 +63 45 18.9 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.59CV 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 05 25.3690 2461185.8690 11.63 01:40:28.47 +60:34:43.8
128.92168 -1.72138 galactic Cas Second-epoch detections are separated by 1.6" and 2.8 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 | 01:40:28.47 +60:34:43.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:28.47 +60:34:43.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:28.47 +60:34:43.8: 14.53 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 25.3690* 01 40 28.47 +60 34 43.8 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461185.8690,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 25.3690 2461185.8690 10.78 01:33:44.53 +60:46:15.0
128.07608 -1.67769 galactic Cas Second-epoch detections are separated by 2.6" and 2.9 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 | 01:33:44.53 +60:46:15.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:44.53 +60:46:15.0: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:44.53 +60:46:15.0: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 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 05 25.3690* 01 33 44.53 +60 46 15.0 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
target,2461185.8690,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260525.3690 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461185.86926525 25.05.2026 08:51:34.518 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 23 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 25695
Objects passed selection criteria: 25553
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 18100.5
Average stars matched: 16570.2 (91.5458 %)
Memory usage VmPeak: 128288 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 04:30:27 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
First image: 2461061.56999090 21.01.2026 01:40:37.214 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461185.86926525 25.05.2026 08:51:34.518 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 336
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 115 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 190245
Objects passed selection criteria: 189733
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 142302
Average stars matched: 129903 (91.2863 %)
Memory usage VmPeak: 2131264 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 04:37:17 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
SExtractor catalog cache: saved Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q2b1x1_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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461185.86871880
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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits'
wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q2b1x1_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-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
Image size: 938.8'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:43:00.007 +61:59:56.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:43:00.007 +61:59:56.83
Angular distance between the image centers 0.0628 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
Image size: 938.7'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 01:42:58.435 +62:00:07.55 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 01:42:58.435 +62:00:07.55
Angular distance between the image centers 0.0606 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 01:43:00.007 +61:59:56.83
Second-epoch second image center 01:42:58.435 +62:00:07.55
Angular distance between the image centers 0.00428 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.QLXLKf4iof
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_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-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.njI9Q9dhpI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_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_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits &> /tmp/tmp.2Wf0ngLpQq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits &> /tmp/tmp.7INy07wyrM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q2b1x1_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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat' -> '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.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.929150
a=0.000000 b=1.000000 c=22.929150
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
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-Q2b1x1_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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.8)
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-Q2b1x1_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-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
2.4 pix fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
14.4 mag. fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
14.3 mag. fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QLXLKf4iof (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q2b1x1_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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3786, passed=31559
Got 31559 stars (including 27744 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
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: 5.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 266 matched stars entering correct_measured_positions(), 9996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
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: 337 matched stars entering correct_measured_positions(), 10041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.38"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.88"
Excluding outliers - 331 stars left (next iteration limit 292)
WCS_QUALITY_DIAG: file=Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits N_match=331 sigma_overall_arcsec=7.729 sigma_q1_arcsec=31.346 sigma_q2_arcsec=12.794 sigma_q3_arcsec=22.422 sigma_q4_arcsec=4.202 n_q1=16 n_q2=97 n_q3=37 n_q4=181 worst_quadrant_to_overall_ratio=4.055
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.njI9Q9dhpI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q2b1x1_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-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3692, passed=31681
Got 31681 stars (including 27947 good ones) from the SExtractor catalog wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat
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(), 29074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29074 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-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits N_match=973 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.346 n_q1=119 n_q2=244 n_q3=303 n_q4=307 worst_quadrant_to_overall_ratio=1.316
The image catalog is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2Wf0ngLpQq (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_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.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_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1296, passed=15982
Got 15982 stars (including 14681 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 15982 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 15644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 15643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 15643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 974 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits N_match=974 sigma_overall_arcsec=0.648 sigma_q1_arcsec=0.553 sigma_q2_arcsec=0.621 sigma_q3_arcsec=0.783 sigma_q4_arcsec=0.769 n_q1=271 n_q2=333 n_q3=214 n_q4=156 worst_quadrant_to_overall_ratio=1.209
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.7INy07wyrM (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_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.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_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
Checking if the catalog wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits.cat corresponding to the image wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
WCS catalog name: wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=10, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1310, passed=15973
Got 15973 stars (including 14656 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 15973 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 15580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 15578 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 15578 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 972 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits N_match=972 sigma_overall_arcsec=0.664 sigma_q1_arcsec=0.631 sigma_q2_arcsec=0.628 sigma_q3_arcsec=0.719 sigma_q4_arcsec=0.761 n_q1=266 n_q2=339 n_q3=207 n_q4=160 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits -region wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits.cat.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-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits sigma_overall=7.729 worst_q_ratio=4.055
ref2=Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits sigma_overall=0.405 worst_q_ratio=1.316
new1=fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits sigma_overall=0.648 worst_q_ratio=1.209
new2=fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits sigma_overall=0.664 worst_q_ratio=1.146
reference average sigma_overall=4.067 worst_q_ratio=2.6855
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018_astrometric_residuals.png (331 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019_astrometric_residuals.png (973 matched stars from wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382_astrometric_residuals.png (974 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383_astrometric_residuals.png (972 matched stars from wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-50-47_20.00sec_5.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cas-03-Q2b1x1_042559_TTUQ2b1x1_42566_W2YlMcsM/wcs_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383.fits'
Preparing the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:13.04 +57:44:19.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:56:38.06 +59:15:33.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:13.04 +57:44:19.4: 10.36 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.36 +/- 0.00
Forced photometry filter REJECTED candidate at 01:47:13.04 +57:44:19.4: ref_mag=10.36 +/- 0.00 new_mean_mag=10.9196 delta=-0.56 (need > 0.90)
Forced photometry on wcs_Cas-03-Q2b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:56:38.06 +59:15:33.8: 9.75 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 01:56:38.06 +59:15:33.8: ref_mag=9.75 +/- 0.00 new_mean_mag=8.8262 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out20109.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 51605_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 51605_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
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Considering the candidate 52697_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 52697_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:19:46.44 +58:12:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55213_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 55213_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:26:40.98 +60:46:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20109_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 20109_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 08339_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 08339_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:38:57.52 +61:08:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247667_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247667_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247671_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247671_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247672_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247672_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247677_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247677_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 247683_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247683_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247685_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247685_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247687_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247687_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:30:06.77 +61:51:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247701_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247701_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247702_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247702_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247705_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247705_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247707_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247707_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247715_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247715_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247721_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247721_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247725_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247725_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247726_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247726_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247727_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247727_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247728_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247728_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247729_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247729_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247731_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247731_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247735_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247735_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247738_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247738_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247741_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247741_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247743_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247743_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247746_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247746_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247747_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247747_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247748_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247748_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:17:40.57 +58:13:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247749_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247749_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247750_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247750_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247752_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247752_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247757_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247757_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247758_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247758_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247759_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247759_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247762_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247762_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 247763_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247763_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247764_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247764_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:13:50.17 +59:40:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247765_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247765_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247766_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247766_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247768_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247768_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247782_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247782_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:39:24.13 +58:23:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247783_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247783_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247784_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247784_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:36:26.71 +64:32:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247786_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247786_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247787_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247787_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247790_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247790_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247794_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247794_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:07:35.01 +57:33:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247796_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247796_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247797_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247797_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247798_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247798_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:33:35.22 +59:56:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247800_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247800_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247801_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247801_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247802_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247802_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247804_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247804_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247805_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247805_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:01:30.61 +65:05:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247806_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247806_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:19:24.10 +58:26:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247808_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247808_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247809_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247809_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247810_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247810_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:07:33.94 +60:52:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247811_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247811_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247812_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247812_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
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Considering the candidate 247814_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247814_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:05:57.29 +63:03:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247817_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247817_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247822_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247822_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247823_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247823_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:15:54.23 +64:24:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247824_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247824_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:40:31.28 +60:31:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247827_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247827_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247828_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247828_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:14:45.23 +60:30:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247832_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247832_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:10:37.47 +57:22:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247834_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247834_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:39:04.22 +61:53:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247835_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247835_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:12:40.97 +61:20:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247837_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247837_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247838_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247838_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:07:08.00 +57:44:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247840_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247840_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247841_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247841_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:55:14.53 +59:32:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247842_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247842_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247843_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247843_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:43:59.24 +61:55:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247846_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247846_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:51:35.69 +57:52:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247848_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247848_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247849_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247849_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247850_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247850_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:19:48.74 +61:38:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247851_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247851_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:23:56.42 +62:06:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247852_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247852_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:22:08.34 +60:22:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247853_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247853_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 247855_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 247855_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:13:07.33 +58:04:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247857_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 247857_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 248927_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 248927_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 251708_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 251708_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:26:41.03 +60:46:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252140_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 252140_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:44:01.78 +61:53:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252184_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 252184_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 252810_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 252810_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:30:55.41 +61:54:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252964_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 252964_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:38:00.48 +57:56:45.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253649_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 253649_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:17:59.13 +57:47:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253838_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 253838_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:19:11.12 +58:20:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254786_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 254786_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:26:46.60 +57:46:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254867_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 254867_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:24:27.30 +58:44:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256228_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 256228_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:18:14.15 +61:44:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256426_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 256426_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:58:16.21 +59:38:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256778_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 256778_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 257487_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 257487_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:46:33.57 +61:16:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257655_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 257655_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:20:11.01 +58:12:09.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 257762_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 257762_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:19:12.42 +65:35:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257791_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 257791_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 258114_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 258114_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:43:53.01 +61:53:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258125_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 258125_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:44:17.71 +61:53:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258314_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 258314_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:44:32.40 +58:45:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258906_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 258906_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:16:08.67 +58:49:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258996_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 258996_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:51:02.54 +64:49:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259146_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 259146_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 259543_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 259543_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:23:56.41 +60:54:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259689_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 259689_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 259692_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 259692_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:20:52.90 +63:53:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260035_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 260035_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:15:59.00 +63:12:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 260069_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 260069_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 260090_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 260090_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
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Considering the candidate 260293_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 260293_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:33:59.39 +58:28:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261009_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261009_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 261112_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261112_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:02:54.94 +64:24:58.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261160_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261160_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:26:35.89 +57:57:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261215_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 261215_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 261290_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261290_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:13:36.04 +57:52:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261340_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261340_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:04:26.77 +65:05:52.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 261466_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261466_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:27:52.51 +62:46:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261502_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261502_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:37:44.63 +64:45:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261567_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261567_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:33:23.23 +57:44:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261683_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261683_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:35:50.43 +61:27:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261725_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261725_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:39:56.85 +60:52:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 261979_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 261979_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:16:05.06 +58:49:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262085_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262085_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:00:36.81 +58:30:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262188_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262188_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:44:27.89 +60:41:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262310_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262310_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:06:23.56 +62:44:02.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 262346_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 262346_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 262603_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262603_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:42:32.94 +63:52:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262636_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262636_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:19:22.27 +58:19:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262651_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262651_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:15:11.68 +60:07:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262691_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262691_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:19:41.39 +62:51:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262735_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262735_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:39:24.71 +63:23:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262826_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 262826_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 262832_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262832_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:11:50.12 +59:02:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262873_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262873_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:21:37.22 +58:54:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262902_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 262902_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:27:02.28 +58:03:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263355_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 263355_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:35:54.19 +60:13:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263380_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 263380_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:44:01.62 +61:52:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263594_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 263594_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:41:50.89 +61:02:06.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263781_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 263781_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:13:30.38 +58:34:24.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263839_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 263839_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 263866_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 263866_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:19:03.80 +63:57:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263877_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 263877_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:54:18.74 +63:38:03.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 263945_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 263945_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:01:15.09 +59:23:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264028_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 264028_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:14:58.53 +60:30:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264223_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 264223_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:10:23.83 +60:01:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264260_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 264260_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264468_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 264468_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:08:33.02 +63:34:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264553_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 264553_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:16:02.09 +58:49:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264570_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 264570_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264668_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 264668_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:08:30.52 +58:24:16.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 264911_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 264911_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264941_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 264941_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:10:31.68 +59:59:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264986_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 264986_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:06:45.34 +59:50:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265013_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 265013_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:38:12.00 +61:01:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265045_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 265045_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:01:37.06 +59:57:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265076_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 265076_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:20:40.56 +60:23:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265133_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 265133_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:43:12.77 +64:00:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265440_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 265440_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 265662_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 265662_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:38:07.56 +61:01:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265708_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 265708_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:58:40.06 +59:15:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265864_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 265864_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:11:41.14 +58:17:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 265877_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 265877_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 266172_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266172_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:16:36.24 +64:57:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266174_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266174_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:42:54.95 +64:01:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266213_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 266213_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 266226_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266226_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:58:04.08 +57:58:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266463_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266463_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:33:24.69 +58:21:30.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266574_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266574_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:16:24.41 +58:04:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266611_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266611_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:35:01.28 +60:22:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266655_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266655_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:48:39.89 +59:09:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266691_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266691_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:31:32.42 +61:02:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266823_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266823_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:38:33.82 +60:47:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266845_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266845_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:55:53.03 +64:15:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266877_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266877_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:42:28.26 +58:17:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266899_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266899_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
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Considering the candidate 266920_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 266920_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:31:29.07 +58:12:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267071_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 267071_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 267281_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267281_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:02:53.96 +60:15:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267316_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267316_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:23:07.57 +61:11:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267451_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267451_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:18:04.19 +65:36:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267456_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267456_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:20:49.30 +64:40:20.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 267457_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267457_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:49:33.58 +59:44:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267526_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267526_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 267583_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267583_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:37:13.40 +58:38:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267684_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267684_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:38:06.53 +58:10:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267709_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 267709_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 267780_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267780_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:59:05.95 +59:55:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267783_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267783_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:14:21.92 +59:59:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267877_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267877_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:55:21.47 +59:25:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267882_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267882_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:46:18.39 +60:59:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267912_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 267912_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:44:32.18 +61:36:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267927_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 267927_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 267967_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 267967_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 268012_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 268012_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:14:00.29 +61:42:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268075_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 268075_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:14:29.88 +63:16:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268133_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 268133_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 268214_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 268214_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:34:34.54 +65:48:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268298_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 268298_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 268340_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 268340_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:55:21.92 +64:02:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268443_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 268443_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 268499_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 268499_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 268543_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 268543_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 268568_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 268568_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 268590_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 268590_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:54:34.77 +59:52:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268691_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 268691_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 268897_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 268897_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 269093_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 269093_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:49:06.13 +65:23:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269107_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 269107_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 269185_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 269185_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 269197_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 269197_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 269266_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 269266_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 269312_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 269312_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:14:00.68 +59:02:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269335_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 269335_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:16:02.37 +60:36:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269426_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 269426_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:11:42.11 +58:41:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269508_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 269508_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:58:04.83 +59:36:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269540_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 269540_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 269585_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 269585_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 269681_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 269681_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:46:50.66 +60:39:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 269897_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 269897_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:27:56.54 +62:46:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270005_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 270005_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:27:31.24 +59:41:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270017_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 270017_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:03:25.39 +57:50:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270073_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 270073_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:55:05.07 +59:57:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270176_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 270176_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 270317_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 270317_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:43:03.35 +58:57:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270377_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 270377_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 270469_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 270469_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 270530_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 270530_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:37:13.04 +58:38:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270734_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 270734_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:27:03.97 +64:43:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 270888_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 270888_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 271035_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 271035_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:10:10.35 +59:08:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271213_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 271213_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:15:05.43 +64:08:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271244_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 271244_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 271250_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 271250_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:34:42.58 +58:42:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271458_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 271458_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:44:56.67 +59:46:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271523_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 271523_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271544_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 271544_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 271690_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 271690_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 271805_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 271805_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 272088_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 272088_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 272161_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 272161_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:56:25.34 +62:05:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 272183_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 272183_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 272808_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 272808_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 272936_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 272936_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 273584_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 273584_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 273649_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 273649_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 273746_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 273746_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 273839_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 273839_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 273934_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 273934_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 274207_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 274207_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 274225_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 274225_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 274231_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 274231_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 274525_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 274525_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 274532_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 274532_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:36:13.67 +60:48:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 274774_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 274774_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 274817_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 274817_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 274984_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 274984_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 275052_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 275052_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 275173_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 275173_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 275463_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 275463_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 275554_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 275554_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
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Considering the candidate 275759_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 275759_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 276024_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 276024_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 276150_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 276150_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 276858_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 276858_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277223_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 277223_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277597_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 277597_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 277603_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 277603_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278135_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 278135_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:53:02.88 +60:26:37.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278276_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 278276_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:48:21.21 +62:53:03.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278310_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 278310_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 278318_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 278318_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70271_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 70271_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:20:32.42 +62:32:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125111_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
Preparing report for the candidate 125111_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21138_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 21138_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:15:23.57 +65:01:37.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153703_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 153703_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:18:22.40 +58:47:10.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112593_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 112593_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:21:55.07 +61:20:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72532_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 72532_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:45:35.60 +63:07:02.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170132_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 170132_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112249_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 112249_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234849_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 234849_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156692_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 156692_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:56:38.06 +59:15:33.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76113_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 76113_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 02:02:02.17 +62:41:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 39378_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
**** FOUND 01:47:55.68 +64:32:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28978_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383
The candidate 28978_fd_Cas-03-Q2b1x1_2026-05-25_03-51-34_20.00sec_4.90C_LIGHT_0383 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 293s
Prepared the HTML report for the field Cas-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:56:38.06 +59:15:33.8
01:33:44.53 +60:46:15.0
01:37:05.49 +62:54:32.1
01:11:20.02 +61:17:54.5
01:36:18.66 +64:32:20.3
01:41:22.16 +58:11:36.2
01:12:00.87 +64:42:19.2
01:34:57.74 +61:00:14.2
01:17:47.95 +57:25:42.1
01:59:58.42 +60:14:10.3
01:27:41.37 +59:04:45.6
01:11:16.57 +58:55:54.2
01:07:01.83 +59:46:18.7
01:06:15.91 +57:53:23.8
01:25:45.62 +59:01:19.9
01:10:04.96 +57:48:01.6
01:37:01.65 +62:19:20.0
01:04:37.03 +62:52:11.1
01:12:09.68 +58:47:53.2
01:32:46.75 +60:59:11.0
01:08:39.13 +60:32:39.6
01:36:48.85 +62:28:28.5
01:26:05.58 +59:01:14.6
01:39:59.26 +60:24:41.5
01:07:39.11 +59:59:17.8
01:43:07.95 +58:54:09.0
02:00:06.49 +59:00:32.6
01:25:27.57 +59:27:13.6
01:12:59.67 +57:34:05.9
01:25:00.93 +62:50:50.8
01:26:37.96 +60:38:03.7
02:20:45.34 +63:43:07.2
01:33:08.64 +61:46:15.7
01:10:43.69 +60:59:20.5
01:13:40.87 +60:51:24.9
01:24:55.02 +59:41:45.6
01:08:15.57 +61:15:06.2
01:13:27.21 +59:57:16.6
01:34:39.57 +59:40:47.6
01:24:49.24 +59:47:14.7
01:08:59.39 +60:47:21.1
01:11:44.66 +61:13:56.5
01:07:31.77 +61:28:27.5
01:26:36.35 +59:41:33.3
01:20:45.02 +57:55:08.6
01:56:43.74 +58:07:02.6
01:19:08.61 +60:33:57.4
01:49:15.81 +59:14:38.1
01:22:28.28 +61:07:37.1
01:25:51.85 +61:17:11.7
01:30:10.15 +59:36:19.1
01:31:23.03 +59:33:42.0
01:31:45.26 +59:35:57.1
01:35:24.95 +60:39:14.8
01:45:34.95 +59:18:09.5
01:25:26.59 +60:57:43.6
01:48:51.09 +59:35:49.5
01:25:56.67 +59:35:11.9
01:44:58.49 +57:57:47.5
01:47:13.05 +57:44:18.9
01:35:37.48 +61:16:48.8
01:28:00.44 +61:19:58.1
01:23:52.89 +60:48:43.7
01:26:15.45 +60:37:28.6
01:31:09.00 +59:34:13.0
01:29:33.38 +63:19:30.8
01:18:37.02 +58:41:37.3
02:00:21.87 +64:56:36.8
01:07:03.66 +59:18:15.9
01:51:09.35 +64:52:46.5
01:29:21.55 +61:44:13.4
01:36:16.25 +60:12:26.3
01:34:53.35 +60:45:26.6
01:29:10.32 +59:39:16.1
01:18:48.35 +64:12:22.5
01:38:05.76 +61:04:11.3
01:19:28.60 +59:54:38.2
02:16:37.80 +64:56:45.6
01:58:13.79 +60:03:14.7
01:22:11.14 +59:09:02.7
01:11:56.65 +58:41:02.0
01:17:48.33 +58:35:16.1
01:31:48.40 +64:21:55.3
02:17:05.29 +64:01:02.3
01:14:41.50 +58:46:44.7
02:00:32.82 +59:40:05.7
01:31:48.47 +64:22:27.8
02:21:38.50 +65:44:29.5
02:20:32.64 +62:45:43.0
02:01:03.52 +64:43:32.9
01:44:03.41 +61:54:43.1
01:13:39.07 +58:10:51.0
01:50:39.98 +62:00:55.2
01:29:39.14 +63:18:44.3
01:07:29.45 +63:11:00.7
01:48:29.48 +60:27:38.2
01:25:25.24 +58:19:59.4
01:59:34.12 +63:37:06.6
01:38:11.29 +61:01:59.0
01:31:55.99 +59:26:39.6
02:02:25.68 +64:38:22.6
01:45:26.42 +60:36:32.8
01:22:24.00 +61:13:49.6
01:13:18.74 +63:56:03.6
01:44:29.97 +65:09:24.5
01:24:36.09 +61:08:54.9
01:30:50.85 +60:06:03.2
01:13:13.57 +57:53:06.1
02:15:16.83 +59:21:33.6
01:37:59.74 +61:04:02.6
01:08:11.52 +62:14:22.7
01:22:13.56 +59:52:25.2
01:21:55.54 +63:45:18.9
01:40:28.47 +60:34:43.8
########### Completed Cas-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:56:38.06 +59:15:33.8
01:37:05.49 +62:54:32.1
01:11:20.02 +61:17:54.5
01:36:18.66 +64:32:20.3
01:41:22.16 +58:11:36.2
01:12:00.87 +64:42:19.2
01:34:57.74 +61:00:14.2
01:17:47.95 +57:25:42.1
01:59:58.42 +60:14:10.3
01:27:41.37 +59:04:45.6
01:11:16.57 +58:55:54.2
01:07:01.83 +59:46:18.7
01:06:15.91 +57:53:23.8
01:25:45.62 +59:01:19.9
01:10:04.96 +57:48:01.6
01:37:01.65 +62:19:20.0
01:04:37.03 +62:52:11.1
01:12:09.68 +58:47:53.2
01:32:46.75 +60:59:11.0
01:08:39.13 +60:32:39.6
01:36:48.85 +62:28:28.5
01:26:05.58 +59:01:14.6
01:39:59.26 +60:24:41.5
01:07:39.11 +59:59:17.8
01:43:07.95 +58:54:09.0
02:00:06.49 +59:00:32.6
01:25:27.57 +59:27:13.6
01:12:59.67 +57:34:05.9
01:25:00.93 +62:50:50.8
01:26:37.96 +60:38:03.7
02:20:45.34 +63:43:07.2
01:33:08.64 +61:46:15.7
01:10:43.69 +60:59:20.5
01:13:40.87 +60:51:24.9
01:24:55.02 +59:41:45.6
01:08:15.57 +61:15:06.2
01:13:27.21 +59:57:16.6
01:34:39.57 +59:40:47.6
01:24:49.24 +59:47:14.7
01:08:59.39 +60:47:21.1
01:11:44.66 +61:13:56.5
01:07:31.77 +61:28:27.5
01:26:36.35 +59:41:33.3
01:20:45.02 +57:55:08.6
01:56:43.74 +58:07:02.6
01:19:08.61 +60:33:57.4
01:49:15.81 +59:14:38.1
01:22:28.28 +61:07:37.1
01:25:51.85 +61:17:11.7
01:30:10.15 +59:36:19.1
01:31:23.03 +59:33:42.0
01:31:45.26 +59:35:57.1
01:35:24.95 +60:39:14.8
01:45:34.95 +59:18:09.5
01:25:26.59 +60:57:43.6
01:48:51.09 +59:35:49.5
01:25:56.67 +59:35:11.9
01:44:58.49 +57:57:47.5
01:47:13.05 +57:44:18.9
01:35:37.48 +61:16:48.8
01:28:00.44 +61:19:58.1
01:23:52.89 +60:48:43.7
01:26:15.45 +60:37:28.6
01:31:09.00 +59:34:13.0
01:29:33.38 +63:19:30.8
01:18:37.02 +58:41:37.3
02:00:21.87 +64:56:36.8
01:07:03.66 +59:18:15.9
01:51:09.35 +64:52:46.5
01:29:21.55 +61:44:13.4
01:36:16.25 +60:12:26.3
01:34:53.35 +60:45:26.6
01:29:10.32 +59:39:16.1
01:18:48.35 +64:12:22.5
01:38:05.76 +61:04:11.3
01:19:28.60 +59:54:38.2
02:16:37.80 +64:56:45.6
01:58:13.79 +60:03:14.7
01:22:11.14 +59:09:02.7
01:11:56.65 +58:41:02.0
01:17:48.33 +58:35:16.1
01:31:48.40 +64:21:55.3
02:17:05.29 +64:01:02.3
01:14:41.50 +58:46:44.7
02:00:32.82 +59:40:05.7
01:31:48.47 +64:22:27.8
02:21:38.50 +65:44:29.5
02:20:32.64 +62:45:43.0
02:01:03.52 +64:43:32.9
01:44:03.41 +61:54:43.1
01:13:39.07 +58:10:51.0
01:50:39.98 +62:00:55.2
01:29:39.14 +63:18:44.3
01:07:29.45 +63:11:00.7
01:48:29.48 +60:27:38.2
01:25:25.24 +58:19:59.4
01:59:34.12 +63:37:06.6
01:38:11.29 +61:01:59.0
01:31:55.99 +59:26:39.6
02:02:25.68 +64:38:22.6
01:45:26.42 +60:36:32.8
01:22:24.00 +61:13:49.6
01:13:18.74 +63:56:03.6
01:44:29.97 +65:09:24.5
01:24:36.09 +61:08:54.9
01:30:50.85 +60:06:03.2
01:13:13.57 +57:53:06.1
02:15:16.83 +59:21:33.6
01:37:59.74 +61:04:02.6
01:08:11.52 +62:14:22.7
01:22:13.56 +59:52:25.2
01:21:55.54 +63:45:18.9
01:40:28.47 +60:34:43.8
01:33:44.53 +60:46:15.0
###################################################################################
01:56:38.06 +59:15:33.8 -- not an asteroid (will add it to exclusion list)
01:37:05.49 +62:54:32.1 -- not an asteroid (will add it to exclusion list)
01:11:20.02 +61:17:54.5 -- not an asteroid (will add it to exclusion list)
01:36:18.66 +64:32:20.3 -- not an asteroid (will add it to exclusion list)
01:41:22.16 +58:11:36.2 -- not an asteroid (will add it to exclusion list)
01:12:00.87 +64:42:19.2 -- not an asteroid (will add it to exclusion list)
01:34:57.74 +61:00:14.2 -- not an asteroid (will add it to exclusion list)
01:17:47.95 +57:25:42.1 -- not an asteroid (will add it to exclusion list)
01:59:58.42 +60:14:10.3 -- not an asteroid (will add it to exclusion list)
01:27:41.37 +59:04:45.6 -- not an asteroid (will add it to exclusion list)
01:11:16.57 +58:55:54.2 -- not an asteroid (will add it to exclusion list)
01:07:01.83 +59:46:18.7 -- not an asteroid (will add it to exclusion list)
01:06:15.91 +57:53:23.8 -- not an asteroid (will add it to exclusion list)
01:25:45.62 +59:01:19.9 -- not an asteroid (will add it to exclusion list)
01:10:04.96 +57:48:01.6 -- not an asteroid (will add it to exclusion list)
01:37:01.65 +62:19:20.0 -- not an asteroid (will add it to exclusion list)
01:04:37.03 +62:52:11.1 -- not an asteroid (will add it to exclusion list)
01:12:09.68 +58:47:53.2 -- not an asteroid (will add it to exclusion list)
01:32:46.75 +60:59:11.0 -- not an asteroid (will add it to exclusion list)
01:08:39.13 +60:32:39.6 -- not an asteroid (will add it to exclusion list)
01:36:48.85 +62:28:28.5 -- not an asteroid (will add it to exclusion list)
01:26:05.58 +59:01:14.6 -- not an asteroid (will add it to exclusion list)
01:39:59.26 +60:24:41.5 -- not an asteroid (will add it to exclusion list)
01:07:39.11 +59:59:17.8 -- not an asteroid (will add it to exclusion list)
01:43:07.95 +58:54:09.0 -- not an asteroid (will add it to exclusion list)
02:00:06.49 +59:00:32.6 -- not an asteroid (will add it to exclusion list)
01:25:27.57 +59:27:13.6 -- not an asteroid (will add it to exclusion list)
01:12:59.67 +57:34:05.9 -- not an asteroid (will add it to exclusion list)
01:25:00.93 +62:50:50.8 -- not an asteroid (will add it to exclusion list)
01:26:37.96 +60:38:03.7 -- not an asteroid (will add it to exclusion list)
02:20:45.34 +63:43:07.2 -- not an asteroid (will add it to exclusion list)
01:33:08.64 +61:46:15.7 -- not an asteroid (will add it to exclusion list)
01:10:43.69 +60:59:20.5 -- not an asteroid (will add it to exclusion list)
01:13:40.87 +60:51:24.9 -- not an asteroid (will add it to exclusion list)
01:24:55.02 +59:41:45.6 -- not an asteroid (will add it to exclusion list)
01:08:15.57 +61:15:06.2 -- not an asteroid (will add it to exclusion list)
01:13:27.21 +59:57:16.6 -- not an asteroid (will add it to exclusion list)
01:34:39.57 +59:40:47.6 -- not an asteroid (will add it to exclusion list)
01:24:49.24 +59:47:14.7 -- not an asteroid (will add it to exclusion list)
01:08:59.39 +60:47:21.1 -- not an asteroid (will add it to exclusion list)
01:11:44.66 +61:13:56.5 -- not an asteroid (will add it to exclusion list)
01:07:31.77 +61:28:27.5 -- not an asteroid (will add it to exclusion list)
01:26:36.35 +59:41:33.3 -- not an asteroid (will add it to exclusion list)
01:20:45.02 +57:55:08.6 -- not an asteroid (will add it to exclusion list)
01:56:43.74 +58:07:02.6 -- not an asteroid (will add it to exclusion list)
01:19:08.61 +60:33:57.4 -- not an asteroid (will add it to exclusion list)
01:49:15.81 +59:14:38.1 -- not an asteroid (will add it to exclusion list)
01:22:28.28 +61:07:37.1 -- not an asteroid (will add it to exclusion list)
01:25:51.85 +61:17:11.7 -- not an asteroid (will add it to exclusion list)
01:30:10.15 +59:36:19.1 -- not an asteroid (will add it to exclusion list)
01:31:23.03 +59:33:42.0 -- not an asteroid (will add it to exclusion list)
01:31:45.26 +59:35:57.1 -- not an asteroid (will add it to exclusion list)
01:35:24.95 +60:39:14.8 -- not an asteroid (will add it to exclusion list)
01:45:34.95 +59:18:09.5 -- not an asteroid (will add it to exclusion list)
01:25:26.59 +60:57:43.6 -- not an asteroid (will add it to exclusion list)
01:48:51.09 +59:35:49.5 -- not an asteroid (will add it to exclusion list)
01:25:56.67 +59:35:11.9 -- not an asteroid (will add it to exclusion list)
01:44:58.49 +57:57:47.5 -- not an asteroid (will add it to exclusion list)
01:47:13.05 +57:44:18.9 -- not an asteroid (will add it to exclusion list)
01:35:37.48 +61:16:48.8 -- not an asteroid (will add it to exclusion list)
01:28:00.44 +61:19:58.1 -- not an asteroid (will add it to exclusion list)
01:23:52.89 +60:48:43.7 -- not an asteroid (will add it to exclusion list)
01:26:15.45 +60:37:28.6 -- not an asteroid (will add it to exclusion list)
01:31:09.00 +59:34:13.0 -- not an asteroid (will add it to exclusion list)
01:29:33.38 +63:19:30.8 -- not an asteroid (will add it to exclusion list)
01:18:37.02 +58:41:37.3 -- not an asteroid (will add it to exclusion list)
02:00:21.87 +64:56:36.8 -- not an asteroid (will add it to exclusion list)
01:07:03.66 +59:18:15.9 -- not an asteroid (will add it to exclusion list)
01:51:09.35 +64:52:46.5 -- not an asteroid (will add it to exclusion list)
01:29:21.55 +61:44:13.4 -- not an asteroid (will add it to exclusion list)
01:36:16.25 +60:12:26.3 -- not an asteroid (will add it to exclusion list)
01:34:53.35 +60:45:26.6 -- not an asteroid (will add it to exclusion list)
01:29:10.32 +59:39:16.1 -- not an asteroid (will add it to exclusion list)
01:18:48.35 +64:12:22.5 -- not an asteroid (will add it to exclusion list)
01:38:05.76 +61:04:11.3 -- not an asteroid (will add it to exclusion list)
01:19:28.60 +59:54:38.2 -- not an asteroid (will add it to exclusion list)
02:16:37.80 +64:56:45.6 -- not an asteroid (will add it to exclusion list)
01:58:13.79 +60:03:14.7 -- not an asteroid (will add it to exclusion list)
01:22:11.14 +59:09:02.7 -- not an asteroid (will add it to exclusion list)
01:11:56.65 +58:41:02.0 -- not an asteroid (will add it to exclusion list)
01:17:48.33 +58:35:16.1 -- not an asteroid (will add it to exclusion list)
01:31:48.40 +64:21:55.3 -- not an asteroid (will add it to exclusion list)
02:17:05.29 +64:01:02.3 -- not an asteroid (will add it to exclusion list)
01:14:41.50 +58:46:44.7 -- not an asteroid (will add it to exclusion list)
02:00:32.82 +59:40:05.7 -- not an asteroid (will add it to exclusion list)
01:31:48.47 +64:22:27.8 -- not an asteroid (will add it to exclusion list)
02:21:38.50 +65:44:29.5 -- not an asteroid (will add it to exclusion list)
02:20:32.64 +62:45:43.0 -- not an asteroid (will add it to exclusion list)
02:01:03.52 +64:43:32.9 -- not an asteroid (will add it to exclusion list)
01:44:03.41 +61:54:43.1 -- not an asteroid (will add it to exclusion list)
01:13:39.07 +58:10:51.0 -- not an asteroid (will add it to exclusion list)
01:50:39.98 +62:00:55.2 -- not an asteroid (will add it to exclusion list)
01:29:39.14 +63:18:44.3 -- not an asteroid (will add it to exclusion list)
01:07:29.45 +63:11:00.7 -- not an asteroid (will add it to exclusion list)
01:48:29.48 +60:27:38.2 -- not an asteroid (will add it to exclusion list)
01:25:25.24 +58:19:59.4 -- not an asteroid (will add it to exclusion list)
01:59:34.12 +63:37:06.6 -- not an asteroid (will add it to exclusion list)
01:38:11.29 +61:01:59.0 -- not an asteroid (will add it to exclusion list)
01:31:55.99 +59:26:39.6 -- not an asteroid (will add it to exclusion list)
02:02:25.68 +64:38:22.6 -- not an asteroid (will add it to exclusion list)
01:45:26.42 +60:36:32.8 -- not an asteroid (will add it to exclusion list)
01:22:24.00 +61:13:49.6 -- not an asteroid (will add it to exclusion list)
01:13:18.74 +63:56:03.6 -- not an asteroid (will add it to exclusion list)
01:44:29.97 +65:09:24.5 -- not an asteroid (will add it to exclusion list)
01:24:36.09 +61:08:54.9 -- not an asteroid (will add it to exclusion list)
01:30:50.85 +60:06:03.2 -- not an asteroid (will add it to exclusion list)
01:13:13.57 +57:53:06.1 -- not an asteroid (will add it to exclusion list)
02:15:16.83 +59:21:33.6 -- not an asteroid (will add it to exclusion list)
01:37:59.74 +61:04:02.6 -- not an asteroid (will add it to exclusion list)
01:08:11.52 +62:14:22.7 -- not an asteroid (will add it to exclusion list)
01:22:13.56 +59:52:25.2 -- not an asteroid (will add it to exclusion list)
01:21:55.54 +63:45:18.9 -- not an asteroid (will add it to exclusion list)
01:40:28.47 +60:34:43.8 -- not an asteroid (will add it to exclusion list)
01:33:44.53 +60:46:15.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:04:37.03 +62:52:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:15.91 +57:53:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:01.83 +59:46:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:03.66 +59:18:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:29.45 +63:11:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:31.77 +61:28:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.11 +59:59:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:11.52 +62:14:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:15.57 +61:15:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:39.13 +60:32:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:59.39 +60:47:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:04.96 +57:48:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:43.69 +60:59:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:16.57 +58:55:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:20.02 +61:17:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:44.66 +61:13:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:56.65 +58:41:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:00.87 +64:42:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:09.68 +58:47:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:59.67 +57:34:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:13.57 +57:53:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:18.74 +63:56:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:27.21 +59:57:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:39.07 +58:10:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:40.87 +60:51:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:41.50 +58:46:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:47.95 +57:25:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:48.33 +58:35:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:37.02 +58:41:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:48.35 +64:12:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:08.61 +60:33:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:28.60 +59:54:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:45.02 +57:55:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:55.54 +63:45:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:11.14 +59:09:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:13.56 +59:52:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:24.00 +61:13:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:28.28 +61:07:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:52.89 +60:48:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:36.09 +61:08:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:49.24 +59:47:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:55.02 +59:41:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:00.93 +62:50:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:25.24 +58:19:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:26.59 +60:57:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:27.57 +59:27:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:45.62 +59:01:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:51.85 +61:17:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:56.67 +59:35:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:05.58 +59:01:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:15.45 +60:37:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:36.35 +59:41:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:37.96 +60:38:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:41.37 +59:04:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:00.44 +61:19:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:10.32 +59:39:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:21.55 +61:44:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:33.38 +63:19:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:39.14 +63:18:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:10.15 +59:36:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:50.85 +60:06:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:09.00 +59:34:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:23.03 +59:33:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:45.26 +59:35:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.40 +64:21:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:48.47 +64:22:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:55.99 +59:26:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:46.75 +60:59:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:08.64 +61:46:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:44.53 +60:46:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:39.57 +59:40:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:53.35 +60:45:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:57.74 +61:00:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:24.95 +60:39:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:37.48 +61:16:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:16.25 +60:12:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:18.66 +64:32:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:48.85 +62:28:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:01.65 +62:19:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:05.49 +62:54:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:59.74 +61:04:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:05.76 +61:04:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:11.29 +61:01:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:59.26 +60:24:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:28.47 +60:34:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:22.16 +58:11:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:07.95 +58:54:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:03.41 +61:54:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:29.97 +65:09:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:58.49 +57:57:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:26.42 +60:36:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:34.95 +59:18:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:13.05 +57:44:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:29.48 +60:27:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:51.09 +59:35:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:15.81 +59:14:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:39.98 +62:00:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:09.35 +64:52:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:38.06 +59:15:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:43.74 +58:07:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:13.79 +60:03:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:34.12 +63:37:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:58.42 +60:14:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:06.49 +59:00:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:21.87 +64:56:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:00:32.82 +59:40:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:01:03.52 +64:43:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:25.68 +64:38:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:16.83 +59:21:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:16:37.80 +64:56:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:05.29 +64:01:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:32.64 +62:45:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:45.34 +63:43:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:38.50 +65:44:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:04:37.03 +62:52:11.1 -- a known variable star
01:06:15.91 +57:53:23.8 -- not a known variable star
01:07:01.83 +59:46:18.7 -- not a known variable star
01:07:03.66 +59:18:15.9 -- not a known variable star
01:07:29.45 +63:11:00.7 -- not a known variable star
01:07:31.77 +61:28:27.5 -- not a known variable star
01:07:39.11 +59:59:17.8 -- not a known variable star
01:08:11.52 +62:14:22.7 -- a known variable star
01:08:15.57 +61:15:06.2 -- not a known variable star
01:08:39.13 +60:32:39.6 -- not a known variable star
01:08:59.39 +60:47:21.1 -- not a known variable star
01:10:04.96 +57:48:01.6 -- not a known variable star
01:10:43.69 +60:59:20.5 -- not a known variable star
01:11:16.57 +58:55:54.2 -- not a known variable star
01:11:20.02 +61:17:54.5 -- not a known variable star
01:11:44.66 +61:13:56.5 -- a known variable star
01:11:56.65 +58:41:02.0 -- not a known variable star
01:12:00.87 +64:42:19.2 -- a known variable star
01:12:09.68 +58:47:53.2 -- not a known variable star
01:12:59.67 +57:34:05.9 -- not a known variable star
01:13:13.57 +57:53:06.1 -- a known variable star
01:13:18.74 +63:56:03.6 -- not a known variable star
01:13:27.21 +59:57:16.6 -- not a known variable star
01:13:39.07 +58:10:51.0 -- not a known variable star
01:13:40.87 +60:51:24.9 -- not a known variable star
01:14:41.50 +58:46:44.7 -- a known variable star
01:17:47.95 +57:25:42.1 -- not a known variable star
01:17:48.33 +58:35:16.1 -- not a known variable star
01:18:37.02 +58:41:37.3 -- a known variable star
01:18:48.35 +64:12:22.5 -- not a known variable star
01:19:08.61 +60:33:57.4 -- not a known variable star
01:19:28.60 +59:54:38.2 -- not a known variable star
01:20:45.02 +57:55:08.6 -- not a known variable star
01:21:55.54 +63:45:18.9 -- not a known variable star
01:22:11.14 +59:09:02.7 -- not a known variable star
01:22:13.56 +59:52:25.2 -- not a known variable star
01:22:24.00 +61:13:49.6 -- a known variable star
01:22:28.28 +61:07:37.1 -- a known variable star
01:23:52.89 +60:48:43.7 -- not a known variable star
01:24:36.09 +61:08:54.9 -- a known variable star
01:24:49.24 +59:47:14.7 -- not a known variable star
01:24:55.02 +59:41:45.6 -- not a known variable star
01:25:00.93 +62:50:50.8 -- not a known variable star
01:25:25.24 +58:19:59.4 -- not a known variable star
01:25:26.59 +60:57:43.6 -- not a known variable star
01:25:27.57 +59:27:13.6 -- a known variable star
01:25:45.62 +59:01:19.9 -- not a known variable star
01:25:51.85 +61:17:11.7 -- not a known variable star
01:25:56.67 +59:35:11.9 -- not a known variable star
01:26:05.58 +59:01:14.6 -- not a known variable star
01:26:15.45 +60:37:28.6 -- not a known variable star
01:26:36.35 +59:41:33.3 -- a known variable star
01:26:37.96 +60:38:03.7 -- not a known variable star
01:27:41.37 +59:04:45.6 -- not a known variable star
01:28:00.44 +61:19:58.1 -- not a known variable star
01:29:10.32 +59:39:16.1 -- not a known variable star
01:29:21.55 +61:44:13.4 -- not a known variable star
01:29:33.38 +63:19:30.8 -- a known variable star
01:29:39.14 +63:18:44.3 -- not a known variable star
01:30:10.15 +59:36:19.1 -- not a known variable star
01:30:50.85 +60:06:03.2 -- not a known variable star
01:31:09.00 +59:34:13.0 -- not a known variable star
01:31:23.03 +59:33:42.0 -- not a known variable star
01:31:45.26 +59:35:57.1 -- not a known variable star
01:31:48.40 +64:21:55.3 -- not a known variable star
01:31:48.47 +64:22:27.8 -- not a known variable star
01:31:55.99 +59:26:39.6 -- not a known variable star
01:32:46.75 +60:59:11.0 -- a known variable star
01:33:08.64 +61:46:15.7 -- not a known variable star
01:33:44.53 +60:46:15.0 -- not a known variable star
01:34:39.57 +59:40:47.6 -- a known variable star
01:34:53.35 +60:45:26.6 -- not a known variable star
01:34:57.74 +61:00:14.2 -- a known variable star
01:35:24.95 +60:39:14.8 -- a known variable star
01:35:37.48 +61:16:48.8 -- a known variable star
01:36:16.25 +60:12:26.3 -- not a known variable star
01:36:18.66 +64:32:20.3 -- not a known variable star
01:36:48.85 +62:28:28.5 -- not a known variable star
01:37:01.65 +62:19:20.0 -- not a known variable star
01:37:05.49 +62:54:32.1 -- not a known variable star
01:37:59.74 +61:04:02.6 -- not a known variable star
01:38:05.76 +61:04:11.3 -- not a known variable star
01:38:11.29 +61:01:59.0 -- not a known variable star
01:39:59.26 +60:24:41.5 -- not a known variable star
01:40:28.47 +60:34:43.8 -- not a known variable star
01:41:22.16 +58:11:36.2 -- not a known variable star
01:43:07.95 +58:54:09.0 -- not a known variable star
01:44:03.41 +61:54:43.1 -- not a known variable star
01:44:29.97 +65:09:24.5 -- a known variable star
01:44:58.49 +57:57:47.5 -- not a known variable star
01:45:26.42 +60:36:32.8 -- a known variable star
01:45:34.95 +59:18:09.5 -- not a known variable star
01:47:13.05 +57:44:18.9 -- a known variable star
01:48:29.48 +60:27:38.2 -- not a known variable star
01:48:51.09 +59:35:49.5 -- not a known variable star
01:49:15.81 +59:14:38.1 -- not a known variable star
01:50:39.98 +62:00:55.2 -- not a known variable star
01:51:09.35 +64:52:46.5 -- a known variable star
01:56:38.06 +59:15:33.8 -- a known variable star
01:56:43.74 +58:07:02.6 -- not a known variable star
01:58:13.79 +60:03:14.7 -- not a known variable star
01:59:34.12 +63:37:06.6 -- not a known variable star
01:59:58.42 +60:14:10.3 -- not a known variable star
02:00:06.49 +59:00:32.6 -- not a known variable star
02:00:21.87 +64:56:36.8 -- not a known variable star
02:00:32.82 +59:40:05.7 -- a known variable star
02:01:03.52 +64:43:32.9 -- not a known variable star
02:02:25.68 +64:38:22.6 -- a known variable star
02:15:16.83 +59:21:33.6 -- not a known variable star
02:16:37.80 +64:56:45.6 -- a known variable star
02:17:05.29 +64:01:02.3 -- not a known variable star
02:20:32.64 +62:45:43.0 -- a known variable star
02:20:45.34 +63:43:07.2 -- not a known variable star
02:21:38.50 +65:44:29.5 -- not a known variable star
Found 87 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
114 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 114 (excluding asteroids and hot pixels, 87 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)2461185.86871880 -observatory V36
05:00:09.62 +24:29:04.9 Mercury (-1.2mag)
06:31:38.47 +25:01:08.3 Venus (-3.9mag)
02:09:43.12 +12:21:14.1 Mars (1.3mag)
07:37:21.54 +21:57:50.4 Jupiter (-1.9mag)
00:45:01.39 +02:24:17.4 Saturn (0.9mag)
03:56:52.27 +20:15:43.5 Uranus (5.8mag)
00:15:09.73 +00:11:10.1 Neptune (7.8mag)
20:33:57.89 -22:59:48.8 Pluto (14.5mag)
11:41:24.89 -00:54:45.9 Moon (-11.0mag)
-rw-r--r-- 1 apache apache 363 May 25 04:30 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461185.86871880:
07:37:29.04 +21:57:31.1 Io (5.9mag)
07:37:29.19 +21:57:31.4 Europa (6.1mag)
07:37:06.05 +21:58:34.8 Ganymede (5.5mag)
07:37:07.22 +21:58:22.2 Callisto (6.7mag)
07:38:29.68 +21:34:14.9 Himalia (15.5mag)
07:37:18.88 +21:57:58.8 Thebe (16.5mag)
07:38:48.96 +21:55:51.6 Elara (17.5mag)
07:38:46.51 +22:17:02.0 Pasiphae (17.7mag)
07:44:30.54 +21:58:37.0 Carme (18.8mag)
00:44:59.87 +02:24:00.9 Titan (8.7mag)
00:44:59.91 +02:24:32.5 Rhea (10.0mag)
00:45:22.50 +02:24:15.2 Iapetus (11.4mag)
00:45:16.71 +02:24:13.9 Hyperion (14.7mag)
00:45:59.94 +02:28:11.1 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 25 04:30 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461185.86871880:
17:15:46.87 -33:12:18.4 JWST
20:02:34.91 -05:37:15.6 Chandra
20:43:49.51 +37:03:48.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 25 04:30 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461185.86871880 -observatory V36
13:21:28.15 -27:08:37.3 14.4mag D/1884 O1 (Barnard)
06:35:56.94 +30:41:34.1 15.7mag D/1886 K1 (Brooks)
15:27:02.41 +01:18:54.4 14.6mag D/1895 Q1 (Swift)
05:26:52.36 +24:37:08.7 17.2mag D/1918 W1 (Schorr)
09:25:37.95 +15:17:01.1 17.9mag P/2009 WX51 (Catalina)
18:51:22.85 -31:35:35.9 13.7mag P/2010 H2 (Vales)
05:40:06.89 -68:17:03.7 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:44:04.17 +31:47:56.0 17.4mag C/2017 K2 (PANSTARRS)
17:20:10.14 +14:29:21.0 17.7mag C/2021 G2 (ATLAS)
23:14:36.42 +31:00:38.3 17.2mag C/2022 E2 (ATLAS)
05:17:00.36 +26:50:52.2 16.4mag C/2022 N2 (PANSTARRS)
09:20:27.40 +31:30:57.1 16.5mag C/2022 QE78 (ATLAS)
08:43:38.48 +03:10:04.3 17.6mag C/2022 R6 (PANSTARRS)
18:36:50.54 +21:10:14.0 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:24:47.24 -11:02:33.7 17.5mag P/2023 B1 (PANSTARRS)
22:16:09.57 +65:36:20.0 17.7mag C/2023 H5 (Lemmon)
18:18:53.57 -05:28:21.4 13.7mag C/2023 R1 (PANSTARRS)
13:42:44.69 +85:57:46.5 17.9mag C/2023 X2 (Lemmon)
06:52:26.95 +63:54:29.3 17.6mag C/2024 A1 (ATLAS)
06:25:34.34 +26:22:59.3 13.1mag C/2024 E1 (Wierzchos)
15:48:33.68 +12:06:55.5 17.3mag C/2024 G6 (ATLAS)
20:20:06.14 +26:55:24.6 14.1mag C/2024 J3 (ATLAS)
04:04:10.28 -17:17:22.4 16.1mag C/2024 T5 (ATLAS)
05:52:53.51 +36:57:53.0 17.9mag C/2025 J1 (Borisov)
11:46:42.10 +53:21:27.7 16.9mag C/2025 L1 (ATLAS)
06:23:16.81 -10:07:45.4 12.5mag C/2025 R3 (PANSTARRS)
12:41:05.39 +04:36:14.4 17.2mag C/2025 Y1 (ATLAS)
01:34:41.25 +42:18:37.7 15.7mag C/2026 B2 (Sun-Gao)
11:10:30.91 -09:21:41.5 16.2mag A/2026 E1
19:58:08.90 -08:07:20.7 9.5mag 10P/Tempel
14:19:07.36 -02:27:21.2 17.6mag 24P/Schaumasse
10:59:37.61 -00:51:51.2 15.9mag 29P/Schwassmann-Wachmann
10:50:47.01 -02:34:20.5 17.7mag 43P/Wolf-Harrington
02:50:11.44 +23:43:07.3 17.6mag 47P/Ashbrook-Jackson
08:30:31.15 +27:35:06.7 16.9mag 63P/Wild
00:14:04.85 -07:23:21.2 15.7mag 65P/Gunn
05:59:04.20 +31:32:52.0 16.5mag 76P/West-Kohoutek-Ikemura
02:36:02.05 +15:15:58.2 13.9mag 78P/Gehrels
00:49:13.19 +01:37:05.0 15.3mag 88P/Howell
04:10:10.39 +28:50:07.2 15.1mag 93P/Lovas
02:05:16.83 +25:12:03.1 18.0mag 114P/Wiseman-Skiff
06:18:07.35 +33:19:49.4 15.7mag 123P/West-Hartley
09:26:35.91 +20:37:28.5 16.4mag 124P/Mrkos
03:36:16.24 +18:13:24.9 16.4mag 128P/Shoemaker-Holt
04:05:56.74 +18:17:36.1 17.7mag 131P/Mueller
04:54:44.84 +19:40:00.4 12.9mag 141P/Machholz
04:57:26.25 +16:15:31.9 12.8mag 141P-A/Machholz
03:42:12.23 +13:31:21.3 10.6mag 141P-D/Machholz
02:47:35.55 -26:47:07.4 17.3mag 161P/Hartley-IRAS
02:57:22.31 +17:51:47.6 14.9mag 162P/SidingSpring
19:34:27.80 -01:54:14.0 17.6mag 169P/NEAT
17:02:58.15 -09:25:45.5 16.2mag 235P/LINEAR
07:03:10.51 +35:52:34.5 17.3mag 240P/NEAT
23:56:27.85 -08:05:11.1 16.8mag 260P/McNaught
03:27:56.52 +29:45:05.3 17.7mag 295P/LINEAR
21:57:01.95 -28:31:46.7 17.7mag 320P/McNaught
15:22:11.04 +08:21:51.6 17.4mag 391P/Kowalski
07:56:37.89 +21:03:13.7 17.8mag 450P/LONEOS
06:37:26.27 +42:38:26.7 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 25 04:30 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
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
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
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
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
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
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
-rw-r--r-- 1 apache apache 5.6K May 25 04:30 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
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
-rw-r--r-- 1 apache apache 188K May 25 04:30 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:23:56.695 +21:12:04.15 SN 2026mxg 2026-05-15.26 20.5476
16:26:51.090 +23:30:02.07 AT 2026mxf 2026-05-09.79 20.19
12:32:29.870 +24:17:28.39 AT 2026mxe 2026-05-07.78 20.84
18:52:28.230 +41:35:58.05 AT 2026mxd 2026-05-06.77 20.29
16:01:49.510 +16:19:54.29 AT 2026mxc 2026-05-03.86 20.43
13:07:34.620 +48:36:49.59 AT 2026mxb 2026-04-28.84 21.35
12:41:13.920 +28:45:38.69 AT 2026mxa 2026-04-28.86 20.83
17:59:59.500 +26:37:11.25 AT 2026mwz 2026-04-27.89 21.34
12:28:50.550 +41:12:21.53 AT 2026mwy 2026-04-24.82 20.86
14:02:54.920 +52:50:36.73 AT 2026mwx 2026-04-19.86 21.51
12:33:02.940 +24:34:37.91 AT 2026mww 2026-04-15.87 21.01
16:40:46.740 +26:54:33.05 AT 2026mwv 2026-04-12.76 21.07
13:03:52.940 +23:49:42.82 AT 2026mwu 2026-04-03.87 20.84
17:45:23.200 +33:15:24.68 AT 2026mwt 2026-03-30.83 20.98
13:11:30.630 +21:00:44.67 AT 2026mws 2026-03-23.71 21.69
12:21:33.740 +27:53:15.15 AT 2026mwr 2026-03-23.70 21
14:26:34.570 +01:19:55.58 AT 2026mwq 2026-05-11.69 22.6
13:16:20.230 +02:48:58.63 AT 2026mwp 2026-05-03.68 21.84
13:17:52.545 -50:04:09.72 AT 2026mwo 2026-04-12.49 19.69
11:28:16.230 +42:22:52.41 AT 2026mwn 2026-05-12.89 19.9
-rw-r--r-- 1 apache apache 30K May 25 04:30 tns_transients_list.txt
