This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8
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 09.4164 2461169.9164 10.46 00:37:00.24 +63:08:01.5
121.30205 0.30769 galactic Cas Second-epoch detections are separated by 0.3" and 2.9 pix
The object was found in VSX 6" TY Cas
Type: M
# Max. Min./Amp. JD0 Period
10.100 V 19.000 V 2443405.00000 645.000000000000 M6-M8
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:37:00.24 +63:08:01.5: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:37:00.24 +63:08:01.5: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 37 00.24 +63 08 01.5 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
TY Cas,2461169.9164,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TY Cas 20260509.4164 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.37 01:49:54.28 +63:40:38.1
129.35906 1.53746 galactic Cas Second-epoch detections are separated by 3.5" 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 | 01:49:54.28 +63:40:38.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:54.28 +63:40:38.1: 12.54 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:54.28 +63:40:38.1: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 49 54.28 +63 40 38.1 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,2461169.9164,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.71 01:26:01.91 +57:08:04.9
127.63363 -5.42091 galactic Cas Second-epoch detections are separated by 2.3" 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 | 01:26:01.91 +57:08:04.9 (user input) | T | P | (position from user input) J-Ks=0.811+/-0.037 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:01.91 +57:08:04.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:01.91 +57:08:04.9: 14.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.21 +/- 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 09.4164* 01 26 01.91 +57 08 04.9 11.7 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,2461169.9164,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.71CV 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 09.4164 2461169.9164 11.49 01:57:29.18 +60:09:19.3
131.06663 -1.66907 galactic Cas Second-epoch detections are separated by 0.9" 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 | 01:57:29.18 +60:09:19.3 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:29.18 +60:09:19.3: 12.88 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:29.18 +60:09:19.3: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 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 09.4164* 01 57 29.18 +60 09 19.3 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,2461169.9164,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.32 01:50:10.11 +57:10:52.0
130.85564 -4.78434 galactic Cas Second-epoch detections are separated by 1.2" 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 | 01:50:10.11 +57:10:52.0 (user input) | T | P | (position from user input) J-Ks=0.789+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:10.11 +57:10:52.0: 12.49 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:10.11 +57:10:52.0: 13.54 +/- 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 09.4164* 01 50 10.11 +57 10 52.0 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,2461169.9164,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.34 01:29:45.03 +59:58:32.3
127.71246 -2.54002 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 | target | 01:29:45.03 +59:58:32.3 (user input) | T | P | (position from user input) J-Ks=0.742+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:45.03 +59:58:32.3: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:45.03 +59:58:32.3: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 09.4164* 01 29 45.03 +59 58 32.3 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,2461169.9164,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.34CV 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 09.4164 2461169.9164 11.46 01:11:20.01 +61:17:54.4
125.31911 -1.48105 galactic Cas Second-epoch detections are separated by 0.0" 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 | 01:11:20.01 +61:17:54.4 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.029 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:20.01 +61:17:54.4: 13.06 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:20.01 +61:17:54.4: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 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 09.4164* 01 11 20.01 +61 17 54.4 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,2461169.9164,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.30 01:10:01.79 +66:17:40.5
124.80232 3.49038 galactic Cas Second-epoch detections are separated by 6.2" 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 | 01:10:01.79 +66:17:40.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:01.79 +66:17:40.5: 12.82 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:01.79 +66:17:40.5: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 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 09.4164* 01 10 01.79 +66 17 40.5 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,2461169.9164,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.30CV 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 09.4164 2461169.9164 11.01 02:30:11.32 +66:01:46.4
132.74000 5.05630 galactic Cas Second-epoch detections are separated by 3.4" 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 | 02:30:11.32 +66:01:46.4 (user input) | T | P | (position from user input) J-Ks=0.267+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:11.32 +66:01:46.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:11.32 +66:01:46.4: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 30 11.32 +66 01 46.4 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,2461169.9164,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.45 01:02:07.21 +61:19:23.6
124.21353 -1.52194 galactic Cas Second-epoch detections are separated by 5.3" 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 | Gaia DR3 426637965010389376 | 01:02:01.52 +61:19:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.590+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:07.21 +61:19:23.6: 11.94 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:07.21 +61:19:23.6: 14.03 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 09.4164* 01 02 07.21 +61 19 23.6 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
Gaia DR3 426637965010389376,2461169.9164,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426637965010389376 20260509.4164 11.45CV 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 09.4164 2461169.9164 11.24 01:58:50.68 +56:57:17.7
132.05854 -4.71761 galactic Per Second-epoch detections are separated by 2.4" 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 J029.7112+56.9548 | 01:58:50.68 +56:57:17.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.404+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:50.68 +56:57:17.7: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:50.68 +56:57:17.7: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 58 50.68 +56 57 17.7 11.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J029.7112+56.9548,2461169.9164,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J029.7112+56.9548 20260509.4164 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.31 01:19:26.87 +57:22:51.4
126.71604 -5.28486 galactic Cas Second-epoch detections are separated by 3.1" 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 J019.8691+57.3895 | 01:19:26.87 +57:22:51.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.265+/-0.055 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:26.87 +57:22:51.4: 13.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:26.87 +57:22:51.4: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 09.4164* 01 19 26.87 +57 22 51.4 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 J019.8691+57.3895,2461169.9164,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.8691+57.3895 20260509.4164 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.32 01:22:50.45 +58:12:42.0
127.07044 -4.40752 galactic Cas Second-epoch detections are separated by 1.2" and 3.3 pix
The object was found in VSX21" Gaia DR3 413816392424091520
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.040 G 13.070 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:22:50.45 +58:12:42.0: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:22:50.45 +58:12:42.0: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.22 +/- 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 09.4164* 01 22 50.45 +58 12 42.0 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 413816392424091520,2461169.9164,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413816392424091520 20260509.4164 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 09.4164 2461169.9164 11.28 02:03:02.00 +56:50:06.8
132.64365 -4.68045 galactic Per Second-epoch detections are separated by 0.4" 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 | 02:03:02.00 +56:50:06.8 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:03:02.00 +56:50:06.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:03:02.00 +56:50:06.8: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 09.4164* 02 03 02.00 +56 50 06.8 11.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.37 01:06:16.04 +57:53:24.3
124.90886 -4.92473 galactic Cas Second-epoch detections are separated by 2.4" 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 | ATO J016.5720+57.8855 | 01:06:16.04 +57:53:24.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.781+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:16.04 +57:53:24.3: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:16.04 +57:53:24.3: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 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 09.4164* 01 06 16.04 +57 53 24.3 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
ATO J016.5720+57.8855,2461169.9164,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J016.5720+57.8855 20260509.4164 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 09.4164 2461169.9164 11.27 01:15:36.33 +63:27:54.0
125.62731 0.71980 galactic Cas Second-epoch detections are separated by 1.6" and 2.9 pix
The object was found in VSX13" PMAK V23
Type: EB
# Max. Min./Amp. JD0 Period
14.280 V 15.080 V 2457777.85500 0.693731000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:36.33 +63:27:54.0: 11.87 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:36.33 +63:27:54.0: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 15 36.33 +63 27 54.0 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
PMAK V23,2461169.9164,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PMAK V23 20260509.4164 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.40 01:27:12.82 +58:27:16.9
127.60926 -4.09178 galactic Cas Second-epoch detections are separated by 0.7" 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 | 01:27:12.82 +58:27:16.9 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:12.82 +58:27:16.9: 11.63 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:12.82 +58:27:16.9: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 27 12.82 +58 27 16.9 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,2461169.9164,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.40CV 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 09.4164 2461169.9164 11.41 01:47:04.43 +59:18:55.3
129.98650 -2.79221 galactic Cas Second-epoch detections are separated by 1.6" 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 | target | 01:47:04.43 +59:18:55.3 (user input) | T | P | (position from user input) J-Ks=0.500+/-0.079 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:04.43 +59:18:55.3: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:04.43 +59:18:55.3: 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 09.4164* 01 47 04.43 +59 18 55.3 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,2461169.9164,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.21 01:13:09.81 +64:30:33.5
125.26762 1.73613 galactic Cas Second-epoch detections are separated by 7.1" 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 | 01:13:09.81 +64:30:33.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:09.81 +64:30:33.5: 12.35 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:09.81 +64:30:33.5: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 13 09.81 +64 30 33.5 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,2461169.9164,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.19 00:49:57.44 +60:17:56.5
122.74834 -2.57219 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 | target | 00:49:57.44 +60:17:56.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:49:57.44 +60:17:56.5: 11.07 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:49:57.44 +60:17:56.5: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.47 +/- 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 09.4164* 00 49 57.44 +60 17 56.5 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,2461169.9164,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.17 00:44:47.70 +66:11:33.2
122.26049 3.32947 galactic Cas Second-epoch detections are separated by 4.1" 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 | target | 00:44:47.70 +66:11:33.2 (user input) | T | P | (position from user input) J-Ks=0.742+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:44:47.70 +66:11:33.2: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:44:47.70 +66:11:33.2: 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 09.4164* 00 44 47.70 +66 11 33.2 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,2461169.9164,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.34 01:09:10.52 +58:09:35.5
125.27724 -4.63109 galactic Cas Second-epoch detections are separated by 1.4" 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 | 01:09:10.52 +58:09:35.5 (user input) | T | P | (position from user input) J-Ks=0.750+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:10.52 +58:09:35.5: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:10.52 +58:09:35.5: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.89 +/- 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 09.4164* 01 09 10.52 +58 09 35.5 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,2461169.9164,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.34CV 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 09.4164 2461169.9164 11.14 01:08:39.16 +60:32:40.7
125.04837 -2.25635 galactic Cas Second-epoch detections are separated by 1.4" 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 | 01:08:39.16 +60:32:40.7 (user input) | T | P | (position from user input) J-Ks=0.751+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:39.16 +60:32:40.7: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:39.16 +60:32:40.7: 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 09.4164* 01 08 39.16 +60 32 40.7 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,2461169.9164,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.14CV 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 09.4164 2461169.9164 11.03 02:21:32.56 +56:32:12.5
135.16027 -4.18053 galactic Per Second-epoch detections are separated by 1.5" 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 | ATO J035.3668+56.5341 | 02:21:32.56 +56:32:12.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.845+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:32.56 +56:32:12.5: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:32.56 +56:32:12.5: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 21 32.56 +56 32 12.5 11.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J035.3668+56.5341,2461169.9164,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J035.3668+56.5341 20260509.4164 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.24 01:10:12.02 +59:17:25.4
125.32983 -3.49398 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 | ATO J017.5672+59.2942 | 01:10:12.02 +59:17:25.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.414+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:10:12.02 +59:17:25.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:10:12.02 +59:17:25.4: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 09.4164* 01 10 12.02 +59 17 25.4 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 J017.5672+59.2942,2461169.9164,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.5672+59.2942 20260509.4164 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.05 01:50:46.76 +58:00:38.2
130.74639 -3.95796 galactic Per Second-epoch detections are separated by 1.9" 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 J027.6849+58.0117 | 01:50:46.76 +58:00:38.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.703+/-0.024 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:46.76 +58:00:38.2: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:46.76 +58:00:38.2: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 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 09.4164* 01 50 46.76 +58 00 38.2 11.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J027.6849+58.0117,2461169.9164,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J027.6849+58.0117 20260509.4164 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 09.4164 2461169.9164 11.30 01:07:39.08 +59:59:18.1
124.96050 -2.81951 galactic Cas Second-epoch detections are separated by 1.8" 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 | 01:07:39.08 +59:59:18.1 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:39.08 +59:59:18.1: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:39.08 +59:59:18.1: 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 09.4164* 01 07 39.08 +59 59 18.1 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
target,2461169.9164,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.30CV 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 09.4164 2461169.9164 11.23 01:09:22.85 +58:34:03.2
125.27582 -4.22251 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 | 01:09:22.85 +58:34:03.2 (user input) | T | P | (position from user input) J-Ks=0.972+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.85 +58:34:03.2: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.85 +58:34:03.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 09 22.85 +58 34 03.2 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,2461169.9164,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.26 01:06:37.45 +60:22:38.2
124.80917 -2.43911 galactic Cas Second-epoch detections are separated by 2.8" 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 | Large-amplitude variable Gaia DR2 426374773712549504 | 01:06:37.45 +60:22:38.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.644+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:37.45 +60:22:38.2: 12.33 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:37.45 +60:22:38.2: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 09.4164* 01 06 37.45 +60 22 38.2 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
Large-amplitude variable Gaia DR2 426374773712549504,2461169.9164,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 426374773712549504 20260509.4164 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.11 01:15:44.77 +60:02:45.6
125.96528 -2.68250 galactic Cas Second-epoch detections are separated by 1.6" 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 | 01:15:44.77 +60:02:45.6 (user input) | T | P | (position from user input) J-Ks=0.321+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:15:44.77 +60:02:45.6: 12.58 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:15:44.77 +60:02:45.6: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 09.4164* 01 15 44.77 +60 02 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,2461169.9164,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.09 01:29:49.42 +58:16:02.6
127.97588 -4.22794 galactic Cas Second-epoch detections are separated by 0.6" 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 | ATO J022.4440+58.2711 | 01:29:49.42 +58:16:02.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.784+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:49.42 +58:16:02.6: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:49.42 +58:16:02.6: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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 09.4164* 01 29 49.42 +58 16 02.6 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 J022.4440+58.2711,2461169.9164,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.4440+58.2711 20260509.4164 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 09.4164 2461169.9164 11.15 01:25:52.13 +57:05:24.0
127.61763 -5.46817 galactic Cas Second-epoch detections are separated by 0.4" and 3.2 pix
The object was found in VSX 3" Gaia DR3 412948431071906944
Type: ROT
# Max. Min./Amp. JD0 Period
15.550 G 15.580 G 1.711830000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:52.13 +57:05:24.0: 11.66 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:52.13 +57:05:24.0: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 25 52.13 +57 05 24.0 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
Gaia DR3 412948431071906944,2461169.9164,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 412948431071906944 20260509.4164 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 09.4164 2461169.9164 11.06 01:07:00.11 +61:28:29.9
124.78943 -1.34063 galactic Cas Second-epoch detections are separated by 1.8" and 2.8 pix
The object was found in VSX15" Gaia DR3 522542355648755328
Type: L
# Max. Min./Amp. JD0 Period
17.340 G 17.500 G O
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:00.11 +61:28:29.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:00.11 +61:28:29.9: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 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 09.4164* 01 07 00.11 +61 28 29.9 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 522542355648755328,2461169.9164,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522542355648755328 20260509.4164 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 09.4164 2461169.9164 10.97 01:01:11.29 +65:10:55.4
123.95564 2.32969 galactic Cas Second-epoch detections are separated by 1.5" 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 | target | 01:01:11.29 +65:10:55.4 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.069 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:11.29 +65:10:55.4: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:01:11.29 +65:10:55.4: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 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 09.4164* 01 01 11.29 +65 10 55.4 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,2461169.9164,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.89 02:47:22.83 +63:30:07.2
135.44180 3.48217 galactic Cas Second-epoch detections are separated by 3.3" and 4.0 pix
The object was found in VSX25" ASASSN-V J024719.18+633011.7
Type: ROT
# Max. Min./Amp. JD0 Period
13.700 V 13.790 V 2458118.89000 1.159400000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:47:22.83 +63:30:07.2: 13.16 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:47:22.83 +63:30:07.2: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 09.4164* 02 47 22.83 +63 30 07.2 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J024719.18+633011.7,2461169.9164,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J024719.18+633011.7 20260509.4164 10.89CV 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 09.4164 2461169.9164 11.14 00:46:55.69 +60:00:23.1
122.36763 -2.86039 galactic Cas Second-epoch detections are separated by 1.6" 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 | 00:46:55.69 +60:00:23.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:46:55.69 +60:00:23.1: 11.61 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:46:55.69 +60:00:23.1: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 09.4164* 00 46 55.69 +60 00 23.1 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
target,2461169.9164,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.14CV 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 09.4164 2461169.9164 10.84 01:47:27.75 +64:31:09.8
128.91328 2.30023 galactic Cas Second-epoch detections are separated by 2.5" 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 | Large-amplitude variable Gaia DR2 512256939768857856 | 01:47:24.78 +64:31:17.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:27.75 +64:31:09.8: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:27.75 +64:31:09.8: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 47 27.75 +64 31 09.8 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
Large-amplitude variable Gaia DR2 512256939768857856,2461169.9164,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 512256939768857856 20260509.4164 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 09.4164 2461169.9164 11.04 02:24:32.99 +56:11:30.8
135.67198 -4.35934 galactic Per Second-epoch detections are separated by 2.8" 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 | 02:24:32.99 +56:11:30.8 (user input) | T | P | (position from user input) J-Ks=0.253+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:24:32.99 +56:11:30.8: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:24:32.99 +56:11:30.8: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 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 09.4164* 02 24 32.99 +56 11 30.8 11.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.12 00:58:14.09 +60:18:23.5
123.77439 -2.55410 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 | 00:58:14.09 +60:18:23.5 (user input) | T | P | (position from user input) J-Ks=2.312+/- (Very red!)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:58:14.09 +60:18:23.5: 11.78 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:58:14.09 +60:18:23.5: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 09.4164* 00 58 14.09 +60 18 23.5 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,2461169.9164,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.88 02:17:30.25 +56:22:50.2
134.68549 -4.51440 galactic Per Second-epoch detections are separated by 0.9" and 3.5 pix
The object was found in VSX 1" Gaia DR3 456815131089871744
Type: ROT
# Max. Min./Amp. JD0 Period
13.400 G 13.440 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:17:30.25 +56:22:50.2: 12.63 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:17:30.25 +56:22:50.2: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 09.4164* 02 17 30.25 +56 22 50.2 10.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 456815131089871744,2461169.9164,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 456815131089871744 20260509.4164 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 09.4164 2461169.9164 11.17 01:12:59.76 +57:33:52.4
125.83142 -5.18578 galactic Cas Second-epoch detections are separated by 2.1" 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 | 01:12:59.76 +57:33:52.4 (user input) | T | P | (position from user input) J-Ks=0.836+/-0.053 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:12:59.76 +57:33:52.4: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:12:59.76 +57:33:52.4: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 12 59.76 +57 33 52.4 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,2461169.9164,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.04 00:49:18.55 +65:56:10.8
122.71461 3.06548 galactic Cas Second-epoch detections are separated by 2.6" 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 | 00:49:18.55 +65:56:10.8 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:49:18.55 +65:56:10.8: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:49:18.55 +65:56:10.8: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 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 09.4164* 00 49 18.55 +65 56 10.8 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,2461169.9164,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.05 01:30:34.21 +59:44:32.0
127.84931 -2.75538 galactic Cas Second-epoch detections are separated by 1.5" 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 J022.6525+59.7408 | 01:30:34.21 +59:44:32.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.454+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:34.21 +59:44:32.0: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:34.21 +59:44:32.0: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 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 09.4164* 01 30 34.21 +59 44 32.0 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 J022.6525+59.7408,2461169.9164,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.6525+59.7408 20260509.4164 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 09.4164 2461169.9164 11.17 01:13:01.33 +61:00:58.3
125.54490 -1.74600 galactic Cas Second-epoch detections are separated by 2.5" and 3.2 pix
The object was found in VSX 4" Gaia DR3 522455906553654144
Type:
# Max. Min./Amp. JD0 Period
16.000 G 16.860 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:01.33 +61:00:58.3: 12.26 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:01.33 +61:00:58.3: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 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 09.4164* 01 13 01.33 +61 00 58.3 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 522455906553654144,2461169.9164,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522455906553654144 20260509.4164 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 09.4164 2461169.9164 11.02 01:02:18.44 +60:28:18.8
124.27193 -2.37158 galactic Cas Second-epoch detections are separated by 1.8" 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 | 01:02:18.44 +60:28:18.8 (user input) | T | P | (position from user input) J-Ks=0.226+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:18.44 +60:28:18.8: 10.89 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:18.44 +60:28:18.8: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 09.4164* 01 02 18.44 +60 28 18.8 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,2461169.9164,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.01 00:44:18.35 +64:55:16.2
122.17577 2.05989 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 | target | 00:44:18.35 +64:55:16.2 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:44:18.35 +64:55:16.2: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:44:18.35 +64:55:16.2: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 09.4164* 00 44 18.35 +64 55 16.2 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
target,2461169.9164,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.72 02:32:09.71 +57:05:33.2
136.31748 -3.13827 galactic Per Second-epoch detections are separated by 1.8" and 3.6 pix
The object was found in VSX 1" Gaia DR3 457975081496330368
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.180 G 13.220 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:09.71 +57:05:33.2: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:09.71 +57:05:33.2: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 09.4164* 02 32 09.71 +57 05 33.2 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457975081496330368,2461169.9164,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457975081496330368 20260509.4164 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 09.4164 2461169.9164 10.96 01:03:55.36 +59:40:27.1
124.50967 -3.15930 galactic Cas Second-epoch detections are separated by 1.0" 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 | 01:03:55.36 +59:40:27.1 (user input) | T | P | (position from user input) J-Ks=0.235+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:03:55.36 +59:40:27.1: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:03:55.36 +59:40:27.1: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 09.4164* 01 03 55.36 +59 40 27.1 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
target,2461169.9164,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.84 02:12:41.30 +62:42:19.4
132.09399 1.28790 galactic Cas Second-epoch detections are separated by 2.7" 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 | target | 02:12:41.30 +62:42:19.4 (user input) | T | P | (position from user input) J-Ks=0.922+/-0.027 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:12:41.30 +62:42:19.4: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:12:41.30 +62:42:19.4: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 09.4164* 02 12 41.30 +62 42 19.4 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.13 00:41:18.92 +60:08:55.3
121.67120 -2.69827 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 | 00:41:18.92 +60:08:55.3 (user input) | T | P | (position from user input) J-Ks=0.967+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:41:18.92 +60:08:55.3: 12.36 +/- 0.20 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:41:18.92 +60:08:55.3: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 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 09.4164* 00 41 18.92 +60 08 55.3 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,2461169.9164,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.12 01:05:58.37 +57:11:40.4
124.90921 -5.62138 galactic Cas Second-epoch detections are separated by 2.2" 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 | target | 01:05:58.37 +57:11:40.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:58.37 +57:11:40.4: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:58.37 +57:11:40.4: 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 09.4164* 01 05 58.37 +57 11 40.4 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
target,2461169.9164,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.98 01:39:34.88 +57:01:21.5
129.47652 -5.23610 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 | 01:39:34.88 +57:01:21.5 (user input) | T | P | (position from user input) J-Ks=0.714+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:39:34.88 +57:01:21.5: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:39:34.88 +57:01:21.5: 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 09.4164* 01 39 34.88 +57 01 21.5 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,2461169.9164,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.17 00:46:51.53 +58:59:59.8
122.34100 -3.86655 galactic Cas Second-epoch detections are separated by 2.6" 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 | ATO J011.7264+58.9949 | 00:46:54.46 +59:00:15.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.667+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:46:51.53 +58:59:59.8: 10.92 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:46:51.53 +58:59:59.8: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.21 +/- 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 09.4164* 00 46 51.53 +58 59 59.8 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 J011.7264+58.9949,2461169.9164,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J011.7264+58.9949 20260509.4164 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 09.4164 2461169.9164 10.91 00:53:08.48 +64:49:01.1
123.11323 1.94582 galactic Cas Second-epoch detections are separated by 3.3" 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 | 00:53:08.48 +64:49:01.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:53:08.48 +64:49:01.1: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:53:08.48 +64:49:01.1: 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 09.4164* 00 53 08.48 +64 49 01.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.91 01:11:50.78 +61:46:45.6
125.34243 -0.99686 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 | ZTF J011154.83+614702.6 | 01:11:52.23 +61:46:59.8 (Gaia DR3) | RS (local) | 2458347.97010 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.606+/-0.029 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:50.78 +61:46:45.6: 12.29 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:50.78 +61:46:45.6: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 09.4164* 01 11 50.78 +61 46 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
ZTF J011154.83+614702.6,2461169.9164,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011154.83+614702.6 20260509.4164 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 09.4164 2461169.9164 10.97 02:08:04.25 +58:11:23.1
132.90896 -3.18979 galactic Per Second-epoch detections are separated by 2.2" and 3.3 pix
The object was found in VSX18" Gaia DR3 506740243256446976
Type: RS
# Max. Min./Amp. JD0 Period
14.640 G 14.830 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:08:04.25 +58:11:23.1: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:08:04.25 +58:11:23.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 09.4164* 02 08 04.25 +58 11 23.1 11.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506740243256446976,2461169.9164,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506740243256446976 20260509.4164 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.86 02:18:03.99 +56:20:30.9
134.77203 -4.52537 galactic Per Second-epoch detections are separated by 0.7" and 3.3 pix
The object was found in VSX17" Gaia DR3 458312837728023552
Type: ROT
# Max. Min./Amp. JD0 Period
13.230 G 13.250 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:03.99 +56:20:30.9: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:03.99 +56:20:30.9: 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 09.4164* 02 18 03.99 +56 20 30.9 10.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458312837728023552,2461169.9164,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458312837728023552 20260509.4164 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.83 00:51:14.86 +61:05:30.2
122.90891 -1.78002 galactic Cas Second-epoch detections are separated by 2.4" 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 | Gaia DR3 427312893348808576 | 00:51:15.83 +61:05:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.483+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:14.86 +61:05:30.2: 11.34 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:14.86 +61:05:30.2: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 51 14.86 +61 05 30.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 427312893348808576,2461169.9164,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427312893348808576 20260509.4164 10.83CV 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 09.4164 2461169.9164 10.85 01:29:58.56 +63:18:25.9
127.24389 0.75855 galactic Cas Second-epoch detections are separated by 0.7" and 3.3 pix
The object was found in VSX 7" ZTF J012958.72+631832.5
Type: EA
# Max. Min./Amp. JD0 Period
17.643 r Y 0.267 r 2458434.70710 1.028084700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:58.56 +63:18:25.9: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:58.56 +63:18:25.9: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 29 58.56 +63 18 25.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J012958.72+631832.5,2461169.9164,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J012958.72+631832.5 20260509.4164 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 09.4164 2461169.9164 10.71 02:08:50.87 +57:39:27.2
133.16450 -3.66813 galactic Per Second-epoch detections are separated by 0.9" and 3.3 pix
The object was found in VSX 1" Gaia DR3 505172648911815424
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.370 G 13.410 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:08:50.87 +57:39:27.2: 13.05 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:08:50.87 +57:39:27.2: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 08 50.87 +57 39 27.2 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505172648911815424,2461169.9164,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505172648911815424 20260509.4164 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 09.4164 2461169.9164 10.52 02:46:16.46 +65:01:23.9
134.67643 4.80356 galactic Cas Second-epoch detections are separated by 4.6" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:46:16.46 +65:01:23.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:46:16.46 +65:01:23.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:46:16.46 +65:01:23.9: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 46 16.46 +65 01 23.9 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,2461169.9164,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.73 02:31:03.24 +56:42:27.2
136.32271 -3.55188 galactic Per Second-epoch detections are separated by 3.1" 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 | Gaia DR3 457588774957846528 | 02:31:06.74 +56:42:22.1 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.760+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:03.24 +56:42:27.2: 12.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:03.24 +56:42:27.2: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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 09.4164* 02 31 03.24 +56 42 27.2 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457588774957846528,2461169.9164,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457588774957846528 20260509.4164 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 09.4164 2461169.9164 10.88 01:02:12.18 +57:26:33.6
124.38628 -5.39868 galactic Cas Second-epoch detections are separated by 2.3" 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 | 01:02:12.18 +57:26:33.6 (user input) | T | P | (position from user input) SpType: A2V (LAMOST DR5) J-Ks=0.395+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:12.18 +57:26:33.6: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:12.18 +57:26:33.6: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 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 09.4164* 01 02 12.18 +57 26 33.6 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
target,2461169.9164,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.85 01:11:44.80 +61:13:57.3
125.37377 -1.54284 galactic Cas Second-epoch detections are separated by 0.6" and 3.2 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:44.80 +61:13:57.3: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:44.80 +61:13:57.3: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 09.4164* 01 11 44.80 +61 13 57.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011144.73+611356.9,2461169.9164,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011144.73+611356.9 20260509.4164 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 09.4164 2461169.9164 10.87 00:49:39.69 +61:23:34.4
122.71921 -1.47813 galactic Cas Second-epoch detections are separated by 2.5" and 3.2 pix
The object was found in VSX 3" Gaia DR3 427389962246234112
Type: VAR
# Max. Min./Amp. JD0 Period
13.870 G 13.900 G 0.025322800000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:49:39.69 +61:23:34.4: 12.16 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:49:39.69 +61:23:34.4: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 49 39.69 +61 23 34.4 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 427389962246234112,2461169.9164,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427389962246234112 20260509.4164 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 09.4164 2461169.9164 10.88 00:47:23.55 +61:04:59.8
122.44267 -1.78463 galactic Cas Second-epoch detections are separated by 2.0" 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 | 00:47:23.55 +61:04:59.8 (user input) | T | P | (position from user input) J-Ks=0.774+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:47:23.55 +61:04:59.8: 12.67 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:47:23.55 +61:04:59.8: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 47 23.55 +61 04 59.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.89 01:35:32.85 +57:32:34.4
128.84488 -4.82158 galactic Cas Second-epoch detections are separated by 2.1" and 3.5 pix
The object was found in VSX16" Gaia DR3 412846623165638144
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.070 G 13.090 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:32.85 +57:32:34.4: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:32.85 +57:32:34.4: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 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 09.4164* 01 35 32.85 +57 32 34.4 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 412846623165638144,2461169.9164,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 412846623165638144 20260509.4164 10.89CV 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 09.4164 2461169.9164 10.98 00:44:21.47 +58:18:53.3
121.99939 -4.54412 galactic Cas Second-epoch detections are separated by 1.6" 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 | ATO J011.1007+58.3220 | 00:44:21.47 +58:18:53.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.447+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:44:21.47 +58:18:53.3: 11.59 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:44:21.47 +58:18:53.3: 13.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 44 21.47 +58 18 53.3 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
ATO J011.1007+58.3220,2461169.9164,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J011.1007+58.3220 20260509.4164 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.04 01:06:13.02 +59:33:47.1
124.80571 -3.25488 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 | 01:06:13.02 +59:33:47.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:06:13.02 +59:33:47.1: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:06:13.02 +59:33:47.1: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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 09.4164* 01 06 13.02 +59 33 47.1 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
target,2461169.9164,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.81 01:13:44.64 +57:24:50.1
125.94490 -5.32728 galactic Cas Second-epoch detections are separated by 2.6" 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 | target | 01:13:44.64 +57:24:50.1 (user input) | T | P | (position from user input) J-Ks=0.655+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:44.64 +57:24:50.1: 13.36 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:44.64 +57:24:50.1: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 13 44.64 +57 24 50.1 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
target,2461169.9164,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.85 00:38:16.23 +61:49:05.9
121.37770 -1.01370 galactic Cas Second-epoch detections are separated by 0.2" 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 | 00:38:16.23 +61:49:05.9 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:38:16.23 +61:49:05.9: 11.52 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:38:16.23 +61:49:05.9: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 09.4164* 00 38 16.23 +61 49 05.9 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,2461169.9164,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.88 01:30:26.42 +58:11:55.8
128.06665 -4.28354 galactic Cas Second-epoch detections are separated by 0.4" 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 J022.6239+58.1973 | 01:30:26.42 +58:11:55.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.184+/-0.041 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:30:26.42 +58:11:55.8: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:30:26.42 +58:11:55.8: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 30 26.42 +58 11 55.8 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.6239+58.1973,2461169.9164,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.6239+58.1973 20260509.4164 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 09.4164 2461169.9164 10.82 01:02:05.20 +57:40:27.8
124.36091 -5.16781 galactic Cas Second-epoch detections are separated by 2.3" 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 | Large-amplitude variable Gaia DR2 424111600829561472 | 01:02:00.81 +57:40:18.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.312+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:05.20 +57:40:27.8: 11.82 +/- 0.10 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:05.20 +57:40:27.8: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 02 05.20 +57 40 27.8 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
Large-amplitude variable Gaia DR2 424111600829561472,2461169.9164,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 424111600829561472 20260509.4164 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 09.4164 2461169.9164 10.87 01:50:50.32 +57:13:03.4
130.93598 -4.72814 galactic Per Second-epoch detections are separated by 6.0" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 505701307844350336 | 01:50:48.01 +57:13:07.8 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:50.32 +57:13:03.4: 12.93 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:50.32 +57:13:03.4: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 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 09.4164* 01 50 50.32 +57 13 03.4 10.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505701307844350336,2461169.9164,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505701307844350336 20260509.4164 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 09.4164 2461169.9164 10.71 00:41:02.79 +63:36:12.4
121.77718 0.75500 galactic Cas Second-epoch detections are separated by 1.7" and 3.2 pix
The object was found in VSX19" Gaia DR3 523926572070113664
Type: VAR
# Max. Min./Amp. JD0 Period
13.420 G 13.460 G 0.018320000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:41:02.79 +63:36:12.4: 12.61 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:41:02.79 +63:36:12.4: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 41 02.79 +63 36 12.4 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
Gaia DR3 523926572070113664,2461169.9164,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523926572070113664 20260509.4164 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 09.4164 2461169.9164 10.88 01:35:27.63 +60:33:46.7
128.31835 -1.84756 galactic Cas Second-epoch detections are separated by 2.5" 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 | Gaia DR3 509811625915787136 | 01:35:29.25 +60:33:31.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.155+/-0.047 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:27.63 +60:33:46.7: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:27.63 +60:33:46.7: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 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 09.4164* 01 35 27.63 +60 33 46.7 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 509811625915787136,2461169.9164,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509811625915787136 20260509.4164 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 09.4164 2461169.9164 10.78 02:10:55.92 +62:17:08.9
132.02923 0.82641 galactic Cas Second-epoch detections are separated by 2.6" and 3.5 pix
The object was found in VSX 3" ASASSN-V J021056.24+621707.7
Type: SR
# Max. Min./Amp. JD0 Period
13.610 V 13.700 V 2457406.80000 41.140000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:55.92 +62:17:08.9: 13.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:55.92 +62:17:08.9: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 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 09.4164* 02 10 55.92 +62 17 08.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J021056.24+621707.7,2461169.9164,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J021056.24+621707.7 20260509.4164 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
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.59 02:25:34.99 +57:05:41.3
135.48439 -3.46469 galactic Per Second-epoch detections are separated by 2.0" and 3.1 pix
The object was found in VSX17" Gaia DR3 458417699341569920
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.030 G 13.070 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:25:34.99 +57:05:41.3: 11.50 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:25:34.99 +57:05:41.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 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 09.4164* 02 25 34.99 +57 05 41.3 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458417699341569920,2461169.9164,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458417699341569920 20260509.4164 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 09.4164 2461169.9164 10.76 01:50:40.43 +57:43:29.4
130.79809 -4.23940 galactic Per Second-epoch detections are separated by 4.4" and 3.6 pix
The object was found in VSX19" ZTF J015042.79+574332.6
Type: RS
# Max. Min./Amp. JD0 Period
15.382 r Y 0.115 r 2458299.92130 0.271638100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:50:40.43 +57:43:29.4: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:50:40.43 +57:43:29.4: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 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 09.4164* 01 50 40.43 +57 43 29.4 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J015042.79+574332.6,2461169.9164,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J015042.79+574332.6 20260509.4164 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.67 01:31:23.18 +59:33:44.1
127.97888 -2.91747 galactic Cas Second-epoch detections are separated by 0.7" 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 | ATO J022.8294+59.5638 | 01:31:23.18 +59:33:44.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.833+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:23.18 +59:33:44.1: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:23.18 +59:33:44.1: 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 09.4164* 01 31 23.18 +59 33 44.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J022.8294+59.5638,2461169.9164,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J022.8294+59.5638 20260509.4164 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.66 00:53:53.44 +63:42:25.3
123.20356 0.83657 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 | 00:53:53.44 +63:42:25.3 (user input) | T | P | (position from user input) J-Ks=0.213+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:53:53.44 +63:42:25.3: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:53:53.44 +63:42:25.3: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 53 53.44 +63 42 25.3 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.78 00:36:46.02 +61:48:23.6
121.19975 -1.01584 galactic Cas Second-epoch detections are separated by 2.8" and 3.3 pix
The object was found in VSX 8" Gaia DR3 430273848108689536
Type: S
# Max. Min./Amp. JD0 Period
16.890 G 17.860 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:36:46.02 +61:48:23.6: 13.10 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:36:46.02 +61:48:23.6: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 36 46.02 +61 48 23.6 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 430273848108689536,2461169.9164,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430273848108689536 20260509.4164 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
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.90 00:59:54.65 +59:58:35.3
123.99294 -2.87782 galactic Cas Second-epoch detections are separated by 2.1" and 3.0 pix
The object was found in VSX20" Gaia DR3 426442668565974400
Type: S
# Max. Min./Amp. JD0 Period
17.270 G 18.430 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:59:54.65 +59:58:35.3: 12.56 +/- 0.19 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:59:54.65 +59:58:35.3: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 09.4164* 00 59 54.65 +59 58 35.3 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 426442668565974400,2461169.9164,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426442668565974400 20260509.4164 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.79 00:53:44.86 +60:23:25.2
123.21749 -2.48013 galactic Cas Second-epoch detections are separated by 2.3" and 2.9 pix
The object was found in VSX17" CzeV3004
Type: DSCT
# Max. Min./Amp. JD0 Period
12.950 V 12.990 V 2459062.48000 0.119600000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:53:44.86 +60:23:25.2: 10.72 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:53:44.86 +60:23:25.2: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.15 +/- 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 09.4164* 00 53 44.86 +60 23 25.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CzeV3004,2461169.9164,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CzeV3004 20260509.4164 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 09.4164 2461169.9164 10.63 01:32:21.95 +60:27:29.1
127.95968 -2.01352 galactic Cas Second-epoch detections are separated by 0.8" 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 | 01:32:21.95 +60:27:29.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:21.95 +60:27:29.1: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:21.95 +60:27:29.1: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 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 09.4164* 01 32 21.95 +60 27 29.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.64 00:51:03.58 +65:42:57.2
122.89298 2.84417 galactic Cas Second-epoch detections are separated by 1.9" 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 | 00:51:03.58 +65:42:57.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:03.58 +65:42:57.2: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:03.58 +65:42:57.2: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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 09.4164* 00 51 03.58 +65 42 57.2 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.67 00:51:29.89 +65:11:40.6
122.93824 2.32286 galactic Cas Second-epoch detections are separated by 1.6" and 3.0 pix
The object was found in VSX 4" Gaia DR3 524535598429383296
Type: VAR
# Max. Min./Amp. JD0 Period
13.230 G 13.250 G 0.573260000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:29.89 +65:11:40.6: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:29.89 +65:11:40.6: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 51 29.89 +65 11 40.6 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 524535598429383296,2461169.9164,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524535598429383296 20260509.4164 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.84 00:51:33.76 +58:43:24.3
122.94815 -4.14833 galactic Cas Second-epoch detections are separated by 1.1" 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 | 00:51:33.76 +58:43:24.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.391+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:33.76 +58:43:24.3: 11.86 +/- 0.11 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:33.76 +58:43:24.3: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 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 09.4164* 00 51 33.76 +58 43 24.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.71 01:44:30.72 +57:38:51.1
130.00863 -4.49315 galactic Cas Second-epoch detections are separated by 2.3" 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 J026.1317+57.6497 | 01:44:33.13 +57:38:39.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.467+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:30.72 +57:38:51.1: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:30.72 +57:38:51.1: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 44 30.72 +57 38 51.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.1317+57.6497,2461169.9164,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.1317+57.6497 20260509.4164 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 09.4164 2461169.9164 10.49 02:04:04.10 +64:05:48.9
130.76280 2.33501 galactic Cas Second-epoch detections are separated by 1.9" 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 514956928010863872 | 02:03:58.86 +64:06:01.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.391+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:04:04.10 +64:05:48.9: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:04:04.10 +64:05:48.9: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 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 09.4164* 02 04 04.10 +64 05 48.9 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 514956928010863872,2461169.9164,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 514956928010863872 20260509.4164 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.63 01:07:34.08 +60:52:43.7
124.89426 -1.93147 galactic Cas Second-epoch detections are separated by 0.6" 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 426412500712083840 | 01:07:34.56 +60:53:29.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5: 1935BSD...C01....0S BSD 8-1112 J-Ks=0.814+/-0.029 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:34.08 +60:52:43.7: 13.10 +/- 0.31 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:34.08 +60:52:43.7: 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 09.4164* 01 07 34.08 +60 52 43.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426412500712083840,2461169.9164,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426412500712083840 20260509.4164 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 09.4164 2461169.9164 10.78 01:03:21.67 +58:04:37.8
124.51304 -4.75797 galactic Cas Second-epoch detections are separated by 0.3" 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 | 01:03:21.67 +58:04:37.8 (user input) | T | P | (position from user input) J-Ks=0.497+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:03:21.67 +58:04:37.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:03:21.67 +58:04:37.8: 13.42 +/- 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 09.4164* 01 03 21.67 +58 04 37.8 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,2461169.9164,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.60 00:54:13.13 +64:20:25.0
123.23306 1.47016 galactic Cas Second-epoch detections are separated by 2.6" and 3.2 pix
The object was found in VSX23" Gaia DR3 524205538785900800
Type: ROT
# Max. Min./Amp. JD0 Period
15.520 G 15.560 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:54:13.13 +64:20:25.0: 12.70 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:54:13.13 +64:20:25.0: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 09.4164* 00 54 13.13 +64 20 25.0 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 524205538785900800,2461169.9164,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524205538785900800 20260509.4164 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.64 01:42:44.36 +58:39:03.4
129.57639 -3.55741 galactic Cas Second-epoch detections are separated by 3.0" 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 | Gaia DR3 506082013747225856 | 01:42:46.84 +58:39:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=12.323+/- (unrealisitic color!)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:42:44.36 +58:39:03.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:42:44.36 +58:39:03.4: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 09.4164* 01 42 44.36 +58 39 03.4 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 506082013747225856,2461169.9164,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506082013747225856 20260509.4164 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.67 00:54:30.87 +59:24:00.8
123.32415 -3.46918 galactic Cas Second-epoch detections are separated by 1.9" and 3.4 pix
The object was found in VSX 2" V0415 Cas
Type: EA/DS
# Max. Min./Amp. JD0 Period
14.000 pg 16.800 pg 2429106.58700 12.536157000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:54:30.87 +59:24:00.8: 11.65 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:54:30.87 +59:24:00.8: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 09.4164* 00 54 30.87 +59 24 00.8 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0415 Cas,2461169.9164,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0415 Cas 20260509.4164 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.60 00:45:45.53 +59:54:30.7
122.21918 -2.95536 galactic Cas Second-epoch detections are separated by 1.5" 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 | 00:45:45.53 +59:54:30.7 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:45:45.53 +59:54:30.7: 11.37 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:45:45.53 +59:54:30.7: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 45 45.53 +59 54 30.7 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.55 00:58:15.67 +62:45:20.2
123.71273 -0.10579 galactic Cas Second-epoch detections are separated by 5.2" and 3.9 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 523684816952461824 | 00:58:19.12 +62:45:50.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:58:15.67 +62:45:20.2: 12.26 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:58:15.67 +62:45:20.2: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 58 15.67 +62 45 20.2 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 523684816952461824,2461169.9164,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523684816952461824 20260509.4164 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.69 01:19:24.09 +58:26:40.3
126.59380 -4.22826 galactic Cas Second-epoch detections are separated by 1.5" 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 | Gaia DR3 413883771873740416 | 01:19:25.94 +58:26:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1951UppAn...2j...1B NGC 457 191 J-Ks=0.329+/-0.040 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:24.09 +58:26:40.3: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:24.09 +58:26:40.3: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 19 24.09 +58 26 40.3 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 413883771873740416,2461169.9164,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413883771873740416 20260509.4164 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 09.4164 2461169.9164 10.53 01:32:19.13 +59:45:28.6
128.06470 -2.70577 galactic Cas Second-epoch detections are separated by 0.7" and 3.1 pix
The object was found in VSX20" ZTF J013221.77+594532.2
Type: SR
# Max. Min./Amp. JD0 Period
12.583 r Y 0.243 r 2458304.52380 52.926856300000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:32:19.13 +59:45:28.6: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:32:19.13 +59:45:28.6: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 09.4164* 01 32 19.13 +59 45 28.6 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J013221.77+594532.2,2461169.9164,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J013221.77+594532.2 20260509.4164 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 09.4164 2461169.9164 10.61 01:17:48.27 +57:17:35.5
126.50393 -5.39557 galactic Cas Second-epoch detections are separated by 2.5" 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 | 01:17:48.27 +57:17:35.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:48.27 +57:17:35.5: 12.90 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:48.27 +57:17:35.5: 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 09.4164* 01 17 48.27 +57 17 35.5 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.45 01:29:33.76 +57:55:08.9
127.99347 -4.57745 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 | target | 01:29:33.76 +57:55:08.9 (user input) | T | P | (position from user input) J-Ks=0.764+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:33.76 +57:55:08.9: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:33.76 +57:55:08.9: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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 09.4164* 01 29 33.76 +57 55 08.9 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,2461169.9164,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.27 01:38:10.65 +60:44:57.1
128.61359 -1.60591 galactic Cas Second-epoch detections are separated by 6.2" and 4.0 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 | 01:38:10.65 +60:44:57.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:10.65 +60:44:57.1: 11.79 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:10.65 +60:44:57.1: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 38 10.65 +60 44 57.1 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.44 01:25:15.49 +64:40:35.1
126.53996 2.04186 galactic Cas Second-epoch detections are separated by 2.5" 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 | Gaia DR3 512840196327698304 | 01:25:16.38 +64:40:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:15.49 +64:40:35.1: 10.93 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:15.49 +64:40:35.1: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 25 15.49 +64 40 35.1 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 512840196327698304,2461169.9164,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512840196327698304 20260509.4164 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.62 01:00:37.27 +58:32:33.2
124.13318 -4.30777 galactic Cas Second-epoch detections are separated by 2.3" and 3.4 pix
The object was found in VSX21" Gaia DR3 425716814782580736
Type: E
# Max. Min./Amp. JD0 Period
18.810 G 19.180 G 1.201470000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:00:37.27 +58:32:33.2: 12.73 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:00:37.27 +58:32:33.2: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 00 37.27 +58 32 33.2 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 425716814782580736,2461169.9164,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425716814782580736 20260509.4164 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 09.4164 2461169.9164 10.66 00:51:09.10 +60:42:14.5
122.89688 -2.16770 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 | 00:51:09.10 +60:42:14.5 (user input) | T | P | (position from user input) J-Ks=0.802+/-0.033 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:09.10 +60:42:14.5: 11.18 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:09.10 +60:42:14.5: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.70 +/- 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 09.4164* 00 51 09.10 +60 42 14.5 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,2461169.9164,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.46 02:04:10.77 +57:54:39.3
132.49444 -3.60395 galactic Per Second-epoch detections are separated by 6.9" and 2.3 pix
The object was found in VSX 0" Gaia DR3 505424574514826112
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.890 G 13.920 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:04:10.77 +57:54:39.3: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:04:10.77 +57:54:39.3: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 09.4164* 02 04 10.77 +57 54 39.3 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505424574514826112,2461169.9164,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505424574514826112 20260509.4164 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.53 01:14:22.29 +57:12:42.3
126.04756 -5.52120 galactic Cas Second-epoch detections are separated by 1.0" 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 413340888006548224 | 01:14:21.96 +57:13:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.364+/-0.036 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:22.29 +57:12:42.3: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:22.29 +57:12:42.3: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 14 22.29 +57 12 42.3 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 413340888006548224,2461169.9164,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413340888006548224 20260509.4164 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 09.4164 2461169.9164 10.46 01:03:35.50 +60:28:06.7
124.43032 -2.36786 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 | Gaia DR3 426387242001692800 | 01:03:37.95 +60:27:48.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.438+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:03:35.50 +60:28:06.7: 11.22 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:03:35.50 +60:28:06.7: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.68 +/- 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 09.4164* 01 03 35.50 +60 28 06.7 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426387242001692800,2461169.9164,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426387242001692800 20260509.4164 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.43 00:50:30.95 +58:09:49.1
122.80991 -4.70789 galactic Cas Second-epoch detections are separated by 2.5" 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 | ATO J012.6311+58.1683 | 00:50:31.48 +58:10:06.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=12.129+/- (unrealisitic color!)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:50:30.95 +58:09:49.1: 11.05 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:50:30.95 +58:09:49.1: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 50 30.95 +58 09 49.1 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
ATO J012.6311+58.1683,2461169.9164,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J012.6311+58.1683 20260509.4164 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.46 00:47:11.40 +58:35:25.7
122.37694 -4.27670 galactic Cas Second-epoch detections are separated by 1.5" and 3.3 pix
The object was found in VSX 1" ASASSN-V J004711.30+583525.0
Type: L
# Max. Min./Amp. JD0 Period
12.500 V 12.620 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:47:11.40 +58:35:25.7: 10.52 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:47:11.40 +58:35:25.7: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.04 +/- 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 09.4164* 00 47 11.40 +58 35 25.7 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
ASASSN-V J004711.30+583525.0,2461169.9164,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J004711.30+583525.0 20260509.4164 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.39 02:11:52.89 +59:02:30.7
133.12747 -2.22825 galactic Per Second-epoch detections are separated by 2.7" 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 | NSVS J0211521+590234 | 02:11:50.43 +59:02:57.3 (Gaia DR3) | SR (local) | 2458346.14140 (local) | Gaia3var=VARIABLE J-Ks=0.249+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:52.89 +59:02:30.7: 13.35 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:52.89 +59:02:30.7: 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 09.4164* 02 11 52.89 +59 02 30.7 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0211521+590234,2461169.9164,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0211521+590234 20260509.4164 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.53 01:02:45.68 +58:39:34.8
124.40779 -4.17963 galactic Cas Second-epoch detections are separated by 0.7" and 3.1 pix
The object was found in VSX21" Gaia DR3 425802855871731072
Type: ROT
# Max. Min./Amp. JD0 Period
12.620 G 12.680 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:02:45.68 +58:39:34.8: 12.45 +/- 0.18 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:02:45.68 +58:39:34.8: 13.26 +/- 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 09.4164* 01 02 45.68 +58 39 34.8 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 425802855871731072,2461169.9164,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425802855871731072 20260509.4164 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 09.4164 2461169.9164 10.30 01:01:40.14 +64:15:03.0
124.04313 1.40116 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 | target | 01:01:40.14 +64:15:03.0 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:40.14 +64:15:03.0: 13.01 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:01:40.14 +64:15:03.0: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 01 40.14 +64 15 03.0 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.52 00:53:20.61 +57:37:02.3
123.18814 -5.25350 galactic Cas Second-epoch detections are separated by 0.9" and 3.3 pix
The object was found in VSX13" ZTF J005322.19+573659.0
Type: RS
# Max. Min./Amp. JD0 Period
16.767 r Y 0.067 r 2458307.84470 3.956748100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:53:20.61 +57:37:02.3: 11.80 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:53:20.61 +57:37:02.3: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 53 20.61 +57 37 02.3 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J005322.19+573659.0,2461169.9164,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J005322.19+573659.0 20260509.4164 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.36 01:03:04.31 +57:50:55.9
124.48508 -4.98780 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 | ATO J015.7670+57.8507 | 01:03:06.70 +57:50:48.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F4 (LAMOST DR5) J-Ks=0.294+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:03:04.31 +57:50:55.9: 10.19 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:03:04.31 +57:50:55.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.52 +/- 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 09.4164* 01 03 04.31 +57 50 55.9 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 J015.7670+57.8507,2461169.9164,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J015.7670+57.8507 20260509.4164 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.17 01:45:34.97 +59:18:10.9
129.80293 -2.84448 galactic Cas Second-epoch detections are separated by 2.2" 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 | ATO J026.3995+59.3029 | 01:45:34.97 +59:18:10.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:45:34.97 +59:18:10.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:45:34.97 +59:18:10.9: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 45 34.97 +59 18 10.9 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.3995+59.3029,2461169.9164,10.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.3995+59.3029 20260509.4164 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.43 01:03:02.73 +58:09:40.5
124.46739 -4.67589 galactic Cas Second-epoch detections are separated by 0.5" and 3.2 pix
The object was found in VSX 1" Gaia DR3 425648855524364544
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.250 G 13.280 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:03:02.73 +58:09:40.5: 13.06 +/- 0.30 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:03:02.73 +58:09:40.5: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 09.4164* 01 03 02.73 +58 09 40.5 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 425648855524364544,2461169.9164,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 425648855524364544 20260509.4164 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.44 01:27:35.64 +57:56:59.8
127.72963 -4.58461 galactic Cas Second-epoch detections are separated by 1.9" 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 | Gaia DR3 413090817828281216 | 01:27:33.40 +57:56:56.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.205+/-0.038 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:27:35.64 +57:56:59.8: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:27:35.64 +57:56:59.8: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 27 35.64 +57 56 59.8 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 413090817828281216,2461169.9164,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413090817828281216 20260509.4164 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.25 01:46:34.07 +59:44:09.6
129.83398 -2.39492 galactic Cas Second-epoch detections are separated by 0.8" 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 | 01:46:34.07 +59:44:09.6 (user input) | T | P | (position from user input) J-Ks=1.005+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:34.07 +59:44:09.6: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:34.07 +59:44:09.6: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 46 34.07 +59 44 09.6 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.29 00:52:55.23 +58:28:51.8
123.12625 -4.39013 galactic Cas Second-epoch detections are separated by 1.8" 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 | ATO J013.2201+58.4812 | 00:52:55.23 +58:28:51.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.367+/-0.026 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:55.23 +58:28:51.8: 11.42 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:55.23 +58:28:51.8: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 52 55.23 +58 28 51.8 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J013.2201+58.4812,2461169.9164,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J013.2201+58.4812 20260509.4164 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.13 01:25:38.40 +59:16:00.1
127.29691 -3.31488 galactic Cas Second-epoch detections are separated by 1.6" 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 | Gaia DR3 510043588502369152 | 01:25:40.25 +59:16:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.017+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:38.40 +59:16:00.1: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:38.40 +59:16:00.1: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 09.4164* 01 25 38.40 +59 16 00.1 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510043588502369152,2461169.9164,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510043588502369152 20260509.4164 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.10 01:49:03.59 +61:04:33.8
129.84377 -1.02005 galactic Cas Second-epoch detections are separated by 0.8" 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 | 01:49:03.59 +61:04:33.8 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:49:03.59 +61:04:33.8: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:49:03.59 +61:04:33.8: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 09.4164* 01 49 03.59 +61 04 33.8 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.14 01:11:16.06 +61:08:30.1
125.32329 -1.63795 galactic Cas Second-epoch detections are separated by 0.1" and 3.1 pix
The object was found in VSX14" ZTF J011114.91+610818.6
Type: RS
# Max. Min./Amp. JD0 Period
13.623 g Y 0.083 g 2458358.91940 0.779401400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:16.06 +61:08:30.1: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:16.06 +61:08:30.1: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 11 16.06 +61 08 30.1 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011114.91+610818.6,2461169.9164,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011114.91+610818.6 20260509.4164 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.12 00:51:25.61 +62:25:15.4
122.93063 -0.45080 galactic Cas Second-epoch detections are separated by 1.9" 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 | Gaia DR3 427541664790555008 | 00:51:25.03 +62:25:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=11.642+/- (unrealisitic color!)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:25.61 +62:25:15.4: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:25.61 +62:25:15.4: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 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 09.4164* 00 51 25.61 +62 25 15.4 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 427541664790555008,2461169.9164,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427541664790555008 20260509.4164 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.26 00:56:45.56 +58:52:45.9
123.62112 -3.98521 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 | ATO J014.1841+58.8773 | 00:56:42.26 +58:52:33.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.476+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:56:45.56 +58:52:45.9: 11.54 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:56:45.56 +58:52:45.9: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 09.4164* 00 56 45.56 +58 52 45.9 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J014.1841+58.8773,2461169.9164,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J014.1841+58.8773 20260509.4164 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.13 01:01:40.03 +58:50:24.2
124.25806 -4.00535 galactic Cas Second-epoch detections are separated by 1.1" 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 | ATO J015.4178+58.8525 | 01:01:40.03 +58:50:24.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.770+/-0.026 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:40.03 +58:50:24.2: 12.87 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:01:40.03 +58:50:24.2: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 01 40.03 +58 50 24.2 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J015.4178+58.8525,2461169.9164,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J015.4178+58.8525 20260509.4164 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.07 01:25:26.55 +60:57:45.1
127.04831 -1.63715 galactic Cas Second-epoch detections are separated by 0.5" 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 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:26.55 +60:57:45.1: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:26.55 +60:57:45.1: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 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 09.4164* 01 25 26.55 +60 57 45.1 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510670688089089920,2461169.9164,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510670688089089920 20260509.4164 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.16 01:01:25.47 +57:50:13.8
124.26574 -5.00872 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 | ATO J015.3611+57.8296 | 01:01:25.47 +57:50:13.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.462+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:25.47 +57:50:13.8: 10.72 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:01:25.47 +57:50:13.8: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.30 +/- 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 09.4164* 01 01 25.47 +57 50 13.8 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J015.3611+57.8296,2461169.9164,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J015.3611+57.8296 20260509.4164 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.98 02:22:36.82 +56:49:53.5
135.19716 -3.85321 galactic Per Second-epoch detections are separated by 1.3" 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 458305789673621888 | 02:22:39.30 +56:49:47.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.083+/-0.033 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:22:36.82 +56:49:53.5: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:22:36.82 +56:49:53.5: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 22 36.82 +56 49 53.5 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458305789673621888,2461169.9164,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458305789673621888 20260509.4164 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.83 02:26:52.85 +57:11:10.4
135.61619 -3.31627 galactic Per 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 457675155341434496 | 02:26:50.90 +57:11:15.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=11.821+/- (unrealisitic color!)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:52.85 +57:11:10.4: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:52.85 +57:11:10.4: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 26 52.85 +57 11 10.4 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457675155341434496,2461169.9164,9.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457675155341434496 20260509.4164 9.83CV 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 09.4164 2461169.9164 10.16 00:40:25.93 +61:07:16.2
121.60288 -1.72218 galactic Cas Second-epoch detections are separated by 2.3" 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 | Gaia DR3 427219056906089600 | 00:40:25.71 +61:07:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:40:25.93 +61:07:16.2: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:40:25.93 +61:07:16.2: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 40 25.93 +61 07 16.2 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 427219056906089600,2461169.9164,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427219056906089600 20260509.4164 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.94 01:53:47.19 +60:15:59.3
130.59370 -1.67450 galactic Cas Second-epoch detections are separated by 0.5" 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 508091916700729984 | 01:53:49.28 +60:16:10.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5 1955ApJS....2..123F LF 5 +60 340 J-Ks=0.162+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:53:47.19 +60:15:59.3: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:53:47.19 +60:15:59.3: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 09.4164* 01 53 47.19 +60 15 59.3 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 508091916700729984,2461169.9164,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508091916700729984 20260509.4164 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.06 00:51:21.61 +57:15:53.7
122.92136 -5.60683 galactic Cas Second-epoch detections are separated by 1.1" 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 424260859533890432 | 00:51:20.27 +57:16:10.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.276+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:21.61 +57:15:53.7: 11.46 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:21.61 +57:15:53.7: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 51 21.61 +57 15 53.7 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 424260859533890432,2461169.9164,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424260859533890432 20260509.4164 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.89 01:35:23.69 +60:39:00.6
128.29559 -1.76300 galactic Cas Second-epoch detections are separated by 0.5" and 3.3 pix
The object was found in VSX23" 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:23.69 +60:39:00.6: 12.39 +/- 0.16 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:23.69 +60:39:00.6: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 35 23.69 +60 39 00.6 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 509819081975016960,2461169.9164,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509819081975016960 20260509.4164 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 09.4164 2461169.9164 9.97 00:55:44.64 +58:25:59.4
123.49714 -4.43386 galactic Cas Second-epoch detections are separated by 0.3" and 3.2 pix
The object was found in VSX22" Gaia DR3 424392354251757184
Type: ROT
# Max. Min./Amp. JD0 Period
16.840 G 16.900 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:55:44.64 +58:25:59.4: 11.57 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:55:44.64 +58:25:59.4: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 55 44.64 +58 25 59.4 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 424392354251757184,2461169.9164,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424392354251757184 20260509.4164 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.87 01:28:26.73 +60:23:26.9
127.49129 -2.15292 galactic Cas Second-epoch detections are separated by 0.6" 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 | Gaia DR3 510221984265315200 | 01:28:28.01 +60:23:13.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.247+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:26.73 +60:23:26.9: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:26.73 +60:23:26.9: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 28 26.73 +60 23 26.9 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 510221984265315200,2461169.9164,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510221984265315200 20260509.4164 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.05 00:58:00.34 +57:24:03.5
123.82047 -5.45945 galactic Cas Second-epoch detections are separated by 2.1" 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 | Gaia DR3 424135377769652480 | 00:58:01.55 +57:24:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:58:00.34 +57:24:03.5: 12.31 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:58:00.34 +57:24:03.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 09.4164* 00 58 00.34 +57 24 03.5 10.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 424135377769652480,2461169.9164,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424135377769652480 20260509.4164 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.01 00:50:57.59 +60:47:11.6
122.87354 -2.08514 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 | Gaia DR3 427301627662163584 | 00:50:57.08 +60:47:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.427+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:50:57.59 +60:47:11.6: 10.68 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:50:57.59 +60:47:11.6: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 50 57.59 +60 47 11.6 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 427301627662163584,2461169.9164,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427301627662163584 20260509.4164 10.01CV 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 09.4164 2461169.9164 9.72 00:36:43.22 +64:22:48.1
121.34125 1.55374 galactic Cas Second-epoch detections are separated by 2.0" 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 | Large-amplitude variable Gaia DR2 526988333994584448 | 00:36:41.83 +64:22:31.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.519+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:36:43.22 +64:22:48.1: 12.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:36:43.22 +64:22:48.1: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 36 43.22 +64 22 48.1 9.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 526988333994584448,2461169.9164,9.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 526988333994584448 20260509.4164 9.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.62 02:31:49.82 +56:26:31.7
136.52218 -3.75742 galactic Per Second-epoch detections are separated by 0.6" 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 | Gaia DR3 457393336767227264 | 02:31:45.96 +56:26:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.145+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:49.82 +56:26:31.7: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:49.82 +56:26:31.7: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 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 09.4164* 02 31 49.82 +56 26 31.7 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457393336767227264,2461169.9164,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457393336767227264 20260509.4164 9.62CV 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 09.4164 2461169.9164 9.76 00:52:48.90 +64:02:29.2
123.08264 1.17010 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 | Gaia DR3 523820091239115264 | 00:52:49.26 +64:02:44.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.437+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:48.90 +64:02:29.2: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:48.90 +64:02:29.2: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 52 48.90 +64 02 29.2 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 523820091239115264,2461169.9164,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523820091239115264 20260509.4164 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.76 01:20:24.34 +59:10:25.1
126.64256 -3.48925 galactic Cas Second-epoch detections are separated by 0.5" 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 J020.1204+59.1623 | 01:20:25.01 +59:10:05.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.296+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:20:24.34 +59:10:25.1: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:20:24.34 +59:10:25.1: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 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 09.4164* 01 20 24.34 +59 10 25.1 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J020.1204+59.1623,2461169.9164,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J020.1204+59.1623 20260509.4164 9.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.39 01:52:09.01 +58:27:40.6
130.81800 -3.47782 galactic Cas Second-epoch detections are separated by 1.3" 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 506205674446445952 | 01:52:09.03 +58:27:25.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.384+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:09.01 +58:27:40.6: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:09.01 +58:27:40.6: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 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 09.4164* 01 52 09.01 +58 27 40.6 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506205674446445952,2461169.9164,9.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506205674446445952 20260509.4164 9.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.47 00:52:40.01 +60:08:46.7
123.08502 -2.72508 galactic Cas Second-epoch detections are separated by 1.2" 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 | Gaia DR3 426893399610150016 | 00:52:39.46 +60:09:00.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9 1935BSD...C01....0S BSD 8- 299 J-Ks=0.658+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:52:40.01 +60:08:46.7: 10.05 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:52:40.01 +60:08:46.7: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 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 09.4164* 00 52 40.01 +60 08 46.7 9.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426893399610150016,2461169.9164,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426893399610150016 20260509.4164 9.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.39 01:19:47.65 +61:38:29.2
126.29304 -1.04511 galactic Cas Second-epoch detections are separated by 1.3" 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 | Gaia DR3 510901241928240128 | 01:19:47.76 +61:38:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2: 1935BSD...C01....0S BSD 8-1789/90 J-Ks=0.134+/-0.035 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:47.65 +61:38:29.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:47.65 +61:38:29.2: 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 09.4164* 01 19 47.65 +61 38 29.2 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510901241928240128,2461169.9164,9.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510901241928240128 20260509.4164 9.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.40 01:25:56.72 +59:35:11.7
127.29281 -2.99267 galactic Cas Second-epoch detections are separated by 0.3" 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 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:56.72 +59:35:11.7: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:56.72 +59:35:11.7: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 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 09.4164* 01 25 56.72 +59 35 11.7 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510075336901717632,2461169.9164,9.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260509.4164 9.40CV 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 09.4164 2461169.9164 9.19 02:34:02.55 +56:37:43.2
136.73313 -3.46851 galactic Per Second-epoch detections are separated by 0.1" and 3.4 pix
The object was found in VSX11" Gaia DR3 457763322428148096
Type: ROT
# Max. Min./Amp. JD0 Period
15.220 G 15.260 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:02.55 +56:37:43.2: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:02.55 +56:37:43.2: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 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 09.4164* 02 34 02.55 +56 37 43.2 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457763322428148096,2461169.9164,9.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457763322428148096 20260509.4164 9.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.42 01:40:53.21 +57:14:54.4
129.60833 -4.98091 galactic Cas Second-epoch detections are separated by 0.3" 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 | ATO J025.1932+57.2470 | 01:40:51.06 +57:14:52.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.180+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:40:53.21 +57:14:54.4: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:40:53.21 +57:14:54.4: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 40 53.21 +57 14 54.4 9.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.1932+57.2470,2461169.9164,9.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.1932+57.2470 20260509.4164 9.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.19 00:40:25.55 +62:13:05.2
121.64902 -0.62620 galactic Cas Second-epoch detections are separated by 1.3" and 3.0 pix
The object was found in VSX 2" Gaia DR3 427684287760924288
Type: RS
# Max. Min./Amp. JD0 Period
11.860 G 11.940 G O
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:40:25.55 +62:13:05.2: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:40:25.55 +62:13:05.2: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 40 25.55 +62 13 05.2 9.2 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 427684287760924288,2461169.9164,9.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 427684287760924288 20260509.4164 9.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.08 00:54:29.86 +59:30:21.8
123.32074 -3.36338 galactic Cas Second-epoch detections are separated by 1.8" 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 | Gaia DR3 426100376848302720 | 00:54:28.38 +59:30:39.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A6 1935BSD...C01....0S BSD 8- 340 J-Ks=0.375+/-0.040 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:54:29.86 +59:30:21.8: 9.87 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:54:29.86 +59:30:21.8: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.35 +/- 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 09.4164* 00 54 29.86 +59 30 21.8 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 426100376848302720,2461169.9164,9.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426100376848302720 20260509.4164 9.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 7.85 02:36:31.37 +57:11:41.5
136.82404 -2.81512 galactic Per Second-epoch detections are separated by 0.4" 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 | Gaia DR3 457813144048325248 | 02:36:28.37 +57:11:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1928AnHar.100...49C HD 236972 J-Ks=0.092+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:31.37 +57:11:41.5: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:31.37 +57:11:41.5: 10.33 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.33 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 36 31.37 +57 11 41.5 7.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457813144048325248,2461169.9164,7.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457813144048325248 20260509.4164 7.85CV 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 09.4164 2461169.9164 6.56 02:30:45.63 +55:56:53.3
136.57046 -4.27109 galactic Per Second-epoch detections are separated by 0.2" 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 | ATO J037.6912+55.9591 | 02:30:45.71 +55:56:53.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.030+/-0.025 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:45.63 +55:56:53.3: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:45.63 +55:56:53.3: 99.00 +/- 99.00 saturated
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new 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 09.4164* 02 30 45.63 +55 56 53.3 6.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.6912+55.9591,2461169.9164,6.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.6912+55.9591 20260509.4164 6.56CV 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 09.4164 2461169.9164 6.94 02:31:26.25 +55:59:07.8
136.64440 -4.20086 galactic Per Second-epoch detections are separated by 0.7" and 3.5 pix
The object was found in VSX21" Gaia DR3 457343205908261760
Type: ROT
# Max. Min./Amp. JD0 Period
16.250 G 16.350 G 0.771500000000 M
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:26.25 +55:59:07.8: 13.07 +/- 0.34 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:26.25 +55:59:07.8: 9.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.43 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 31 26.25 +55 59 07.8 6.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457343205908261760,2461169.9164,6.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457343205908261760 20260509.4164 6.94CV 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 09.4164 2461169.9164 6.97 02:34:11.08 +55:50:02.2
137.05915 -4.19388 galactic Per Second-epoch detections are separated by 0.1" and 3.6 pix
The object was found in VSX 1" Gaia DR3 457311320070532608
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
9.230 G 9.290 G 0.086248700000 B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:11.08 +55:50:02.2: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:11.08 +55:50:02.2: 9.42 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.42 +/- 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 09.4164* 02 34 11.08 +55 50 02.2 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457311320070532608,2461169.9164,6.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457311320070532608 20260509.4164 6.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 7.05 02:34:34.68 +56:21:56.3
136.90339 -3.68246 galactic Per Second-epoch detections are separated by 0.9" 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 | Gaia DR3 457749475453771648 | 02:34:34.64 +56:21:57.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.152+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:34.68 +56:21:56.3: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:34.68 +56:21:56.3: 9.57 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.57 +/- 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 09.4164* 02 34 34.68 +56 21 56.3 7.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457749475453771648,2461169.9164,7.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457749475453771648 20260509.4164 7.05CV 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 09.4164 2461169.9164 7.16 02:34:44.54 +56:06:08.1
137.02697 -3.91631 galactic Per Second-epoch detections are separated by 0.0" 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 | ATO J038.6785+56.0961 | 02:34:44.47 +56:06:09.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.215+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:44.54 +56:06:08.1: 11.97 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:44.54 +56:06:08.1: 9.65 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.65 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 44.54 +56 06 08.1 7.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.6785+56.0961,2461169.9164,7.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.6785+56.0961 20260509.4164 7.16CV 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 09.4164 2461169.9164 7.16 02:33:35.07 +55:54:27.1
136.95282 -4.15847 galactic Per 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 | ATO J038.3939+55.9184 | 02:33:35.02 +55:54:27.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.134+/-0.039 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:35.07 +55:54:27.1: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:35.07 +55:54:27.1: 9.67 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.67 +/- 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 09.4164* 02 33 35.07 +55 54 27.1 7.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.3939+55.9184,2461169.9164,7.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.3939+55.9184 20260509.4164 7.16CV 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 09.4164 2461169.9164 8.15 01:47:13.15 +57:44:19.2
130.34413 -4.32809 galactic Cas Second-epoch detections are separated by 0.1" and 3.4 pix
The object was found in VSX 5" 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:47:13.15 +57:44:19.2: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:47:13.15 +57:44:19.2: 10.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.69 +/- 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 09.4164* 01 47 13.15 +57 44 19.2 8.2 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 505962471920178944,2461169.9164,8.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505962471920178944 20260509.4164 8.15CV 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 09.4164 2461169.9164 8.29 02:31:46.11 +55:57:58.2
136.69471 -4.20127 galactic Per Second-epoch detections are separated by 0.4" 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 J037.9520+55.9630 | 02:31:46.12 +55:57:58.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.866+/-0.036 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:46.11 +55:57:58.2: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:46.11 +55:57:58.2: 10.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.95 +/- 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 09.4164* 02 31 46.11 +55 57 58.2 8.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.9520+55.9630,2461169.9164,8.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.9520+55.9630 20260509.4164 8.29CV 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 09.4164 2461169.9164 8.45 02:33:34.64 +56:11:51.0
136.84009 -3.89118 galactic Per Second-epoch detections are separated by 0.1" and 3.5 pix
The object was found in VSX 2" Gaia DR3 457371518333663744
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.980 G 11.010 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.64 +56:11:51.0: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.64 +56:11:51.0: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 34.64 +56 11 51.0 8.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457371518333663744,2461169.9164,8.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457371518333663744 20260509.4164 8.45CV 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 09.4164 2461169.9164 8.49 02:32:14.58 +55:56:24.6
136.76621 -4.20015 galactic Per Second-epoch detections are separated by 0.3" and 3.6 pix
The object was found in VSX 0" V1071 Per
Type: EW
# Max. Min./Amp. JD0 Period
10.940 V 11.240 V 2457070.72700 0.359847600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:14.58 +55:56:24.6: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:14.58 +55:56:24.6: 11.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.04 +/- 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 09.4164* 02 32 14.58 +55 56 24.6 8.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1071 Per,2461169.9164,8.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1071 Per 20260509.4164 8.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 8.55 02:34:13.31 +56:12:38.9
136.91783 -3.84435 galactic Per Second-epoch detections are separated by 0.2" and 3.6 pix
The object was found in VSX 0" Gaia DR3 457326232196815232
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.910 G 10.930 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.31 +56:12:38.9: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.31 +56:12:38.9: 11.10 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 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 09.4164* 02 34 13.31 +56 12 38.9 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457326232196815232,2461169.9164,8.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457326232196815232 20260509.4164 8.55CV 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 09.4164 2461169.9164 8.55 02:35:29.23 +56:28:22.8
136.97750 -3.53461 galactic Per Second-epoch detections are separated by 0.9" and 3.6 pix
The object was found in VSX 1" Gaia DR3 457711026906434048
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
10.890 G 10.920 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:29.23 +56:28:22.8: 13.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:29.23 +56:28:22.8: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 35 29.23 +56 28 22.8 8.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457711026906434048,2461169.9164,8.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457711026906434048 20260509.4164 8.55CV 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 09.4164 2461169.9164 8.67 02:33:05.57 +56:13:00.8
136.77028 -3.89913 galactic Per Second-epoch detections are separated by 1.2" 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 457372446046599424 | 02:33:05.74 +56:12:59.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.319+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:05.57 +56:13:00.8: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:05.57 +56:13:00.8: 11.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 05.57 +56 13 00.8 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457372446046599424,2461169.9164,8.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457372446046599424 20260509.4164 8.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 8.70 02:31:00.53 +56:00:30.9
136.58001 -4.20203 galactic Per Second-epoch detections are separated by 0.5" 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 457355163097206784 | 02:31:00.46 +56:00:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.177+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:00.53 +56:00:30.9: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:00.53 +56:00:30.9: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 31 00.53 +56 00 30.9 8.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457355163097206784,2461169.9164,8.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457355163097206784 20260509.4164 8.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 8.89 01:44:52.14 +57:41:43.0
130.04564 -4.43661 galactic Cas Second-epoch detections are separated by 0.3" and 3.3 pix
The object was found in VSX 2" Gaia DR3 505969726120091264
Type: ROT
# Max. Min./Amp. JD0 Period
11.620 G 11.650 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:52.14 +57:41:43.0: 13.42 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:52.14 +57:41:43.0: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 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 09.4164* 01 44 52.14 +57 41 43.0 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
Gaia DR3 505969726120091264,2461169.9164,8.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505969726120091264 20260509.4164 8.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.13 00:59:37.43 +59:16:40.0
123.97929 -3.57732 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 | ATO J014.9158+59.2824 | 00:59:36.51 +59:16:19.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 1935BSD...C01....0S BSD 8- 64 J-Ks=0.040+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:59:37.43 +59:16:40.0: 10.47 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:59:37.43 +59:16:40.0: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 59 37.43 +59 16 40.0 9.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J014.9158+59.2824,2461169.9164,9.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J014.9158+59.2824 20260509.4164 9.13CV 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 09.4164 2461169.9164 9.04 00:41:14.50 +61:35:32.2
121.71924 -1.25546 galactic Cas Second-epoch detections are separated by 0.7" and 3.1 pix
The object was found in VSX19" ZTF J004114.30+613550.9
Type: EW
# Max. Min./Amp. JD0 Period
19.942 r Y 0.720 r 2458376.85470 0.297943600000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:41:14.50 +61:35:32.2: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:41:14.50 +61:35:32.2: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 41 14.50 +61 35 32.2 9.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J004114.30+613550.9,2461169.9164,9.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J004114.30+613550.9 20260509.4164 9.04CV 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 09.4164 2461169.9164 8.90 02:33:34.36 +55:49:28.4
136.98329 -4.23569 galactic Per Second-epoch detections are separated by 1.2" 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 | ATO J038.3792+55.8236 | 02:33:34.38 +55:49:28.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.293+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.36 +55:49:28.4: 12.22 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.36 +55:49:28.4: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 34.36 +55 49 28.4 8.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.3792+55.8236,2461169.9164,8.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.3792+55.8236 20260509.4164 8.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.00 02:30:44.35 +55:58:12.9
136.55938 -4.25171 galactic Per Second-epoch detections are separated by 0.3" 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 J037.6774+55.9705 | 02:30:44.39 +55:58:12.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.306+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:44.35 +55:58:12.9: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:44.35 +55:58:12.9: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 30 44.35 +55 58 12.9 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.6774+55.9705,2461169.9164,9.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.6774+55.9705 20260509.4164 9.00CV 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 09.4164 2461169.9164 9.01 02:34:13.08 +56:11:55.4
136.92202 -3.85569 galactic Per Second-epoch detections are separated by 0.3" 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 457326232196815232 | 02:34:13.32 +56:12:39.2 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE J-Ks=0.127+/-0.030 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.08 +56:11:55.4: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.08 +56:11:55.4: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 13.08 +56 11 55.4 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457326232196815232,2461169.9164,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457326232196815232 20260509.4164 9.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.06 02:33:52.04 +56:11:00.6
136.88281 -3.88857 galactic Per Second-epoch detections are separated by 0.2" 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 J038.4611+56.1832 | 02:33:52.13 +56:11:00.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.724+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:52.04 +56:11:00.6: 13.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:52.04 +56:11:00.6: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 52.04 +56 11 00.6 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4611+56.1832,2461169.9164,9.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4611+56.1832 20260509.4164 9.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.11 02:34:03.60 +56:00:36.3
136.97474 -4.03819 galactic Per Second-epoch detections are separated by 0.1" 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 | Gaia DR3 457322280826978560 | 02:34:03.58 +56:00:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.307+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:03.60 +56:00:36.3: 13.03 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:03.60 +56:00:36.3: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 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 09.4164* 02 34 03.60 +56 00 36.3 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457322280826978560,2461169.9164,9.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457322280826978560 20260509.4164 9.11CV 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 09.4164 2461169.9164 9.16 02:33:51.13 +55:59:56.4
136.95216 -4.05962 galactic Per Second-epoch detections are separated by 1.7" 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 | Gaia DR3 457322349546464896 | 02:33:51.13 +55:59:55.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.763+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:51.13 +55:59:56.4: 12.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:51.13 +55:59:56.4: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 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 09.4164* 02 33 51.13 +55 59 56.4 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457322349546464896,2461169.9164,9.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457322349546464896 20260509.4164 9.16CV 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 09.4164 2461169.9164 9.14 02:33:43.06 +55:51:19.0
136.99027 -4.19950 galactic Per Second-epoch detections are separated by 1.4" 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 | Gaia DR3 457312453941894912 | 02:33:43.08 +55:51:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.827+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:43.06 +55:51:19.0: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:43.06 +55:51:19.0: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 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 09.4164* 02 33 43.06 +55 51 19.0 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457312453941894912,2461169.9164,9.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457312453941894912 20260509.4164 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 09.4164 2461169.9164 9.13 02:34:08.57 +55:49:36.3
137.05651 -4.20279 galactic Per Second-epoch detections are separated by 1.7" 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 | Gaia DR3 457311320070532608 | 02:34:11.00 +55:50:02.9 (Gaia DR3) | DSCT/GDOR (local) | B (local) | Gaia3var=VARIABLE SpType: OB- 1959LS....C01....0H LS I +55 38 J-Ks=0.368+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:08.57 +55:49:36.3: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:08.57 +55:49:36.3: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 08.57 +55 49 36.3 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457311320070532608,2461169.9164,9.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457311320070532608 20260509.4164 9.13CV 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 09.4164 2461169.9164 9.18 02:34:14.08 +56:19:37.9
136.87436 -3.73632 galactic Per Second-epoch detections are separated by 0.9" 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 J038.5642+56.3253 | 02:34:14.03 +56:19:38.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.205+/-0.027 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:14.08 +56:19:37.9: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:14.08 +56:19:37.9: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 14.08 +56 19 37.9 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5642+56.3253,2461169.9164,9.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5642+56.3253 20260509.4164 9.18CV 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 09.4164 2461169.9164 9.14 02:33:49.28 +55:57:07.5
136.96631 -4.10458 galactic Per Second-epoch detections are separated by 1.1" 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 J038.4666+55.9563 | 02:33:49.36 +55:57:06.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.715+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:49.28 +55:57:07.5: 12.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:49.28 +55:57:07.5: 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 09.4164* 02 33 49.28 +55 57 07.5 9.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4666+55.9563,2461169.9164,9.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4666+55.9563 20260509.4164 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 09.4164 2461169.9164 9.19 02:30:41.72 +55:56:24.9
136.56495 -4.28183 galactic Per Second-epoch detections are separated by 1.1" and 3.4 pix
The object was found in VSX 3" ASASSN-V J023041.92+555622.1
Type: L
# Max. Min./Amp. JD0 Period
12.500 V 12.680 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:41.72 +55:56:24.9: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:41.72 +55:56:24.9: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 30 41.72 +55 56 24.9 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J023041.92+555622.1,2461169.9164,9.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J023041.92+555622.1 20260509.4164 9.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.24 02:34:22.75 +56:20:28.3
136.88744 -3.71567 galactic Per Second-epoch detections are separated by 0.9" 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 J038.5944+56.3413 | 02:34:22.68 +56:20:28.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.252+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:22.75 +56:20:28.3: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:22.75 +56:20:28.3: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 22.75 +56 20 28.3 9.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5944+56.3413,2461169.9164,9.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5944+56.3413 20260509.4164 9.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.32 02:35:16.32 +56:26:20.6
136.96338 -3.57747 galactic Per Second-epoch detections are separated by 0.5" 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 457710477150655104 | 02:35:16.32 +56:26:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.240+/-0.026 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:16.32 +56:26:20.6: 10.74 +/- 0.04 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:16.32 +56:26:20.6: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 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 09.4164* 02 35 16.32 +56 26 20.6 9.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457710477150655104,2461169.9164,9.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457710477150655104 20260509.4164 9.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.37 02:32:37.64 +56:00:40.9
136.78889 -4.11385 galactic Per Second-epoch detections are separated by 0.5" 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 | Gaia DR3 457363443795236736 | 02:32:37.60 +56:00:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.204+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:37.64 +56:00:40.9: 12.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:37.64 +56:00:40.9: 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 09.4164* 02 32 37.64 +56 00 40.9 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457363443795236736,2461169.9164,9.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457363443795236736 20260509.4164 9.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.38 02:33:06.79 +56:00:36.9
136.85222 -4.08893 galactic Per Second-epoch detections are separated by 0.8" 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 | Gaia DR3 457363993551045760 | 02:33:06.84 +56:00:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.365+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:06.79 +56:00:36.9: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:06.79 +56:00:36.9: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 06.79 +56 00 36.9 9.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457363993551045760,2461169.9164,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457363993551045760 20260509.4164 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.80 01:21:20.04 +56:57:25.3
127.01921 -5.67728 galactic Cas Second-epoch detections are separated by 1.5" 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 | Gaia DR3 412606001921491712 | 01:21:21.77 +56:57:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.964+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:21:20.04 +56:57:25.3: 13.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:21:20.04 +56:57:25.3: 12.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 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 09.4164* 01 21 20.04 +56 57 25.3 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 412606001921491712,2461169.9164,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 412606001921491712 20260509.4164 9.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.56 02:33:40.44 +56:00:07.9
136.92789 -4.06627 galactic Per Second-epoch detections are separated by 0.9" and 3.6 pix
The object was found in VSX24" Gaia DR3 457316508390945792
Type: ROT
# Max. Min./Amp. JD0 Period
17.460 G 17.500 G 0.393643000000 K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:40.44 +56:00:07.9: 12.51 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:40.44 +56:00:07.9: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 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 09.4164* 02 33 40.44 +56 00 07.9 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457316508390945792,2461169.9164,9.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457316508390945792 20260509.4164 9.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.53 02:33:28.43 +56:01:32.1
136.89298 -4.05544 galactic Per Second-epoch detections are separated by 0.7" and 3.5 pix
The object was found in VSX 2" GPX-1
Type: EA/BD
# Max. Min./Amp. JD0 Period
12.310 V Y 0.010 V 2458770.23823 1.744579000000 F2Vn+L
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:28.43 +56:01:32.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:28.43 +56:01:32.1: 11.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 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 09.4164* 02 33 28.43 +56 01 32.1 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GPX-1,2461169.9164,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GPX-1 20260509.4164 9.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.55 02:34:32.09 +56:11:10.8
136.96755 -3.85005 galactic Per Second-epoch detections are separated by 0.3" 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 | ATO J038.6110+56.1853 | 02:34:32.06 +56:11:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.251+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:32.09 +56:11:10.8: 11.18 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:32.09 +56:11:10.8: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 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 09.4164* 02 34 32.09 +56 11 10.8 9.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.6110+56.1853,2461169.9164,9.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.6110+56.1853 20260509.4164 9.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.70 02:34:06.92 +56:06:17.2
136.94521 -3.94786 galactic Per Second-epoch detections are separated by 1.2" and 3.6 pix
The object was found in ASASSN-V 1" ASASSN-V J023406.97+560618.0
Type: EA
MeanMag 12.45 m Amp. 1.03 m Period 0.2057389 d
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:06.92 +56:06:17.2: 11.40 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:06.92 +56:06:17.2: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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 09.4164* 02 34 06.92 +56 06 17.2 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461169.9164,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260509.4164 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.68 02:29:26.16 +55:58:53.6
136.38550 -4.30911 galactic Per Second-epoch detections are separated by 1.7" and 3.6 pix
The object was found in VSX 2" ASASSN-V J022926.29+555852.4
Type: SR
# Max. Min./Amp. JD0 Period
12.620 V 12.810 V 2457232.00000 79.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:26.16 +55:58:53.6: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:26.16 +55:58:53.6: 12.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.31 +/- 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 09.4164* 02 29 26.16 +55 58 53.6 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J022926.29+555852.4,2461169.9164,9.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J022926.29+555852.4 20260509.4164 9.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.81 01:48:07.33 +59:50:53.1
130.00094 -2.24340 galactic Cas Second-epoch detections are separated by 0.4" 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 506613868138000384 | 01:48:06.95 +59:51:11.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.826+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:07.33 +59:50:53.1: 13.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:07.33 +59:50:53.1: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 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 09.4164* 01 48 07.33 +59 50 53.1 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506613868138000384,2461169.9164,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506613868138000384 20260509.4164 9.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.72 02:34:41.51 +56:11:02.0
136.98868 -3.84382 galactic Per Second-epoch detections are separated by 0.5" 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 | ATO J038.6605+56.1803 | 02:34:41.56 +56:11:01.9 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.064+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:41.51 +56:11:02.0: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:41.51 +56:11:02.0: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 41.51 +56 11 02.0 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.6605+56.1803,2461169.9164,9.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.6605+56.1803 20260509.4164 9.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.77 02:34:19.33 +56:07:37.8
136.96318 -3.91606 galactic Per Second-epoch detections are separated by 0.6" 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 | ATO J038.5805+56.1272 | 02:34:19.32 +56:07:38.2 (Gaia DR3) | SINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=0.560+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:19.33 +56:07:37.8: 12.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:19.33 +56:07:37.8: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 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 09.4164* 02 34 19.33 +56 07 37.8 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5805+56.1272,2461169.9164,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5805+56.1272 20260509.4164 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.79 02:32:01.75 +55:53:20.4
136.75790 -4.25886 galactic Per Second-epoch detections are separated by 1.9" 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 457339185819254144 | 02:32:01.84 +55:53:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.701+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:01.75 +55:53:20.4: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:01.75 +55:53:20.4: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 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 09.4164* 02 32 01.75 +55 53 20.4 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457339185819254144,2461169.9164,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457339185819254144 20260509.4164 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.74 02:31:04.78 +56:05:05.6
136.56045 -4.12760 galactic Per Second-epoch detections are separated by 0.7" and 3.6 pix
The object was found in VSX23" ZTF J023102.07+560506.0
Type: RS
# Max. Min./Amp. JD0 Period
16.508 r Y 0.070 r 2458425.80690 0.946063100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:04.78 +56:05:05.6: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:04.78 +56:05:05.6: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 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 09.4164* 02 31 04.78 +56 05 05.6 9.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J023102.07+560506.0,2461169.9164,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J023102.07+560506.0 20260509.4164 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.79 02:34:14.64 +56:14:11.5
136.91071 -3.81943 galactic Per Second-epoch detections are separated by 0.4" 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 457326399692569216 | 02:34:14.66 +56:14:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.469+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:14.64 +56:14:11.5: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:14.64 +56:14:11.5: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 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 09.4164* 02 34 14.64 +56 14 11.5 9.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457326399692569216,2461169.9164,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457326399692569216 20260509.4164 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.89 02:32:30.22 +55:59:10.3
136.78248 -4.14371 galactic Per Second-epoch detections are separated by 1.0" 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 J038.1327+55.9847 | 02:32:30.22 +55:59:10.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.266+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:30.22 +55:59:10.3: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:30.22 +55:59:10.3: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 32 30.22 +55 59 10.3 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.1327+55.9847,2461169.9164,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.1327+55.9847 20260509.4164 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 09.4164 2461169.9164 9.93 01:58:16.32 +59:38:59.1
131.29071 -2.13296 galactic Cas Second-epoch detections are separated by 0.5" 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 | 01:58:16.32 +59:38:59.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:16.32 +59:38:59.1: 12.59 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:16.32 +59:38:59.1: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 58 16.32 +59 38 59.1 9.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.86 02:34:10.27 +56:06:39.8
136.94997 -3.93906 galactic Per Second-epoch detections are separated by 0.5" and 3.6 pix
The object was found in VSX 1" Gaia DR3 457324617289144576
Type: RS
# Max. Min./Amp. JD0 Period
12.140 G 12.220 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:10.27 +56:06:39.8: 12.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:10.27 +56:06:39.8: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 10.27 +56 06 39.8 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457324617289144576,2461169.9164,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457324617289144576 20260509.4164 9.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.00 00:55:26.78 +60:51:04.8
123.42030 -2.01661 galactic Cas Second-epoch detections are separated by 2.0" 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 426563202528365824 | 00:55:25.40 +60:50:37.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5p 1935BSD...C01....0S BSD 8- 876 J-Ks=0.414+/-0.029 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:55:26.78 +60:51:04.8: 9.88 +/- 0.02 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:55:26.78 +60:51:04.8: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 55 26.78 +60 51 04.8 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 426563202528365824,2461169.9164,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426563202528365824 20260509.4164 10.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.00 01:18:14.18 +61:44:36.2
126.09849 -0.96348 galactic Cas Second-epoch detections are separated by 0.5" 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 | 01:18:14.18 +61:44:36.2 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:14.18 +61:44:36.2: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:14.18 +61:44:36.2: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 18 14.18 +61 44 36.2 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
target,2461169.9164,10.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.95 02:34:25.79 +56:10:43.4
136.95701 -3.86273 galactic Per Second-epoch detections are separated by 0.8" and 3.6 pix
The object was found in VSX25" Gaia DR3 457325957318911616
Type: E
# Max. Min./Amp. JD0 Period
15.150 G 15.470 G 3.840110000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:25.79 +56:10:43.4: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:25.79 +56:10:43.4: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 25.79 +56 10 43.4 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457325957318911616,2461169.9164,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457325957318911616 20260509.4164 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.02 02:33:11.33 +56:00:07.8
136.86512 -4.09235 galactic Per Second-epoch detections are separated by 1.1" 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 | Gaia DR3 457317053843745920 | 02:33:11.37 +56:00:07.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.869+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:11.33 +56:00:07.8: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:11.33 +56:00:07.8: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 11.33 +56 00 07.8 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457317053843745920,2461169.9164,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457317053843745920 20260509.4164 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.95 02:34:50.95 +56:14:16.1
136.98788 -3.78564 galactic Per Second-epoch detections are separated by 0.7" and 3.5 pix
The object was found in VSX 1" GPX-TF8A-1104
Type: ROT
# Max. Min./Amp. JD0 Period
12.380 V 12.640 V 2457600.79000 1.894100000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:50.95 +56:14:16.1: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:50.95 +56:14:16.1: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 50.95 +56 14 16.1 9.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GPX-TF8A-1104,2461169.9164,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GPX-TF8A-1104 20260509.4164 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.98 02:32:09.03 +55:55:39.6
136.75896 -4.21663 galactic Per Second-epoch detections are separated by 1.3" 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 | ATO J038.0417+55.9259 | 02:32:09.03 +55:55:39.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.414+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:09.03 +55:55:39.6: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:09.03 +55:55:39.6: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 32 09.03 +55 55 39.6 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.0417+55.9259,2461169.9164,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.0417+55.9259 20260509.4164 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.21 01:14:45.30 +60:30:04.8
125.80071 -2.24047 galactic Cas Second-epoch detections are separated by 0.8" 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 510401067222116992 | 01:14:43.22 +60:30:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5: 1935BSD...C01....0S BSD 8- 705 J-Ks=0.606+/-0.039 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:14:45.30 +60:30:04.8: 12.71 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:14:45.30 +60:30:04.8: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 14 45.30 +60 30 04.8 10.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510401067222116992,2461169.9164,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510401067222116992 20260509.4164 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.10 02:31:58.20 +56:05:41.8
136.67194 -4.07143 galactic Per Second-epoch detections are separated by 0.5" 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 | ATO J037.9859+56.1042 | 02:31:58.14 +56:05:42.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.362+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:58.20 +56:05:41.8: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:58.20 +56:05:41.8: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 31 58.20 +56 05 41.8 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.9859+56.1042,2461169.9164,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.9859+56.1042 20260509.4164 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.24 01:54:04.65 +57:00:35.8
131.41378 -4.82668 galactic Per Second-epoch detections are separated by 0.3" 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 504953605581021568 | 01:54:08.94 +57:00:36.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1932MeUpp..55....1S BD+56 383 J-Ks=0.380+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:54:04.65 +57:00:35.8: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:54:04.65 +57:00:35.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 54 04.65 +57 00 35.8 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 504953605581021568,2461169.9164,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 504953605581021568 20260509.4164 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.27 01:18:28.22 +58:11:22.5
126.49920 -4.49481 galactic Cas Second-epoch detections are separated by 0.9" 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 | ATO J019.6245+58.1745 | 01:18:29.87 +58:10:59.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8III 1951UppAn...2j...1B NGC 457 236 J-Ks=0.371+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:18:28.22 +58:11:22.5: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:18:28.22 +58:11:22.5: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 18 28.22 +58 11 22.5 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J019.6245+58.1745,2461169.9164,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J019.6245+58.1745 20260509.4164 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.34 01:58:55.84 +57:26:42.4
131.94250 -4.24112 galactic Per 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 | Gaia DR3 505306720610433024 | 01:58:57.62 +57:26:57.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: em? 1978VatOP...1..257C VES 661 J-Ks=0.879+/-0.028 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:55.84 +57:26:42.4: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:55.84 +57:26:42.4: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 58 55.84 +57 26 42.4 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505306720610433024,2461169.9164,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505306720610433024 20260509.4164 10.34CV 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 09.4164 2461169.9164 10.29 01:03:22.70 +60:32:14.0
124.40085 -2.30047 galactic Cas Second-epoch detections are separated by 0.3" 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 426389926362885504 | 01:03:24.61 +60:32:35.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.064+/-0.031 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:03:22.70 +60:32:14.0: 10.86 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:03:22.70 +60:32:14.0: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.43 +/- 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 09.4164* 01 03 22.70 +60 32 14.0 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 426389926362885504,2461169.9164,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426389926362885504 20260509.4164 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.27 01:44:32.29 +58:45:36.3
129.78361 -3.40348 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 506461620135299584 | 01:44:30.78 +58:46:10.9 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: B8: 1955ApJS....2..123F LF 5 +58 58 J-Ks=0.189+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:32.29 +58:45:36.3: 13.01 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:32.29 +58:45:36.3: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 09.4164* 01 44 32.29 +58 45 36.3 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 506461620135299584,2461169.9164,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506461620135299584 20260509.4164 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.14 02:31:42.28 +56:00:52.2
136.66809 -4.15991 galactic Per Second-epoch detections are separated by 0.5" and 3.6 pix
The object was found in VSX 4" Gaia DR3 457343686944562560
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.950 G 12.980 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:42.28 +56:00:52.2: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:42.28 +56:00:52.2: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 31 42.28 +56 00 52.2 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457343686944562560,2461169.9164,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457343686944562560 20260509.4164 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.15 02:32:31.89 +56:04:32.8
136.75187 -4.05940 galactic Per Second-epoch detections are separated by 1.8" and 3.7 pix
The object was found in VSX19" Gaia DR3 457365299221088896
Type: ROT
# Max. Min./Amp. JD0 Period
14.750 G 14.800 G G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:31.89 +56:04:32.8: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:31.89 +56:04:32.8: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 32 31.89 +56 04 32.8 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457365299221088896,2461169.9164,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457365299221088896 20260509.4164 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.13 02:33:01.37 +56:09:30.5
136.78367 -3.95682 galactic Per Second-epoch detections are separated by 1.3" 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 | target | 02:33:01.37 +56:09:30.5 (user input) | T | P | (position from user input) J-Ks=0.610+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:01.37 +56:09:30.5: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:01.37 +56:09:30.5: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 01.37 +56 09 30.5 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.13 02:33:07.17 +56:01:46.1
136.84566 -4.07084 galactic Per Second-epoch detections are separated by 1.0" 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 | Gaia DR3 457364092325569536 | 02:33:07.21 +56:01:46.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.269+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:07.17 +56:01:46.1: 13.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:07.17 +56:01:46.1: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 07.17 +56 01 46.1 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457364092325569536,2461169.9164,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457364092325569536 20260509.4164 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.06 02:30:56.83 +56:00:04.8
136.57473 -4.21199 galactic Per Second-epoch detections are separated by 1.2" 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 | Gaia DR3 457355163097206784 | 02:31:00.46 +56:00:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.439+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:56.83 +56:00:04.8: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:56.83 +56:00:04.8: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 30 56.83 +56 00 04.8 10.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457355163097206784,2461169.9164,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457355163097206784 20260509.4164 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.31 02:32:56.82 +56:04:05.6
136.80849 -4.04425 galactic Per Second-epoch detections are separated by 0.8" 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 | Gaia DR3 457365501074840320 | 02:32:56.93 +56:04:05.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.981+/-0.034 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:56.82 +56:04:05.6: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:56.82 +56:04:05.6: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 09.4164* 02 32 56.82 +56 04 05.6 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457365501074840320,2461169.9164,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457365501074840320 20260509.4164 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.26 02:31:53.23 +55:53:50.7
136.73622 -4.25862 galactic Per Second-epoch detections are separated by 1.2" 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 | target | 02:31:53.23 +55:53:50.7 (user input) | T | P | (position from user input) J-Ks=0.508+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:53.23 +55:53:50.7: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:53.23 +55:53:50.7: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 09.4164* 02 31 53.23 +55 53 50.7 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.35 01:33:15.70 +56:57:52.0
128.63558 -5.44342 galactic Cas Second-epoch detections are separated by 1.4" 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 J023.3188+56.9601 | 01:33:13.50 +56:58:10.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.908+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:33:15.70 +56:57:52.0: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:33:15.70 +56:57:52.0: 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 09.4164* 01 33 15.70 +56 57 52.0 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.3188+56.9601,2461169.9164,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J023.3188+56.9601 20260509.4164 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.24 02:34:47.05 +56:16:36.7
136.96433 -3.75317 galactic Per Second-epoch detections are separated by 0.8" 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 | ATO J038.6960+56.2768 | 02:34:47.05 +56:16:36.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.362+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:47.05 +56:16:36.7: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:47.05 +56:16:36.7: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 47.05 +56 16 36.7 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.6960+56.2768,2461169.9164,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.6960+56.2768 20260509.4164 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.24 02:31:23.81 +55:56:10.2
136.65776 -4.24870 galactic Per Second-epoch detections are separated by 0.6" 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 J037.8633+55.9364 | 02:31:23.81 +55:56:10.2 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.426+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:23.81 +55:56:10.2: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:23.81 +55:56:10.2: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 09.4164* 02 31 23.81 +55 56 10.2 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.8633+55.9364,2461169.9164,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.8633+55.9364 20260509.4164 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.46 01:16:30.98 +57:14:55.3
126.33438 -5.45729 galactic Cas Second-epoch detections are separated by 0.4" 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 413420499519574400 | 01:16:33.62 +57:14:41.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.880+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:16:30.98 +57:14:55.3: 11.76 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:16:30.98 +57:14:55.3: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 09.4164* 01 16 30.98 +57 14 55.3 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 413420499519574400,2461169.9164,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 413420499519574400 20260509.4164 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.52 00:51:32.85 +59:59:13.6
122.94564 -2.88463 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 | Gaia DR3 426864434349441664 | 00:51:36.39 +59:59:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.041 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:51:32.85 +59:59:13.6: 11.07 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:51:32.85 +59:59:13.6: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.61 +/- 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 09.4164* 00 51 32.85 +59 59 13.6 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 426864434349441664,2461169.9164,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426864434349441664 20260509.4164 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.35 02:35:07.08 +56:20:15.3
136.98338 -3.67921 galactic Per Second-epoch detections are separated by 1.6" 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 | target | 02:35:07.08 +56:20:15.3 (user input) | T | P | (position from user input) J-Ks=0.200+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:07.08 +56:20:15.3: 11.65 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:07.08 +56:20:15.3: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 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 09.4164* 02 35 07.08 +56 20 15.3 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.59 00:47:11.29 +58:29:06.0
122.37495 -4.38215 galactic Cas Second-epoch detections are separated by 1.6" 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 | ATO J011.7996+58.4919 | 00:47:11.29 +58:29:06.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A6IV (LAMOST DR5) J-Ks=0.295+/-0.043 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:47:11.29 +58:29:06.0: 11.23 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:47:11.29 +58:29:06.0: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.75 +/- 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 09.4164* 00 47 11.29 +58 29 06.0 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
ATO J011.7996+58.4919,2461169.9164,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J011.7996+58.4919 20260509.4164 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 09.4164 2461169.9164 10.45 00:33:46.94 +63:27:56.6
120.96151 0.66154 galactic Cas Second-epoch detections are separated by 0.8" 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 430883355509555584 | 00:33:46.85 +63:28:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.453+/-0.038 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:33:46.94 +63:27:56.6: 13.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:33:46.94 +63:27:56.6: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 09.4164* 00 33 46.94 +63 27 56.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 430883355509555584,2461169.9164,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 430883355509555584 20260509.4164 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 09.4164 2461169.9164 10.41 01:51:54.81 +57:35:15.7
130.99158 -4.33463 galactic Per Second-epoch detections are separated by 1.1" 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 | ATO J028.0105+57.5877 | 01:51:58.96 +57:35:14.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B9IV/V 1928MeUpp..37....1S [S28] 383 J-Ks=0.859+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:51:54.81 +57:35:15.7: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:51:54.81 +57:35:15.7: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 51 54.81 +57 35 15.7 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J028.0105+57.5877,2461169.9164,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J028.0105+57.5877 20260509.4164 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.36 01:05:57.35 +63:03:31.2
124.57549 0.23326 galactic Cas Second-epoch detections are separated by 0.8" 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 | Gaia DR3 523282292613942656 | 01:05:59.30 +63:03:46.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.019+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:05:57.35 +63:03:31.2: 10.64 +/- 0.03 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:05:57.35 +63:03:31.2: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 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 09.4164* 01 05 57.35 +63 03 31.2 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 523282292613942656,2461169.9164,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523282292613942656 20260509.4164 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.27 02:33:21.52 +56:04:02.2
136.86205 -4.02312 galactic Per Second-epoch detections are separated by 1.6" and 3.6 pix
The object was found in VSX 6" Gaia DR3 457364577666574464
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.790 G 13.810 G B
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:21.52 +56:04:02.2: 12.58 +/- 0.23 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:21.52 +56:04:02.2: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 21.52 +56 04 02.2 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457364577666574464,2461169.9164,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457364577666574464 20260509.4164 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.37 02:33:20.71 +55:51:56.8
136.93784 -4.20991 galactic Per 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 | ATO J038.3415+55.8640 | 02:33:20.71 +55:51:56.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.323+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:20.71 +55:51:56.8: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:20.71 +55:51:56.8: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 20.71 +55 51 56.8 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.3415+55.8640,2461169.9164,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.3415+55.8640 20260509.4164 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 09.4164 2461169.9164 10.35 02:32:39.77 +55:52:01.6
136.84866 -4.24530 galactic Per Second-epoch detections are separated by 1.4" 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 | Gaia DR3 457291249680242560 | 02:32:35.58 +55:51:31.8 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE SpType: F0 (LAMOST DR5) J-Ks=0.404+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:39.77 +55:52:01.6: 12.74 +/- 0.26 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:39.77 +55:52:01.6: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 09.4164* 02 32 39.77 +55 52 01.6 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457291249680242560,2461169.9164,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457291249680242560 20260509.4164 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.52 01:46:13.78 +57:54:08.3
130.18007 -4.19630 galactic Cas Second-epoch detections are separated by 2.0" 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 J026.5676+57.9049 | 01:46:16.02 +57:53:41.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.694+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:13.78 +57:54:08.3: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:13.78 +57:54:08.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 09.4164* 01 46 13.78 +57 54 08.3 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.5676+57.9049,2461169.9164,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.5676+57.9049 20260509.4164 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.38 02:34:48.63 +56:07:35.8
137.02625 -3.89018 galactic Per Second-epoch detections are separated by 1.4" 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 | ATO J038.7094+56.1248 | 02:34:48.63 +56:07:35.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.962+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:48.63 +56:07:35.8: 12.05 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:48.63 +56:07:35.8: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 48.63 +56 07 35.8 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.7094+56.1248,2461169.9164,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.7094+56.1248 20260509.4164 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 09.4164 2461169.9164 10.56 01:17:41.01 +57:07:19.9
126.50515 -5.56735 galactic Cas Second-epoch detections are separated by 3.8" and 3.4 pix
The object was found in VSX21" ZTF J011740.11+570739.6
Type: EW
# Max. Min./Amp. JD0 Period
18.175 r Y 0.983 r 2458456.67660 0.355051000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:17:41.01 +57:07:19.9: 13.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:17:41.01 +57:07:19.9: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 09.4164* 01 17 41.01 +57 07 19.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J011740.11+570739.6,2461169.9164,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J011740.11+570739.6 20260509.4164 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 09.4164 2461169.9164 10.48 02:30:39.08 +56:07:12.9
136.49165 -4.11722 galactic Per Second-epoch detections are separated by 0.7" 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 | 02:30:39.08 +56:07:12.9 (user input) | T | P | (position from user input) J-Ks=0.215+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:39.08 +56:07:12.9: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:39.08 +56:07:12.9: 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 09.4164* 02 30 39.08 +56 07 12.9 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.79 01:01:14.73 +57:14:39.1
124.26462 -5.60217 galactic Cas Second-epoch detections are separated by 2.1" and 3.4 pix
The object was found in VSX 1" ASASSN-V J010114.83+571438.2
Type: L
# Max. Min./Amp. JD0 Period
13.570 V 13.750 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:01:14.73 +57:14:39.1: 11.44 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:01:14.73 +57:14:39.1: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 09.4164* 01 01 14.73 +57 14 39.1 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
ASASSN-V J010114.83+571438.2,2461169.9164,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J010114.83+571438.2 20260509.4164 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 09.4164 2461169.9164 10.54 02:07:35.01 +56:36:56.3
133.30660 -4.71451 galactic Per Second-epoch detections are separated by 1.1" 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 | Gaia DR3 505012738691536768 | 02:07:38.32 +56:36:55.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.440+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:35.01 +56:36:56.3: 13.37 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:35.01 +56:36:56.3: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 07 35.01 +56 36 56.3 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505012738691536768,2461169.9164,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505012738691536768 20260509.4164 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.45 02:37:49.70 +57:46:16.6
136.75643 -2.21639 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 | ATO J039.4571+57.7717 | 02:37:50.58 +57:45:50.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB- 1959LS....C01....0H LS I +57 75 J-Ks=0.194+/-0.028 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:37:49.70 +57:46:16.6: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:37:49.70 +57:46:16.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 09.4164* 02 37 49.70 +57 46 16.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J039.4571+57.7717,2461169.9164,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J039.4571+57.7717 20260509.4164 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 09.4164 2461169.9164 10.46 02:34:28.10 +56:04:39.7
137.00122 -3.95378 galactic Per Second-epoch detections are separated by 1.1" 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 | target | 02:34:28.10 +56:04:39.7 (user input) | T | P | (position from user input) J-Ks=0.736+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:28.10 +56:04:39.7: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:28.10 +56:04:39.7: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 28.10 +56 04 39.7 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.45 02:33:15.77 +55:52:19.1
136.92476 -4.20862 galactic Per Second-epoch detections are separated by 0.7" and 3.5 pix
The object was found in VSX 0" Gaia DR3 457314137569073280
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.620 G 12.660 G 0.725330000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:15.77 +55:52:19.1: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:15.77 +55:52:19.1: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 15.77 +55 52 19.1 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457314137569073280,2461169.9164,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457314137569073280 20260509.4164 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 09.4164 2461169.9164 10.62 02:32:04.79 +56:03:54.2
136.69751 -4.09327 galactic Per Second-epoch detections are separated by 2.0" 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 | 02:32:04.79 +56:03:54.2 (user input) | T | P | (position from user input) J-Ks=0.192+/-0.034 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:04.79 +56:03:54.2: 13.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:04.79 +56:03:54.2: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 09.4164* 02 32 04.79 +56 03 54.2 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.75 01:09:22.48 +57:26:31.4
125.35388 -5.34532 galactic Cas Second-epoch detections are separated by 0.5" 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 J017.3204+57.4562 | 01:09:17.29 +57:26:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:09:22.48 +57:26:31.4: 13.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:09:22.48 +57:26:31.4: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 09.4164* 01 09 22.48 +57 26 31.4 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J017.3204+57.4562,2461169.9164,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.3204+57.4562 20260509.4164 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.41 02:30:46.93 +55:56:09.0
136.57791 -4.28137 galactic Per Second-epoch detections are separated by 2.3" and 3.9 pix
The object was found in VSX 8" Gaia DR3 457353479464937856
Type: E
# Max. Min./Amp. JD0 Period
18.790 G 19.120 G 0.332278000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:46.93 +55:56:09.0: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:46.93 +55:56:09.0: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 09.4164* 02 30 46.93 +55 56 09.0 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457353479464937856,2461169.9164,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457353479464937856 20260509.4164 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.46 02:11:23.25 +61:21:06.1
132.36388 -0.04735 galactic Cas Second-epoch detections are separated by 1.5" and 3.6 pix
The object was found in VSX19" Gaia DR3 507740455237382016
Type: ROT
# Max. Min./Amp. JD0 Period
14.500 G 14.530 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:11:23.25 +61:21:06.1: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:11:23.25 +61:21:06.1: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 11 23.25 +61 21 06.1 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 507740455237382016,2461169.9164,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507740455237382016 20260509.4164 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.64 01:35:19.56 +58:24:48.5
128.66715 -3.96871 galactic Cas Second-epoch detections are separated by 1.1" 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 509018534428095488 | 01:35:19.85 +58:24:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1960IzKry..24..160B [B60] +58 324 J-Ks=0.335+/-0.040 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:35:19.56 +58:24:48.5: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:35:19.56 +58:24:48.5: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 09.4164* 01 35 19.56 +58 24 48.5 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 509018534428095488,2461169.9164,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509018534428095488 20260509.4164 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.53 01:58:40.24 +59:15:59.7
131.43819 -2.49026 galactic Cas Second-epoch detections are separated by 1.0" and 3.5 pix
The object was found in VSX 2" Gaia DR3 507801031456497792
Type: RS
# Max. Min./Amp. JD0 Period
13.250 G 13.370 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:58:40.24 +59:15:59.7: 12.99 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:58:40.24 +59:15:59.7: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 58 40.24 +59 15 59.7 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 507801031456497792,2461169.9164,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507801031456497792 20260509.4164 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 09.4164 2461169.9164 10.38 02:30:44.71 +56:03:12.4
136.52890 -4.17426 galactic Per Second-epoch detections are separated by 1.6" 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 | Large-amplitude variable Gaia DR2 457356262608799232 | 02:30:44.71 +56:03:12.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.326+/-0.030 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:30:44.71 +56:03:12.4: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:30:44.71 +56:03:12.4: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 30 44.71 +56 03 12.4 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457356262608799232,2461169.9164,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457356262608799232 20260509.4164 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 09.4164 2461169.9164 10.79 01:00:17.82 +60:23:28.8
124.02698 -2.46158 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 | ATO J015.0567+60.3969 | 01:00:15.77 +60:23:42.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:00:17.82 +60:23:28.8: 12.23 +/- 0.14 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:00:17.82 +60:23:28.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 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 09.4164* 01 00 17.82 +60 23 28.8 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 J015.0567+60.3969,2461169.9164,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J015.0567+60.3969 20260509.4164 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 09.4164 2461169.9164 10.45 02:33:51.70 +56:01:15.0
136.94495 -4.03897 galactic Per Second-epoch detections are separated by 1.1" 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 | ATO J038.4647+56.0211 | 02:33:51.70 +56:01:15.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.415+/-0.042 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:51.70 +56:01:15.0: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:51.70 +56:01:15.0: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 51.70 +56 01 15.0 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4647+56.0211,2461169.9164,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4647+56.0211 20260509.4164 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 09.4164 2461169.9164 10.62 02:32:26.77 +56:07:14.1
136.72374 -4.02250 galactic Per Second-epoch detections are separated by 0.3" 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 J038.0959+56.1138 | 02:32:26.77 +56:07:14.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.482+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:26.77 +56:07:14.1: 13.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:26.77 +56:07:14.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 32 26.77 +56 07 14.1 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.0959+56.1138,2461169.9164,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.0959+56.1138 20260509.4164 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 09.4164 2461169.9164 10.70 02:33:31.71 +55:59:51.2
136.91085 -4.07838 galactic Per Second-epoch detections are separated by 1.2" 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 J038.3866+55.9928 | 02:33:31.71 +55:59:51.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.262+/-0.031 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:31.71 +55:59:51.2: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:31.71 +55:59:51.2: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 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 09.4164* 02 33 31.71 +55 59 51.2 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.3866+55.9928,2461169.9164,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.3866+55.9928 20260509.4164 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.54 02:32:17.00 +55:59:24.0
136.75246 -4.15191 galactic Per Second-epoch detections are separated by 1.4" 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 | ATO J038.0703+55.9922 | 02:32:17.00 +55:59:24.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.284+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:17.00 +55:59:24.0: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:17.00 +55:59:24.0: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 32 17.00 +55 59 24.0 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.0703+55.9922,2461169.9164,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.0703+55.9922 20260509.4164 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.78 00:57:06.54 +58:58:31.2
123.66428 -3.88835 galactic Cas Second-epoch detections are separated by 1.3" 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 | target | 00:57:06.54 +58:58:31.2 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.429+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:57:06.54 +58:58:31.2: 10.96 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:57:06.54 +58:58:31.2: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 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 09.4164* 00 57 06.54 +58 58 31.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.46 02:34:06.54 +56:16:48.1
136.87653 -3.78656 galactic Per Second-epoch detections are separated by 0.6" 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 | target | 02:34:06.54 +56:16:48.1 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:06.54 +56:16:48.1: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:06.54 +56:16:48.1: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 06.54 +56 16 48.1 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.54 01:53:10.31 +58:09:47.0
131.01900 -3.73607 galactic Cas Second-epoch detections are separated by 1.2" 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 | ATO J028.3001+58.1673 | 01:53:12.04 +58:10:02.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.787+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:53:10.31 +58:09:47.0: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:53:10.31 +58:09:47.0: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 53 10.31 +58 09 47.0 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J028.3001+58.1673,2461169.9164,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J028.3001+58.1673 20260509.4164 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.74 01:25:06.70 +59:33:57.1
127.19079 -3.02715 galactic Cas Second-epoch detections are separated by 0.5" and 3.3 pix
The object was found in VSX 1" Gaia DR3 510086091499587328
Type: ROT
# Max. Min./Amp. JD0 Period
13.620 G 13.660 G F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:06.70 +59:33:57.1: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:06.70 +59:33:57.1: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 09.4164* 01 25 06.70 +59 33 57.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 510086091499587328,2461169.9164,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 510086091499587328 20260509.4164 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 09.4164 2461169.9164 10.73 02:32:53.75 +56:02:28.7
136.81219 -4.07186 galactic Per Second-epoch detections are separated by 1.9" and 3.7 pix
The object was found in VSX23" ZTF J023251.33+560240.1
Type: RS
# Max. Min./Amp. JD0 Period
16.049 r Y 0.059 r 2458353.99290 5.324340100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:53.75 +56:02:28.7: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:53.75 +56:02:28.7: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 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 09.4164* 02 32 53.75 +56 02 28.7 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J023251.33+560240.1,2461169.9164,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J023251.33+560240.1 20260509.4164 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 09.4164 2461169.9164 10.71 02:33:02.37 +56:01:38.3
136.83614 -4.07712 galactic Per Second-epoch detections are separated by 0.8" 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 457364092325569536 | 02:33:07.21 +56:01:46.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.530+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:02.37 +56:01:38.3: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:02.37 +56:01:38.3: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 02.37 +56 01 38.3 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457364092325569536,2461169.9164,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457364092325569536 20260509.4164 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 09.4164 2461169.9164 10.76 01:04:33.85 +57:23:33.9
124.70757 -5.43374 galactic Cas Second-epoch detections are separated by 1.3" 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 | Gaia DR3 424089679316794112 | 01:04:32.85 +57:23:58.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.342+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:04:33.85 +57:23:33.9: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:04:33.85 +57:23:33.9: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 04 33.85 +57 23 33.9 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 424089679316794112,2461169.9164,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424089679316794112 20260509.4164 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.68 02:31:19.12 +56:02:17.6
136.60905 -4.15829 galactic Per Second-epoch detections are separated by 0.2" and 3.6 pix
The object was found in VSX 0" Gaia DR3 457355644133505536
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.090 G 13.150 G 0.481849000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:19.12 +56:02:17.6: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:19.12 +56:02:17.6: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 31 19.12 +56 02 17.6 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457355644133505536,2461169.9164,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457355644133505536 20260509.4164 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.71 01:46:38.52 +60:07:33.4
129.76021 -2.01189 galactic Cas Second-epoch detections are separated by 1.8" 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 | ATO J026.6591+60.1406 | 01:46:39.63 +60:07:57.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:38.52 +60:07:33.4: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:38.52 +60:07:33.4: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 09.4164* 01 46 38.52 +60 07 33.4 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
ATO J026.6591+60.1406,2461169.9164,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.6591+60.1406 20260509.4164 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 09.4164 2461169.9164 10.52 02:33:17.19 +56:06:00.2
136.84012 -3.99671 galactic Per Second-epoch detections are separated by 1.9" 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 | 02:33:17.19 +56:06:00.2 (user input) | T | P | (position from user input) J-Ks=0.847+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:17.19 +56:06:00.2: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:17.19 +56:06:00.2: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 17.19 +56 06 00.2 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.75 01:38:07.73 +61:01:40.6
128.55751 -1.33279 galactic Cas Second-epoch detections are separated by 1.7" 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 | target | 01:38:07.73 +61:01:40.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:07.73 +61:01:40.6: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:07.73 +61:01:40.6: 13.62 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 09.4164* 01 38 07.73 +61 01 40.6 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,2461169.9164,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.81 00:55:18.16 +60:03:32.6
123.41471 -2.80907 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 | Gaia DR3 426138687957303808 | 00:55:16.42 +60:03:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:55:18.16 +60:03:32.6: 11.51 +/- 0.08 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:55:18.16 +60:03:32.6: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 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 09.4164* 00 55 18.16 +60 03 32.6 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 426138687957303808,2461169.9164,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426138687957303808 20260509.4164 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.73 01:19:41.36 +62:51:05.1
126.14824 0.15623 galactic Cas Second-epoch detections are separated by 1.0" 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 | 01:19:41.36 +62:51:05.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:41.36 +62:51:05.1: 13.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:41.36 +62:51:05.1: 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 09.4164* 01 19 41.36 +62 51 05.1 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.65 02:18:59.76 +57:04:00.7
134.65212 -3.79907 galactic Per Second-epoch detections are separated by 1.4" 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 | Gaia DR3 458368672303402112 | 02:19:00.38 +57:04:27.2 (Gaia DR3) | BCEP (local) | (local) | Gaia3var=VARIABLE J-Ks=0.215+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:18:59.76 +57:04:00.7: 12.17 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:18:59.76 +57:04:00.7: 12.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.86 +/- 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 09.4164* 02 18 59.76 +57 04 00.7 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 458368672303402112,2461169.9164,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 458368672303402112 20260509.4164 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 09.4164 2461169.9164 10.54 02:33:57.45 +56:01:33.1
136.95539 -4.02916 galactic Per Second-epoch detections are separated by 1.2" 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 J038.4712+56.0294 | 02:33:57.45 +56:01:33.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.351+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:57.45 +56:01:33.1: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:57.45 +56:01:33.1: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 57.45 +56 01 33.1 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4712+56.0294,2461169.9164,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4712+56.0294 20260509.4164 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.71 02:34:24.39 +55:59:28.1
137.02687 -4.03691 galactic Per Second-epoch detections are separated by 1.4" 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 | target | 02:34:24.39 +55:59:28.1 (user input) | T | P | (position from user input) J-Ks=1.050+/-0.030 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:24.39 +55:59:28.1: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:24.39 +55:59:28.1: 13.57 +/- 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 09.4164* 02 34 24.39 +55 59 28.1 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.82 02:32:04.89 +55:55:17.2
136.75236 -4.22606 galactic Per Second-epoch detections are separated by 0.9" 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 | ATO J038.0417+55.9259 | 02:32:04.89 +55:55:17.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.118+/-0.037 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:04.89 +55:55:17.2: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:04.89 +55:55:17.2: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 09.4164* 02 32 04.89 +55 55 17.2 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.0417+55.9259,2461169.9164,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.0417+55.9259 20260509.4164 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 09.4164 2461169.9164 10.84 01:44:30.83 +57:33:34.1
130.02697 -4.57929 galactic Cas Second-epoch detections are separated by 2.2" 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 505874755803185536 | 01:44:32.05 +57:34:06.5 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE SpType: G5 1928AnHar.100...49C HD 236848 J-Ks=0.295+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:44:30.83 +57:33:34.1: 12.21 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:44:30.83 +57:33:34.1: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 09.4164* 01 44 30.83 +57 33 34.1 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 505874755803185536,2461169.9164,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505874755803185536 20260509.4164 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 09.4164 2461169.9164 10.64 02:33:36.90 +55:50:23.1
136.98292 -4.21938 galactic Per Second-epoch detections are separated by 1.7" 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 | 02:33:36.90 +55:50:23.1 (user input) | T | P | (position from user input) J-Ks=0.574+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:36.90 +55:50:23.1: 13.03 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:36.90 +55:50:23.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 36.90 +55 50 23.1 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.87 01:13:54.30 +58:12:33.7
125.89678 -4.53299 galactic Cas Second-epoch detections are separated by 0.3" 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 J018.4686+58.2100 | 01:13:54.30 +58:12:33.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:54.30 +58:12:33.7: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:54.30 +58:12:33.7: 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 09.4164* 01 13 54.30 +58 12 33.7 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
ATO J018.4686+58.2100,2461169.9164,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.4686+58.2100 20260509.4164 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 09.4164 2461169.9164 10.65 02:19:57.86 +59:32:26.9
133.94513 -1.42466 galactic Cas Second-epoch detections are separated by 0.5" 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 | ATO J034.9820+59.5389 | 02:19:57.86 +59:32:26.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.279+/-0.036 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:19:57.86 +59:32:26.9: 13.32 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:19:57.86 +59:32:26.9: 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 09.4164* 02 19 57.86 +59 32 26.9 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
ATO J034.9820+59.5389,2461169.9164,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J034.9820+59.5389 20260509.4164 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 09.4164 2461169.9164 10.66 02:34:47.29 +56:12:09.8
136.99372 -3.82126 galactic Per Second-epoch detections are separated by 1.5" 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 | Large-amplitude variable Gaia DR2 457700615896974336 | 02:34:47.29 +56:12:09.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.399+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:47.29 +56:12:09.8: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:47.29 +56:12:09.8: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 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 09.4164* 02 34 47.29 +56 12 09.8 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 457700615896974336,2461169.9164,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 457700615896974336 20260509.4164 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.64 02:34:19.23 +56:15:01.8
136.91511 -3.80244 galactic Per Second-epoch detections are separated by 1.9" 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 | 02:34:19.23 +56:15:01.8 (user input) | T | P | (position from user input) J-Ks=0.291+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:19.23 +56:15:01.8: 13.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:19.23 +56:15:01.8: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 19.23 +56 15 01.8 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.88 00:50:03.30 +57:23:20.9
122.74474 -5.48211 galactic Cas Second-epoch detections are separated by 1.4" 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 | Gaia DR3 424275840380123904 | 00:50:01.30 +57:22:57.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.422+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:50:03.30 +57:23:20.9: 11.26 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:50:03.30 +57:23:20.9: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 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 09.4164* 00 50 03.30 +57 23 20.9 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
Gaia DR3 424275840380123904,2461169.9164,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424275840380123904 20260509.4164 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 09.4164 2461169.9164 10.72 02:07:25.40 +57:54:58.4
132.90672 -3.47641 galactic Per Second-epoch detections are separated by 1.5" 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 | Gaia DR3 506730034109607680 | 02:07:24.66 +57:55:23.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.827+/-0.029 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:07:25.40 +57:54:58.4: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:07:25.40 +57:54:58.4: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 07 25.40 +57 54 58.4 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 506730034109607680,2461169.9164,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506730034109607680 20260509.4164 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 09.4164 2461169.9164 10.71 02:10:23.96 +60:01:13.7
132.65123 -1.35281 galactic Cas Second-epoch detections are separated by 0.4" 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 | 02:10:23.96 +60:01:13.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.329+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:10:23.96 +60:01:13.7: 13.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:10:23.96 +60:01:13.7: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 09.4164* 02 10 23.96 +60 01 13.7 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.70 02:33:04.96 +56:00:14.2
136.85069 -4.09639 galactic Per 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 457363993551045760 | 02:33:06.84 +56:00:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:04.96 +56:00:14.2: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:04.96 +56:00:14.2: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 04.96 +56 00 14.2 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457363993551045760,2461169.9164,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457363993551045760 20260509.4164 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.87 01:11:41.02 +58:17:27.9
125.59786 -4.47583 galactic Cas Second-epoch detections are separated by 1.0" 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 | ATO J017.9458+58.3022 | 01:11:42.53 +58:18:10.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3 1928AnHar.100...49C HD 236647 J-Ks=0.537+/-0.034 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:11:41.02 +58:17:27.9: 11.42 +/- 0.07 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:11:41.02 +58:17:27.9: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 09.4164* 01 11 41.02 +58 17 27.9 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
ATO J017.9458+58.3022,2461169.9164,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J017.9458+58.3022 20260509.4164 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 09.4164 2461169.9164 10.70 01:59:33.38 +60:01:45.4
131.34851 -1.72463 galactic Cas Second-epoch detections are separated by 1.3" and 3.4 pix
The object was found in VSX17" ZTF J015934.53+600159.8
Type: SR
# Max. Min./Amp. JD0 Period
15.783 r Y 0.432 r 2458492.34860 197.227334200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:33.38 +60:01:45.4: 13.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:33.38 +60:01:45.4: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 59 33.38 +60 01 45.4 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
ZTF J015934.53+600159.8,2461169.9164,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J015934.53+600159.8 20260509.4164 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.91 01:48:01.86 +57:39:19.3
130.46842 -4.38592 galactic Cas Second-epoch detections are separated by 2.3" 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 505773703817729024 | 01:48:05.53 +57:39:15.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.351+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:01.86 +57:39:19.3: 12.39 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:01.86 +57:39:19.3: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 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 09.4164* 01 48 01.86 +57 39 19.3 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 505773703817729024,2461169.9164,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505773703817729024 20260509.4164 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 09.4164 2461169.9164 10.70 02:29:49.57 +56:00:09.6
136.42846 -4.26927 galactic Per Second-epoch detections are separated by 0.6" and 3.6 pix
The object was found in VSX 3" Gaia DR3 457351727118196992
Type: E
# Max. Min./Amp. JD0 Period
18.170 G 18.390 G 0.483597000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:49.57 +56:00:09.6: 13.08 +/- 0.35 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:49.57 +56:00:09.6: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 29 49.57 +56 00 09.6 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457351727118196992,2461169.9164,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457351727118196992 20260509.4164 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.79 02:34:55.55 +56:12:20.3
137.01026 -3.81113 galactic Per Second-epoch detections are separated by 1.5" 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 J038.7383+56.2055 | 02:34:55.55 +56:12:20.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.196+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:55.55 +56:12:20.3: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:55.55 +56:12:20.3: 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 09.4164* 02 34 55.55 +56 12 20.3 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.7383+56.2055,2461169.9164,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.7383+56.2055 20260509.4164 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 09.4164 2461169.9164 11.05 01:13:38.95 +58:10:50.4
125.86560 -4.56451 galactic Cas Second-epoch detections are separated by 1.9" 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 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:13:38.95 +58:10:50.4: 13.13 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:13:38.95 +58:10:50.4: 13.71 +/- 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 09.4164* 01 13 38.95 +58 10 50.4 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 J018.4234+58.1762,2461169.9164,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J018.4234+58.1762 20260509.4164 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 09.4164 2461169.9164 10.82 02:32:38.56 +55:54:40.8
136.82912 -4.20550 galactic Per Second-epoch detections are separated by 1.2" 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 | 02:32:38.56 +55:54:40.8 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:38.56 +55:54:40.8: 12.92 +/- 0.33 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:38.56 +55:54:40.8: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 32 38.56 +55 54 40.8 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.79 02:21:28.82 +63:55:29.7
132.63130 2.76191 galactic Cas Second-epoch detections are separated by 7.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 515135804807626112 | 02:21:28.44 +63:54:58.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:21:28.82 +63:55:29.7: 12.91 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:21:28.82 +63:55:29.7: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 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 09.4164* 02 21 28.82 +63 55 29.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 515135804807626112,2461169.9164,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 515135804807626112 20260509.4164 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 09.4164 2461169.9164 10.69 02:34:28.15 +56:03:40.0
137.00777 -3.96902 galactic Per Second-epoch detections are separated by 2.0" 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 | 02:34:28.15 +56:03:40.0 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:28.15 +56:03:40.0: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:28.15 +56:03:40.0: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 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 09.4164* 02 34 28.15 +56 03 40.0 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.82 01:38:33.84 +60:47:24.6
128.65259 -1.55707 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 | 01:38:33.84 +60:47:24.6 (user input) | T | P | (position from user input) J-Ks=0.216+/-0.037 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:33.84 +60:47:24.6: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:33.84 +60:47:24.6: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 38 33.84 +60 47 24.6 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,2461169.9164,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.82 02:35:13.46 +56:19:56.7
136.99899 -3.67822 galactic Per Second-epoch detections are separated by 2.2" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J038.8155+56.3217 | 02:35:13.46 +56:19:56.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.419+/-0.027 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:13.46 +56:19:56.7: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:13.46 +56:19:56.7: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 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 09.4164* 02 35 13.46 +56 19 56.7 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.8155+56.3217,2461169.9164,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.8155+56.3217 20260509.4164 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 09.4164 2461169.9164 11.23 00:56:42.62 +58:03:48.0
123.63158 -4.80125 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 | Gaia DR3 424366618808033152 | 00:56:41.03 +58:04:10.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.604+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:56:42.62 +58:03:48.0: 13.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:56:42.62 +58:03:48.0: 14.28 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.28 +/- 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 09.4164* 00 56 42.62 +58 03 48.0 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
Gaia DR3 424366618808033152,2461169.9164,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424366618808033152 20260509.4164 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 09.4164 2461169.9164 10.99 01:57:13.86 +57:26:43.7
131.72075 -4.29927 galactic Per Second-epoch detections are separated by 4.1" 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 | ATO J029.2798+57.4367 | 01:57:08.70 +57:26:40.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:57:13.86 +57:26:43.7: 11.01 +/- 0.05 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:57:13.86 +57:26:43.7: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.41 +/- 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 09.4164* 01 57 13.86 +57 26 43.7 11.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J029.2798+57.4367,2461169.9164,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J029.2798+57.4367 20260509.4164 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 09.4164 2461169.9164 10.72 02:28:46.17 +56:02:23.7
136.27709 -4.28923 galactic Per Second-epoch detections are separated by 3.2" 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 | target | 02:28:46.17 +56:02:23.7 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.033 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:46.17 +56:02:23.7: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:46.17 +56:02:23.7: 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 09.4164* 02 28 46.17 +56 02 23.7 10.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.96 02:31:39.66 +56:01:58.4
136.65546 -4.14519 galactic Per Second-epoch detections are separated by 2.8" 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 | 02:31:39.66 +56:01:58.4 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:39.66 +56:01:58.4: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:39.66 +56:01:58.4: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 31 39.66 +56 01 58.4 11.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.11 01:38:06.27 +58:10:40.1
129.06883 -4.13681 galactic Cas Second-epoch detections are separated by 5.2" and 3.9 pix
The object was found in VSX10" Gaia DR3 508962699851411840
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
16.190 G 16.240 G A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:38:06.27 +58:10:40.1: 13.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:38:06.27 +58:10:40.1: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 09.4164* 01 38 06.27 +58 10 40.1 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 508962699851411840,2461169.9164,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 508962699851411840 20260509.4164 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 09.4164 2461169.9164 11.03 00:50:31.13 +64:31:47.5
122.83307 1.65829 galactic Cas Second-epoch detections are separated by 3.6" 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 | 00:50:31.13 +64:31:47.5 (user input) | T | P | (position from user input) J-Ks=1.071+/-0.033 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:50:31.13 +64:31:47.5: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:50:31.13 +64:31:47.5: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 50 31.13 +64 31 47.5 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,2461169.9164,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.84 01:46:23.23 +61:12:56.7
129.49869 -0.95345 galactic Cas Second-epoch detections are separated by 0.9" and 3.4 pix
The object was found in VSX22" Gaia DR3 511217282805374208
Type: ROT
# Max. Min./Amp. JD0 Period
18.220 G 18.350 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:23.23 +61:12:56.7: 12.59 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:23.23 +61:12:56.7: 13.81 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 46 23.23 +61 12 56.7 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 511217282805374208,2461169.9164,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 511217282805374208 20260509.4164 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 09.4164 2461169.9164 11.19 01:26:28.54 +59:41:35.0
127.34494 -2.87814 galactic Cas Second-epoch detections are separated by 2.7" 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 J021.6536+59.6928 | 01:26:31.85 +59:41:21.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.039 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:26:28.54 +59:41:35.0: 12.81 +/- 0.29 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:26:28.54 +59:41:35.0: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 09.4164* 01 26 28.54 +59 41 35.0 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
ATO J021.6536+59.6928,2461169.9164,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J021.6536+59.6928 20260509.4164 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 09.4164 2461169.9164 10.79 02:34:09.98 +55:51:55.6
137.04456 -4.16583 galactic Per Second-epoch detections are separated by 1.7" 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 | ATO J038.5415+55.8654 | 02:34:09.98 +55:51:55.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.453+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:09.98 +55:51:55.6: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:09.98 +55:51:55.6: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 09.98 +55 51 55.6 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5415+55.8654,2461169.9164,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5415+55.8654 20260509.4164 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 09.4164 2461169.9164 10.90 01:59:05.94 +59:55:34.3
131.32005 -1.83904 galactic Cas Second-epoch detections are separated by 2.4" 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 | Gaia DR3 507895516435392512 | 01:59:07.43 +59:54:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B2 1953IzKry..10..120K [K53] 683 J-Ks=0.818+/-0.035 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:59:05.94 +59:55:34.3: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:59:05.94 +59:55:34.3: 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 09.4164* 01 59 05.94 +59 55 34.3 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 507895516435392512,2461169.9164,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507895516435392512 20260509.4164 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.03 01:28:07.91 +58:50:39.6
127.67293 -3.68923 galactic Cas Second-epoch detections are separated by 0.4" and 3.2 pix
The object was found in VSX23" Gaia DR3 509266886619110144
Type: ROT
# Max. Min./Amp. JD0 Period
15.900 G 15.940 G 6.018600000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:28:07.91 +58:50:39.6: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:28:07.91 +58:50:39.6: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 09.4164* 01 28 07.91 +58 50 39.6 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
Gaia DR3 509266886619110144,2461169.9164,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509266886619110144 20260509.4164 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.81 02:34:19.54 +56:15:41.6
136.91148 -3.79197 galactic Per Second-epoch detections are separated by 0.6" and 3.5 pix
The object was found in VSX11" Gaia DR3 457701749777231232
Type: ROT
# Max. Min./Amp. JD0 Period
17.650 G 17.720 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:19.54 +56:15:41.6: 13.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:19.54 +56:15:41.6: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 09.4164* 02 34 19.54 +56 15 41.6 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457701749777231232,2461169.9164,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457701749777231232 20260509.4164 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.81 00:44:10.04 +64:27:25.8
122.14798 1.59649 galactic Cas Second-epoch detections are separated by 3.6" and 3.0 pix
The object was found in VSX16" Gaia DR3 524089505951689984
Type: RS
# Max. Min./Amp. JD0 Period
18.070 G 18.230 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:44:10.04 +64:27:25.8: 12.42 +/- 0.22 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:44:10.04 +64:27:25.8: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 00 44 10.04 +64 27 25.8 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 524089505951689984,2461169.9164,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524089505951689984 20260509.4164 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.99 02:32:09.39 +56:09:40.6
136.67082 -4.00019 galactic Per Second-epoch detections are separated by 2.0" and 3.5 pix
The object was found in VSX16" Gaia DR3 457369559828613504
Type: ROT
# Max. Min./Amp. JD0 Period
15.080 G 15.100 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:09.39 +56:09:40.6: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:09.39 +56:09:40.6: 13.75 +/- 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 09.4164* 02 32 09.39 +56 09 40.6 11.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457369559828613504,2461169.9164,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457369559828613504 20260509.4164 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 09.4164 2461169.9164 10.91 01:43:03.30 +58:57:12.9
129.55634 -3.25268 galactic Cas Second-epoch detections are separated by 0.6" 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 | ATO J025.7767+58.9545 | 01:43:03.30 +58:57:12.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.236+/-0.035 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:43:03.30 +58:57:12.9: 13.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:43:03.30 +58:57:12.9: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 09.4164* 01 43 03.30 +58 57 12.9 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
ATO J025.7767+58.9545,2461169.9164,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.7767+58.9545 20260509.4164 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 09.4164 2461169.9164 10.86 02:02:53.90 +60:15:42.0
131.68742 -1.38966 galactic Cas Second-epoch detections are separated by 2.1" 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 507950977353541248 | 02:02:48.33 +60:15:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.870+/-0.032 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:53.90 +60:15:42.0: 13.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:53.90 +60:15:42.0: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 09.4164* 02 02 53.90 +60 15 42.0 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
Gaia DR3 507950977353541248,2461169.9164,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507950977353541248 20260509.4164 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.78 02:33:46.62 +55:56:04.6
136.96732 -4.12309 galactic Per Second-epoch detections are separated by 0.8" 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 J038.4446+55.9342 | 02:33:46.62 +55:56:04.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.708+/-0.028 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:46.62 +55:56:04.6: 13.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:46.62 +55:56:04.6: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 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 09.4164* 02 33 46.62 +55 56 04.6 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4446+55.9342,2461169.9164,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4446+55.9342 20260509.4164 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
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.84 02:35:02.29 +56:14:22.9
137.01138 -3.77368 galactic Per Second-epoch detections are separated by 1.0" 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 | target | 02:35:02.29 +56:14:22.9 (user input) | T | P | (position from user input) J-Ks=0.856+/-0.056 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:02.29 +56:14:22.9: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:02.29 +56:14:22.9: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 35 02.29 +56 14 22.9 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.03 01:24:55.22 +57:12:20.0
127.47423 -5.37060 galactic Cas Second-epoch detections are separated by 1.2" 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 412996878304856960 | 01:24:59.06 +57:12:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.757+/-0.035 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:24:55.22 +57:12:20.0: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:24:55.22 +57:12:20.0: 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 09.4164* 01 24 55.22 +57 12 20.0 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
Gaia DR3 412996878304856960,2461169.9164,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 412996878304856960 20260509.4164 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.10 01:34:42.46 +58:42:15.2
128.53836 -3.69572 galactic Cas Second-epoch detections are separated by 1.4" 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 | 01:34:42.46 +58:42:15.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:34:42.46 +58:42:15.2: 13.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:34:42.46 +58:42:15.2: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 09.4164* 01 34 42.46 +58 42 15.2 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,2461169.9164,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.09 02:05:23.30 +59:19:31.5
132.24862 -2.20206 galactic Cas Second-epoch detections are separated by 1.2" and 3.3 pix
The object was found in VSX19" Gaia DR3 507054012083283584
Type: ROT
# Max. Min./Amp. JD0 Period
18.020 G 18.120 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:05:23.30 +59:19:31.5: 12.17 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:05:23.30 +59:19:31.5: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 09.4164* 02 05 23.30 +59 19 31.5 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
Gaia DR3 507054012083283584,2461169.9164,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 507054012083283584 20260509.4164 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 09.4164 2461169.9164 10.95 02:32:58.07 +56:06:56.5
136.79298 -3.99928 galactic Per 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 | target | 02:32:58.07 +56:06:56.5 (user input) | T | P | (position from user input) J-Ks=0.258+/-0.045 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:58.07 +56:06:56.5: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:58.07 +56:06:56.5: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 32 58.07 +56 06 56.5 10.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.23 01:19:29.17 +59:25:20.5
126.49815 -3.25503 galactic Cas Second-epoch detections are separated by 2.6" 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 | Large-amplitude variable Gaia DR2 414042479505165696 | 01:19:30.78 +59:24:54.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G3 1935BSD...C01....0S BSD 8- 264 J-Ks=0.435+/-0.045 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:19:29.17 +59:25:20.5: 13.01 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:19:29.17 +59:25:20.5: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 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 09.4164* 01 19 29.17 +59 25 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
Large-amplitude variable Gaia DR2 414042479505165696,2461169.9164,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 414042479505165696 20260509.4164 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 09.4164 2461169.9164 11.15 01:36:50.88 +59:55:48.3
128.59739 -2.44121 galactic Cas Second-epoch detections are separated by 1.3" and 3.1 pix
The object was found in VSX 1" Gaia DR3 509760361181182976
Type: ROT
# Max. Min./Amp. JD0 Period
13.870 G 13.910 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:50.88 +59:55:48.3: 12.78 +/- 0.21 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:50.88 +59:55:48.3: 14.00 +/- 0.06 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 09.4164* 01 36 50.88 +59 55 48.3 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 509760361181182976,2461169.9164,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509760361181182976 20260509.4164 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 09.4164 2461169.9164 10.87 02:39:10.93 +63:43:59.5
134.51621 3.31147 galactic Cas Second-epoch detections are separated by 0.2" 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 | target | 02:39:10.93 +63:43:59.5 (user input) | T | P | (position from user input) J-Ks=0.484+/-0.027 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:39:10.93 +63:43:59.5: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:39:10.93 +63:43:59.5: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 39 10.93 +63 43 59.5 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,2461169.9164,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.92 02:20:14.56 +59:20:12.7
134.04700 -1.60487 galactic Cas Second-epoch detections are separated by 3.4" 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 | ZTF J022011.89+592041.4 | 02:20:13.98 +59:20:38.1 (Gaia DR3) | BY (local) | 2458491.72350 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:20:14.56 +59:20:12.7: 13.41 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:20:14.56 +59:20:12.7: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 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 09.4164* 02 20 14.56 +59 20 12.7 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 J022011.89+592041.4,2461169.9164,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J022011.89+592041.4 20260509.4164 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 09.4164 2461169.9164 11.01 02:32:27.21 +55:53:12.4
136.81392 -4.23831 galactic Per Second-epoch detections are separated by 2.1" 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 | target | 02:32:27.21 +55:53:12.4 (user input) | T | P | (position from user input) J-Ks=0.133+/-0.037 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:27.21 +55:53:12.4: 13.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:27.21 +55:53:12.4: 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 09.4164* 02 32 27.21 +55 53 12.4 11.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.34 00:50:58.17 +59:43:06.7
122.87278 -3.15317 galactic Cas Second-epoch detections are separated by 3.5" and 3.4 pix
The object was found in VSX 2" WISE J005058.3+594306
Type: EW
# Max. Min./Amp. JD0 Period
14.315 r Y 0.420 r 2458424.74210 0.775185200000
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:50:58.17 +59:43:06.7: 11.67 +/- 0.09 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:50:58.17 +59:43:06.7: 14.41 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 09.4164* 00 50 58.17 +59 43 06.7 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
WISE J005058.3+594306,2461169.9164,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J005058.3+594306 20260509.4164 11.34CV 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 09.4164 2461169.9164 11.18 01:48:30.79 +58:02:54.6
130.44483 -3.98828 galactic Cas Second-epoch detections are separated by 1.6" 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 505808304072634240 | 01:48:34.21 +58:02:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.550+/-0.038 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:48:30.79 +58:02:54.6: 13.08 +/- 0.27 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:48:30.79 +58:02:54.6: 13.91 +/- 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 09.4164* 01 48 30.79 +58 02 54.6 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 505808304072634240,2461169.9164,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505808304072634240 20260509.4164 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 09.4164 2461169.9164 11.10 02:33:09.09 +56:06:53.6
136.81700 -3.99022 galactic Per Second-epoch detections are separated by 1.0" 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 | 02:33:09.09 +56:06:53.6 (user input) | T | P | (position from user input) J-Ks=0.461+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:09.09 +56:06:53.6: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:09.09 +56:06:53.6: 13.75 +/- 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 09.4164* 02 33 09.09 +56 06 53.6 11.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.17 01:25:45.38 +59:01:19.8
127.34425 -3.55526 galactic Cas Second-epoch detections are separated by 0.5" 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 | 01:25:45.38 +59:01:19.8 (user input) | T | P | (position from user input) J-Ks=0.769+/- (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:25:45.38 +59:01:19.8: 13.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:25:45.38 +59:01:19.8: 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 09.4164* 01 25 45.38 +59 01 19.8 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,2461169.9164,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 11.32 00:59:00.02 +59:04:33.1
123.90549 -3.78159 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 | ATO J014.7371+59.0689 | 00:59:00.02 +59:04:33.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.403+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:59:00.02 +59:04:33.1: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:59:00.02 +59:04:33.1: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 09.4164* 00 59 00.02 +59 04 33.1 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
ATO J014.7371+59.0689,2461169.9164,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J014.7371+59.0689 20260509.4164 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 09.4164 2461169.9164 11.28 01:52:55.36 +59:33:30.6
130.65684 -2.38792 galactic Cas Second-epoch detections are separated by 1.3" and 3.2 pix
The object was found in VSX17" Gaia DR3 506553498077188608
Type: ROT
# Max. Min./Amp. JD0 Period
15.360 G 15.380 G 2.474540000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:52:55.36 +59:33:30.6: 13.34 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:52:55.36 +59:33:30.6: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 52 55.36 +59 33 30.6 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 506553498077188608,2461169.9164,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 506553498077188608 20260509.4164 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 09.4164 2461169.9164 11.21 01:08:11.66 +62:14:23.2
124.88182 -0.56851 galactic Cas Second-epoch detections are separated by 4.0" and 3.0 pix
The object was found in VSX 1" 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:08:11.66 +62:14:23.2: 12.21 +/- 0.13 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:08:11.66 +62:14:23.2: 14.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 09.4164* 01 08 11.66 +62 14 23.2 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 522685876279259136,2461169.9164,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 522685876279259136 20260509.4164 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 09.4164 2461169.9164 11.26 01:46:56.97 +57:21:54.8
130.38910 -4.70059 galactic Cas Second-epoch detections are separated by 1.2" 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 J026.7341+57.3724 | 01:46:56.97 +57:21:54.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.448+/-0.035 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:46:56.97 +57:21:54.8: 11.40 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:46:56.97 +57:21:54.8: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.79 +/- 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 09.4164* 01 46 56.97 +57 21 54.8 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 J026.7341+57.3724,2461169.9164,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.7341+57.3724 20260509.4164 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.40 02:02:32.20 +58:06:03.8
132.23241 -3.48106 galactic Per Second-epoch detections are separated by 1.3" 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 505442853895424256 | 02:02:33.95 +58:05:25.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.216+/-0.041 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:02:32.20 +58:06:03.8: 13.30 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:02:32.20 +58:06:03.8: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 09.4164* 02 02 32.20 +58 06 03.8 11.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 505442853895424256,2461169.9164,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 505442853895424256 20260509.4164 11.40CV 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 09.4164 2461169.9164 11.45 00:58:34.73 +57:44:23.1
123.88852 -5.11873 galactic Cas Second-epoch detections are separated by 5.5" and 3.7 pix
The object was found in VSX 4" Gaia DR3 424170012386792064
Type: ROT
# Max. Min./Amp. JD0 Period
14.240 G 14.280 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:58:34.73 +57:44:23.1: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:58:34.73 +57:44:23.1: 14.24 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.24 +/- 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 09.4164* 00 58 34.73 +57 44 23.1 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
Gaia DR3 424170012386792064,2461169.9164,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 424170012386792064 20260509.4164 11.45CV 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 09.4164 2461169.9164 11.34 01:36:37.08 +58:44:43.7
128.77607 -3.61268 galactic Cas Second-epoch detections are separated by 0.9" and 3.2 pix
The object was found in VSX 2" Gaia DR3 509123228550621568
Type: ROT
# Max. Min./Amp. JD0 Period
14.260 G 14.310 G 2.477030000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:36:37.08 +58:44:43.7: 13.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:36:37.08 +58:44:43.7: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 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 09.4164* 01 36 37.08 +58 44 43.7 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
Gaia DR3 509123228550621568,2461169.9164,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 509123228550621568 20260509.4164 11.34CV 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 09.4164 2461169.9164 11.24 02:32:25.16 +56:00:34.4
136.76263 -4.12660 galactic Per Second-epoch detections are separated by 1.5" 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 | 02:32:25.16 +56:00:34.4 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.034 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:25.16 +56:00:34.4: 13.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:25.16 +56:00:34.4: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 09.4164* 02 32 25.16 +56 00 34.4 11.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 11.53 01:31:55.84 +59:26:39.9
128.06555 -3.02312 galactic Cas Second-epoch detections are separated by 2.1" 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:31:55.84 +59:26:39.9: 13.28 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:31:55.84 +59:26:39.9: 14.16 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.16 +/- 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 09.4164* 01 31 55.84 +59 26 39.9 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J023.0100+59.4551,2461169.9164,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J023.0100+59.4551 20260509.4164 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 09.4164 2461169.9164 11.55 01:07:30.37 +60:38:18.7
124.90174 -2.17175 galactic Cas Second-epoch detections are separated by 0.1" 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 | Gaia DR3 426402639467423488 | 01:07:32.09 +60:38:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A8 1935BSD...C01....0S BSD 8-1110 J-Ks=0.426+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:07:30.37 +60:38:18.7: 12.40 +/- 0.17 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:07:30.37 +60:38:18.7: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 07 30.37 +60 38 18.7 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 426402639467423488,2461169.9164,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 426402639467423488 20260509.4164 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 09.4164 2461169.9164 10.43 02:28:46.53 +56:00:06.1
136.29197 -4.32446 galactic Per Second-epoch detections are separated by 3.1" 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 | target | 02:28:46.53 +56:00:06.1 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.032 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:46.53 +56:00:06.1: 12.24 +/- 0.15 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:46.53 +56:00:06.1: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 28 46.53 +56 00 06.1 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.16 02:32:01.70 +57:03:30.6
136.31360 -3.17666 galactic Per Second-epoch detections are separated by 0.3" 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 J037.9985+57.0505 | 02:32:01.70 +57:03:30.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.309+/-0.033 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:01.70 +57:03:30.6: 13.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:01.70 +57:03:30.6: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 09.4164* 02 32 01.70 +57 03 30.6 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.9985+57.0505,2461169.9164,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.9985+57.0505 20260509.4164 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.53 02:26:40.29 +56:09:51.2
135.95850 -4.27993 galactic Per Second-epoch detections are separated by 1.8" 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 | 02:26:40.29 +56:09:51.2 (user input) | T | P | (position from user input) J-Ks=0.312+/-0.030 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:26:40.29 +56:09:51.2: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:26:40.29 +56:09:51.2: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 26 40.29 +56 09 51.2 10.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.29 02:27:56.21 +56:10:22.8
136.11990 -4.20791 galactic Per Second-epoch detections are separated by 0.5" 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 | target | 02:27:56.21 +56:10:22.8 (user input) | T | P | (position from user input) J-Ks=0.734+/-0.030 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:56.21 +56:10:22.8: 13.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:56.21 +56:10:22.8: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 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 09.4164* 02 27 56.21 +56 10 22.8 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 8.91 01:29:32.61 +63:18:22.4
127.19599 0.75039 galactic Cas Second-epoch detections are separated by 1.5" and 3.1 pix
The object was found in VSX21" Gaia DR3 512422416270622592
Type: E
# Max. Min./Amp. JD0 Period
14.980 G 15.330 G 0.779180000000 A
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 01:29:32.61 +63:18:22.4: 12.22 +/- 0.25 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 01:29:32.61 +63:18:22.4: 12.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 01 29 32.61 +63 18 22.4 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
Gaia DR3 512422416270622592,2461169.9164,8.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 512422416270622592 20260509.4164 8.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.98 02:34:00.02 +55:56:27.7
136.99376 -4.10511 galactic Per Second-epoch detections are separated by 1.3" and 3.5 pix
The object was found in VSX 1" Gaia DR3 457313205553053184
Type: ROT
# Max. Min./Amp. JD0 Period
12.440 G 12.480 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:00.02 +55:56:27.7: 13.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:00.02 +55:56:27.7: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 00.02 +55 56 27.7 10.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457313205553053184,2461169.9164,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457313205553053184 20260509.4164 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.24 02:29:11.65 +56:22:44.6
136.20686 -3.95219 galactic Per Second-epoch detections are separated by 0.3" 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 | ATO J037.2825+56.3782 | 02:29:11.71 +56:22:43.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.814+/-0.031 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:11.65 +56:22:44.6: 13.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:11.65 +56:22:44.6: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 29 11.65 +56 22 44.6 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.2825+56.3782,2461169.9164,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.2825+56.3782 20260509.4164 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.52 02:33:51.39 +55:58:25.7
136.96246 -4.08264 galactic Per Second-epoch detections are separated by 0.6" 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 J038.4645+55.9736 | 02:33:51.48 +55:58:25.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.991+/-0.036 (M)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:51.39 +55:58:25.7: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:51.39 +55:58:25.7: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 51.39 +55 58 25.7 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.4645+55.9736,2461169.9164,9.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.4645+55.9736 20260509.4164 9.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.56 02:33:52.85 +56:31:18.5
136.75385 -3.57569 galactic Per Second-epoch detections are separated by 1.1" 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 | 02:33:52.85 +56:31:18.5 (user input) | T | P | (position from user input) J-Ks=0.178+/-0.029 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:52.85 +56:31:18.5: 13.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:52.85 +56:31:18.5: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 33 52.85 +56 31 18.5 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 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 09.4164 2461169.9164 10.56 02:34:27.89 +57:30:42.7
136.44425 -2.63179 galactic Per Second-epoch detections are separated by 1.3" 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 | ATO J038.6072+57.5164 | 02:34:27.89 +57:30:42.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.419+/-0.028 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:27.89 +57:30:42.7: 12.99 +/- 0.32 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:27.89 +57:30:42.7: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 09.4164* 02 34 27.89 +57 30 42.7 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.6072+57.5164,2461169.9164,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.6072+57.5164 20260509.4164 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 09.4164 2461169.9164 9.50 02:34:13.39 +56:03:48.2
136.97516 -3.98022 galactic Per Second-epoch detections are separated by 0.5" 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 J038.5561+56.0631 | 02:34:13.47 +56:03:47.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.310+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.39 +56:03:48.2: 13.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.39 +56:03:48.2: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 34 13.39 +56 03 48.2 9.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J038.5561+56.0631,2461169.9164,9.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J038.5561+56.0631 20260509.4164 9.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.61 02:44:06.26 +62:20:01.3
135.60268 2.26640 galactic Cas Second-epoch detections are separated by 2.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:44:06.26 +62:20:01.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:44:06.26 +62:20:01.3: 12.15 +/- 0.12 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:44:06.26 +62:20:01.3: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 44 06.26 +62 20 01.3 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 7.08 02:34:05.94 +56:37:27.5
136.74200 -3.46954 galactic Per Second-epoch detections are separated by 0.7" and 3.6 pix
The object was found in VSX24" Gaia DR3 457763322428148096
Type: ROT
# Max. Min./Amp. JD0 Period
15.220 G 15.260 G K
The object was not found in astcheck.
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:05.94 +56:37:27.5: 13.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:05.94 +56:37:27.5: 9.62 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.62 +/- 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 09.4164* 02 34 05.94 +56 37 27.5 7.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457763322428148096,2461169.9164,7.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457763322428148096 20260509.4164 7.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.44 02:27:52.20 +56:32:26.7
135.97686 -3.86884 galactic Per Second-epoch detections are separated by 1.2" 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 | target | 02:27:52.20 +56:32:26.7 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.032 (K)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:27:52.20 +56:32:26.7: 13.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:27:52.20 +56:32:26.7: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 27 52.20 +56 32 26.7 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.29 02:29:03.07 +56:34:20.1
136.11705 -3.77990 galactic Per Second-epoch detections are separated by 0.8" 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 | ATO J037.2539+56.5741 | 02:29:03.07 +56:34:20.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.287+/-0.032 (F)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:29:03.07 +56:34:20.1: 13.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:29:03.07 +56:34:20.1: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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 09.4164* 02 29 03.07 +56 34 20.1 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J037.2539+56.5741,2461169.9164,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J037.2539+56.5741 20260509.4164 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 10.57 02:46:03.81 +63:32:43.3
135.29035 3.45822 galactic Cas Second-epoch detections are separated by 0.8" 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 | 02:46:03.81 +63:32:43.3 (user input) | T | P | (position from user input) J-Ks=0.346+/-0.026 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:46:03.81 +63:32:43.3: 13.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:46:03.81 +63:32:43.3: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 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 09.4164* 02 46 03.81 +63 32 43.3 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461169.9164,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260509.4164 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.87 02:49:57.09 +63:51:39.7
135.54165 3.92958 galactic Cas Second-epoch detections are separated by 1.6" 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 467697169465689088 | 02:49:53.99 +63:51:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.456+/-0.031 (G)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:49:57.09 +63:51:39.7: 13.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:49:57.09 +63:51:39.7: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 09.4164* 02 49 57.09 +63 51 39.7 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 467697169465689088,2461169.9164,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 467697169465689088 20260509.4164 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 09.4164 2461169.9164 9.01 02:28:35.24 +56:03:02.7
136.24937 -4.28850 galactic Per Second-epoch detections are separated by 0.3" 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 | Gaia DR3 457539743610843648 | 02:28:35.31 +56:03:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.051+/-0.034 (A)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:28:35.24 +56:03:02.7: 13.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:28:35.24 +56:03:02.7: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 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 09.4164* 02 28 35.24 +56 03 02.7 9.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 457539743610843648,2461169.9164,9.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 457539743610843648 20260509.4164 9.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461169.91677302 09.05.2026 09:59:59.189 /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 43
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
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: 7 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): 29625
Objects passed selection criteria: 29505
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 22441.5
Average stars matched: 21816.8 (97.2161 %)
Memory usage VmPeak: 132912 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 6 12:14:36 CDT 2026
VaST build number 1.0rc89-43-g0c21e0c3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat May 9 05:02:42 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-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Last image: 2461169.91677302 09.05.2026 09:59:59.189 /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 846
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 82 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): 203442
Objects passed selection criteria: 203002
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 164544
Average stars matched: 159020 (96.6427 %)
Memory usage VmPeak: 2088396 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 6 12:14:36 CDT 2026
VaST build number 1.0rc89-43-g0c21e0c3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat May 9 05:08:59 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
SExtractor catalog cache: saved Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.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: 2461169.91610925
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits'
wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits exists and is non-empty
Saving wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits to local_wcs_cache/
'wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits' -> 'local_wcs_cache/wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (1st reference image)
verification OK: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Image size: 935.1'x628.0' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 01:42:28.702 +61:59:06.60 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits (1st new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
Image size: 943.0'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:31.223 +62:01:37.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:42:28.702 +61:59:06.60
Second-epoch image center 01:42:31.223 +62:01:37.30
Angular distance between the image centers 0.0421 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits (2nd new image)
verification OK: wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
Image size: 943.0'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:30.165 +62:01:19.40 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 01:42:30.165 +62:01:19.40
Angular distance between the image centers 0.0370 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 01:42:31.223 +62:01:37.30
Second-epoch second image center 01:42:30.165 +62:01:19.40
Angular distance between the image centers 0.00539 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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits &> /tmp/tmp.tC3Hdo0sRC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits &> /tmp/tmp.GVKkpqUx05
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits &> /tmp/tmp.SEgsZm0uAG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits &> /tmp/tmp.4reRQVVWXK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
Found non-empty wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits and wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat
The reference image (wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits) and catalog (wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat) found
'wcs_Cas-03-Q1b1x1_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 22.937800
a=0.000000 b=1.000000 c=22.937800
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31559 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.1058 to 45.5655 deg, Dec +55.3302 to +67.4436 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.1058 to 45.5655 deg, Dec 55.3302 to 67.4436 deg
Loaded 26111 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 24 out of 32 total matches.
Matched with Tycho-2 32 out of 31559 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -> calib.txt_param_ref_wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits (aperture=5.9)
Read 31681 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 7.0659 to 45.7628 deg, Dec +55.3336 to +67.4023 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 7.0659 to 45.7628 deg, Dec 55.3336 to 67.4023 deg
Loaded 26179 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 14497 out of 16269 total matches.
Matched with Tycho-2 16269 out of 31681 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 32 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
2.3 pix fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
2.3 pix fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
2.2 pix wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
2.2 pix wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Limiting magnitude estimates:
15.3 mag. Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
15.3 mag. Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
14.2 mag. fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
14.2 mag. fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.tC3Hdo0sRC (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits' -> 'wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
Checking if the catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits
WCS catalog name: wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.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-Q1b1x1_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: 5.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 267 matched stars entering correct_measured_positions(), 10048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 403 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 336 matched stars entering correct_measured_positions(), 10093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.39"
Accuracy estimation diagnostic: 331 matched stars entering correct_measured_positions(), 12854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.75"
Excluding outliers - 331 stars left (next iteration limit 293)
The image catalog is written to wcs_Cas-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits -region wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GVKkpqUx05 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits' -> 'wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
Checking if the catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat corresponding to the image wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits
WCS catalog name: wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.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-Q1b1x1_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(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 29075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-03-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits -region wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SEgsZm0uAG (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_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.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_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1304, passed=13486
Got 13486 stars (including 12173 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits.cat
util/solve_plate_with_UCAC5 got 13486 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.0'
Seting catalog search parameters based on the expected field of view 943.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013097 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010478 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 13155 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 13154 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 13154 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits -region wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.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.4reRQVVWXK (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_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.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_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
WCS_IMAGE_NAME=wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
WCS-calibrated image found: wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
Checking if the catalog wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits.cat corresponding to the image wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
WCS catalog name: wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1306, passed=13589
Got 13589 stars (including 12267 good ones) from the SExtractor catalog wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits.cat
util/solve_plate_with_UCAC5 got 13589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.0'
Seting catalog search parameters based on the expected field of view 943.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013097 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010478 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 13216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 13217 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 13217 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits -region wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-01_20.00sec_-4.90C_LIGHTs_0327.fits'
Saving fully-calibrated image wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-09_CI_Cas-03-Q1b1x1_050104_TTUQ1b1x1_2198374_vC3XQgG8/wcs_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328.fits'
Preparing the HTML report for the field Cas-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:31.08 +55:57:01.6: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:27.12 +56:17:13.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:35.11 +55:54:26.8: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:15:45.93 +65:17:15.0: 13.90 +/- 0.06 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:30.83 +55:55:53.7: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:13.86 +56:15:04.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:44.57 +56:06:07.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:11.09 +55:50:02.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:26.27 +55:59:07.8: 15.24 +/- 0.24 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 00:37:00.24 +63:08:01.5: 15.53 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:31.08 +55:57:01.6: 10.33 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:35:31.08 +55:57:01.6: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:27.12 +56:17:13.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 02:36:27.12 +56:17:13.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:35.11 +55:54:26.8: 9.65 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:15:45.93 +65:17:15.0: 10.86 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:30.83 +55:55:53.7: 9.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.65 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:30.83 +55:55:53.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry filter REJECTED candidate at 02:33:35.11 +55:54:26.8: ref_mag=9.65 +/- 0.00 new_mean_mag=9.7935 delta=-0.14 (need > 0.90)
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:13.86 +56:15:04.9: 9.90 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:35:13.86 +56:15:04.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry filter REJECTED candidate at 02:15:45.93 +65:17:15.0: ref_mag=10.87 +/- 0.00 new_mean_mag=10.9909 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:44.57 +56:06:07.9: 9.64 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:34:44.57 +56:06:07.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:11.09 +55:50:02.4: 9.40 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:26.27 +55:59:07.8: 9.42 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:34:11.09 +55:50:02.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 9.42 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:26.27 +55:59:07.8: ref_mag=9.42 +/- 0.00 new_mean_mag=9.5651 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:23.75 +56:25:38.7: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:44.68 +56:11:29.5: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 00:37:00.24 +63:08:01.5: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Forced photometry filter KEPT candidate at 00:37:00.24 +63:08:01.5: ref_mag=13.04 +/- 0.03 new_mean_mag=10.4609 delta=2.58 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:40.23 +56:10:17.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:23.75 +56:25:38.7: 10.59 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:36:23.75 +56:25:38.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:46.12 +55:57:58.2: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:32:14.62 +55:56:24.5: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:26.57 +55:50:36.3: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:33:34.73 +56:11:50.4: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:44.68 +56:11:29.5: 11.16 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 02:35:44.68 +56:11:29.5: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:13.37 +56:12:38.5: 15.30 +/- 0.28 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:31:00.55 +56:00:30.8: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:40.23 +56:10:17.9: 11.33 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 02:35:40.23 +56:10:17.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:46.12 +55:57:58.2: 10.94 +/- 0.00 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:26.57 +55:50:36.3: 10.84 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:34:26.57 +55:50:36.3: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 10.94 +/- 0.00
Forced photometry filter REJECTED candidate at 02:31:46.12 +55:57:58.2: ref_mag=10.94 +/- 0.00 new_mean_mag=10.9234 delta=0.02 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:32:14.62 +55:56:24.5: 11.02 +/- 0.01 detection
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:33:34.73 +56:11:50.4: 10.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.01
Forced photometry filter REJECTED candidate at 02:32:14.62 +55:56:24.5: ref_mag=11.02 +/- 0.01 new_mean_mag=11.1047 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 10.95 +/- 0.00
Forced photometry filter REJECTED candidate at 02:33:34.73 +56:11:50.4: ref_mag=10.95 +/- 0.00 new_mean_mag=10.9835 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:35:16.83 +56:08:45.7: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:36:15.20 +56:20:24.0: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:13.37 +56:12:38.5: 11.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.01
Forced photometry filter REJECTED candidate at 02:34:13.37 +56:12:38.5: ref_mag=11.08 +/- 0.01 new_mean_mag=11.1990 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:31:00.55 +56:00:30.8: 11.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.01
Forced photometry filter REJECTED candidate at 02:31:00.55 +56:00:30.8: ref_mag=11.23 +/- 0.01 new_mean_mag=11.3244 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:35:16.83 +56:08:45.7: 10.88 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 02:35:16.83 +56:08:45.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:36:15.20 +56:20:24.0: 11.51 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 02:36:15.20 +56:20:24.0: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-40-37_20.00sec_-14.90C_LIGHT_0018.fits at 02:34:05.93 +56:37:27.6: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Cas-03-Q1b1x1_2026-01-20_19-41-18_20.00sec_-15.00C_LIGHT_0019.fits at 02:34:05.93 +56:37:27.6: 9.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.61 +/- 0.00
Forced photometry filter REJECTED candidate at 02:34:05.93 +56:37:27.6: ref_mag=9.61 +/- 0.00 new_mean_mag=9.7332 delta=-0.13 (need > 0.90)
Adding exclusion_list_local.txt__out52269.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: 2s
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Considering the candidate 52171_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52171_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52213_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52213_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:34:59.11 +55:58:58.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52214_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52214_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:33:24.74 +56:01:05.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52227_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52227_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52230_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52230_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52236_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52236_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52247_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52247_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52248_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52248_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52250_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52250_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:19:06.77 +57:08:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52265_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52265_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52269_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 52269_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 52289_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52289_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52303_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52303_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52316_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52316_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:19:16.49 +57:10:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52325_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52325_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52360_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52360_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52362_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52362_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52367_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52367_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52386_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52386_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52394_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52394_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:38:01.10 +63:01:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52396_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52396_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:18:52.26 +57:06:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52403_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52403_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52406_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52406_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52427_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52427_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52443_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52443_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52445_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52445_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:32:19.54 +56:13:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52449_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52449_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 52468_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 52468_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 23703_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 23703_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:54:53.92 +58:33:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25035_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 25035_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 51449_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 51449_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:30:27.28 +62:31:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08339_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 08339_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:25:46.78 +57:59:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250703_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250703_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250706_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250706_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:25:29.88 +57:00:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250709_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250709_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:46:31.96 +57:52:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250713_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250713_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250715_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250715_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250739_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250739_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250740_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250740_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250741_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250741_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250751_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250751_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250752_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250752_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250755_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250755_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:09:24.51 +58:01:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250760_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250760_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250765_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250765_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250766_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250766_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250769_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250769_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250771_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250771_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250772_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250772_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:07:36.75 +58:09:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250773_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250773_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250777_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250777_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:20:42.11 +59:35:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250778_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250778_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250779_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250779_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250784_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250784_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:32:32.51 +57:12:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250786_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250786_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 250788_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250788_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250791_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250791_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:49:19.56 +59:37:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250792_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250792_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:01:13.96 +59:02:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250794_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250794_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250795_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250795_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:12:09.72 +58:47:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250799_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250799_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250802_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250802_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250807_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250807_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250812_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250812_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250813_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250813_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250815_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250815_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250818_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250818_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250821_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250821_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250826_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250826_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250831_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250831_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250836_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250836_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250840_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250840_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250842_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250842_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250844_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250844_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 250845_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250845_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250846_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250846_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:49:09.25 +58:48:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250852_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250852_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250853_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250853_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:49:24.53 +57:18:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250855_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250855_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:51:39.92 +58:29:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250856_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250856_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:58:55.63 +60:52:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250859_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250859_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250860_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250860_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:55:46.31 +59:17:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250862_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250862_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250863_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250863_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250864_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250864_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250865_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250865_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250873_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250873_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250875_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250875_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250877_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250877_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250879_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250879_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:54:46.11 +58:44:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250880_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250880_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250881_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250881_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:17:15.37 +57:23:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250883_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250883_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:46:20.37 +57:33:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250884_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250884_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:43:27.31 +58:38:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250886_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250886_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:55:02.65 +58:24:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250888_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250888_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 250893_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250893_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250899_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250899_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250900_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250900_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250902_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250902_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250903_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250903_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250907_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250907_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250908_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250908_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250910_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250910_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250915_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250915_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250919_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250919_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250920_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250920_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250921_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250921_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:58:07.79 +64:50:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250926_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250926_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:09:21.92 +64:35:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250928_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250928_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250931_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250931_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250932_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250932_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250935_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250935_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250938_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250938_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:50:14.37 +60:18:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250939_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250939_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:30:45.96 +58:16:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250940_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250940_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250941_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250941_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:00:26.42 +63:04:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250942_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250942_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250943_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250943_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250944_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250944_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250946_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250946_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250948_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250948_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:59:21.04 +66:57:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250951_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250951_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250952_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250952_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:47:41.77 +60:06:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250953_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250953_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:26:36.61 +59:41:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250955_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250955_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250956_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250956_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:17:14.97 +58:35:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250957_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250957_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 250959_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250959_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:18:38.87 +64:37:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250961_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250961_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:55:56.95 +59:45:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250962_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250962_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:07:34.97 +57:33:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250963_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250963_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 250964_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250964_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250966_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250966_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250968_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250968_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250969_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250969_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:20:40.41 +56:58:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250970_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250970_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:00:35.10 +57:15:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250972_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250972_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 250974_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250974_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250975_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250975_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 250979_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250979_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250980_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250980_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250982_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250982_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250983_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250983_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:33:32.61 +56:18:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250984_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250984_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250986_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250986_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:52:40.27 +60:40:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250987_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250987_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250988_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250988_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250990_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250990_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250991_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250991_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250993_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250993_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:02:09.89 +57:03:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250994_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250994_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250995_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 250995_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:53:50.55 +59:10:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250997_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250997_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 250998_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 250998_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251000_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251000_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251001_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251001_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:14:01.35 +57:40:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251002_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251002_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251007_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251007_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251008_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251008_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251009_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251009_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251012_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251012_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:44:52.01 +59:55:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251015_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251015_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:58:23.80 +57:37:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251017_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251017_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:15:01.11 +61:41:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251018_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251018_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:15:19.43 +57:44:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251021_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251021_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251024_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251024_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251025_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251025_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251026_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251026_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:44:49.71 +61:12:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251028_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251028_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:30:25.68 +57:18:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251030_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251030_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251034_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251034_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251035_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251035_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251036_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251036_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:20:45.00 +57:55:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251037_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251037_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 251039_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251039_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251040_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251040_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251043_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251043_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251044_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251044_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251047_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251047_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251048_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251048_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:00:49.05 +64:08:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251050_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251050_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:57:03.71 +59:44:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251052_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251052_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251053_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251053_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:57:01.36 +57:18:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251054_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251054_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:56:44.81 +59:40:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251055_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251055_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:20:40.41 +56:58:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251056_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251056_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251058_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251058_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251063_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251063_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251064_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251064_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:52:17.14 +58:00:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251066_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251066_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:21:37.59 +57:52:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251067_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251067_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251068_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251068_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251072_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251072_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251073_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251073_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251076_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251076_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251077_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251077_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251078_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251078_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251080_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251080_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:55:45.20 +58:21:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251082_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251082_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251083_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251083_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251086_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251086_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251087_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251087_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:03:21.61 +57:48:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251089_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251089_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:45:22.96 +57:47:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251090_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251090_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251091_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251091_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:02:17.85 +58:15:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251092_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251092_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251093_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251093_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251095_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251095_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:10:37.48 +57:22:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251097_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251097_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251098_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251098_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251099_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251099_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:08:27.87 +57:06:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251101_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251101_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251102_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251102_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251103_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251103_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251104_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251104_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:45:38.83 +59:44:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251106_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251106_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251110_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251110_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:50:06.93 +58:35:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251111_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251111_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251114_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251114_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251115_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251115_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251116_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251116_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:42:49.59 +60:21:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251117_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251117_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251118_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251118_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251119_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251119_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 251121_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251121_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251122_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251122_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251123_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251123_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251124_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251124_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:08:10.19 +58:38:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251125_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251125_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251127_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251127_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251129_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251129_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:43:22.82 +60:41:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251131_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251131_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:30:39.89 +57:40:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251133_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251133_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251134_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251134_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:07:08.01 +57:44:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251136_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251136_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251137_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251137_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251138_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251138_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251139_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251139_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:53:30.98 +63:23:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251141_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251141_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251142_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251142_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:59:11.73 +62:14:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251143_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251143_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251144_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251144_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:55:14.57 +59:32:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251146_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251146_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251147_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251147_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251148_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251148_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251149_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251149_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:23:03.14 +57:10:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251150_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251150_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:44:34.59 +58:49:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251152_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251152_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251154_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251154_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:53:34.98 +56:58:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251155_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251155_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:35:19.99 +62:46:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251156_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251156_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251157_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251157_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251160_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251160_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:15:16.87 +57:28:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251161_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251161_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:53:24.66 +57:04:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251164_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251164_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251166_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251166_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:45:01.10 +60:52:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251167_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251167_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251168_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251168_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:56:58.94 +60:15:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251170_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251170_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251171_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251171_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251172_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251172_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251173_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251173_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251174_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251174_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251175_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251175_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251176_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251176_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:49:12.95 +64:11:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251178_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251178_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:58:40.45 +58:55:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251180_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251180_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251181_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251181_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:59:47.54 +63:45:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251183_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251183_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:13:07.04 +58:04:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251184_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251184_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:50:19.93 +63:44:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251185_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251185_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:22:08.29 +60:22:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251189_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251189_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251193_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251193_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:02:14.63 +61:54:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251195_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251195_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251196_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251196_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:57:16.02 +60:20:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251234_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251234_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:34:59.10 +55:58:58.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 251235_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251235_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:33:24.68 +56:01:06.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 251236_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251236_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251238_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251238_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251249_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251249_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251251_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251251_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251257_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251257_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251259_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251259_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251268_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251268_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251269_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251269_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251285_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251285_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:19:06.80 +57:08:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251287_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251287_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251307_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251307_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251308_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251308_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251318_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251318_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251319_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251319_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 251340_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251340_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251351_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251351_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:19:16.51 +57:10:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251363_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251363_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251368_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251368_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:32:06.83 +56:40:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251382_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251382_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251390_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251390_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251407_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251407_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251410_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251410_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251421_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251421_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251423_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251423_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251428_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251428_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251436_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251436_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 251438_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251438_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:18:52.94 +57:06:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251443_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251443_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251448_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251448_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251455_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251455_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251463_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251463_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251484_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251484_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251486_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251486_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251492_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251492_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 251496_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251496_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251499_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251499_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251508_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251508_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251517_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251517_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251519_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251519_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251538_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251538_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251549_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251549_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:56:38.51 +59:13:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251560_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251560_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:46:05.95 +58:14:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251561_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251561_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:44:02.26 +61:53:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251562_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251562_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251568_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251568_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251571_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251571_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251577_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251577_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251583_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251583_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251596_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251596_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:32:19.27 +56:13:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251597_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251597_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:19:11.12 +58:20:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251598_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251598_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251604_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251604_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:38:00.41 +57:56:45.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251610_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251610_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:53:29.02 +57:10:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251611_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251611_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251614_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251614_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:18:49.78 +57:06:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251618_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251618_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251625_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251625_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:33:23.23 +58:01:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251627_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251627_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251635_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251635_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251657_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251657_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:45:52.38 +64:24:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251659_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251659_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:50:20.17 +58:31:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251662_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251662_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251668_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251668_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251672_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251672_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:16:47.30 +57:00:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251675_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251675_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251677_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251677_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251679_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251679_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251682_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251682_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 251734_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251734_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251741_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251741_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:53:16.09 +61:08:53.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251743_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251743_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251745_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251745_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251747_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251747_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:26:22.40 +57:24:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251757_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251757_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251760_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251760_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251771_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251771_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251773_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251773_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251774_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251774_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:42:19.84 +58:34:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251779_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251779_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251780_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251780_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:28:15.29 +58:44:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251796_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251796_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:16:34.92 +57:02:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251802_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251802_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:46:48.01 +59:52:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251809_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251809_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251813_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251813_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251815_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251815_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251820_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251820_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:04:32.55 +57:59:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251823_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251823_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:26:46.64 +57:46:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251829_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251829_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251831_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251831_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251841_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251841_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251851_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251851_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 251858_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251858_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251860_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251860_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:21:50.73 +57:15:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251863_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251863_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 251867_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251867_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251872_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251872_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251874_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251874_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:31:15.08 +58:01:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251877_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251877_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251878_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251878_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251880_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251880_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251882_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251882_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251884_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251884_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 251892_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251892_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251897_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251897_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 251899_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251899_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 251903_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251903_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:51:34.71 +57:33:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251907_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251907_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251913_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251913_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:56:23.23 +59:10:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251921_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251921_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251928_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251928_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251936_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251936_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251941_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251941_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:27:22.72 +57:31:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251944_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251944_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 251945_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251945_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251947_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251947_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:54:00.30 +60:01:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251949_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251949_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 251952_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251952_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251959_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251959_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251960_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251960_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 251977_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251977_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:35:22.21 +56:08:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251979_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251979_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:39:31.45 +60:01:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251981_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251981_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:20:11.06 +58:12:08.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251985_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 251985_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 251988_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251988_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:04:18.74 +57:35:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251991_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 251991_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252001_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252001_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 252002_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252002_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252012_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252012_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252019_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252019_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 252023_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252023_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:51:46.62 +57:14:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252027_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252027_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252045_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252045_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:57:33.48 +57:46:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252055_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252055_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 252057_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252057_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:19:12.55 +65:35:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252061_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252061_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:04:31.74 +58:01:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252063_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252063_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:57:15.08 +58:47:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252071_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252071_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:26:41.06 +60:46:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252072_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252072_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252077_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252077_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:46:34.29 +63:01:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252085_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252085_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 252086_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252086_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:04:17.19 +57:09:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252087_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252087_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252090_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252090_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 252092_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252092_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252099_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252099_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252106_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252106_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:41:14.32 +61:03:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252111_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252111_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252115_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252115_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:55:05.57 +56:57:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252117_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252117_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:46:33.58 +61:16:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252126_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252126_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 252131_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252131_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:58:52.06 +60:36:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252139_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252139_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252142_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252142_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:39:20.06 +62:14:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252143_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252143_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252147_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252147_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252149_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252149_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252156_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252156_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252157_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252157_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:16:08.62 +58:49:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252158_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252158_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252160_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252160_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252165_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252165_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252168_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252168_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252169_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252169_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252171_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252171_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252180_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252180_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252181_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252181_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:58:55.36 +58:52:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252184_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252184_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252196_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252196_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:44:53.95 +58:19:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252201_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252201_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252212_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252212_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252216_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252216_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:44:17.64 +61:53:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252222_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252222_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252223_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252223_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:16:39.09 +57:02:20.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252224_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252224_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:43:03.38 +58:08:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252227_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252227_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 252243_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252243_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252244_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252244_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252254_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252254_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 252257_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252257_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:18:57.96 +57:06:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252258_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252258_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252264_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252264_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:52:33.14 +60:18:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252270_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252270_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:21:28.08 +57:48:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252274_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252274_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252281_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252281_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252286_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252286_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 252295_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252295_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252298_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252298_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252303_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252303_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252304_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252304_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 252306_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252306_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 252309_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252309_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252318_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252318_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252321_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252321_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252327_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252327_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252328_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252328_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 252330_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252330_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252331_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252331_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252348_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252348_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252351_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252351_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:42:59.84 +57:39:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252362_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252362_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252364_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252364_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:36:28.68 +62:40:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252367_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252367_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:00:51.86 +58:31:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252371_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252371_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:58:13.52 +64:23:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252378_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252378_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:19:22.26 +58:19:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252382_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252382_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:13:30.05 +58:34:25.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252384_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252384_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 252387_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252387_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252390_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252390_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 252413_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252413_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252428_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252428_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252430_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252430_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252441_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252441_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252442_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252442_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:49:24.96 +57:34:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252445_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252445_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:37:21.84 +64:05:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252453_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252453_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:26:35.89 +57:57:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252454_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252454_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 252461_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252461_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:54:50.76 +62:25:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252462_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252462_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:17:00.05 +57:02:23.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252472_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252472_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:00:36.79 +58:30:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252474_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252474_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252475_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252475_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252477_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252477_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252481_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252481_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:16:05.17 +58:49:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252485_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252485_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252490_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252490_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252495_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252495_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:02:54.88 +64:24:57.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252496_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252496_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252502_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252502_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252504_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252504_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:03:58.39 +58:23:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252508_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252508_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:03:48.05 +60:49:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252509_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252509_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:19:37.56 +57:03:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252512_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252512_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252519_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252519_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:16:02.13 +58:49:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252526_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252526_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252528_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252528_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252530_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252530_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:02:44.35 +58:55:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252544_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252544_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252547_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252547_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:46:55.33 +59:35:28.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252552_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252552_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:41:47.87 +59:55:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252558_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252558_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:07:47.76 +57:02:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252560_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252560_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252562_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252562_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252566_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252566_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:06:23.65 +62:44:04.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252568_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252568_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 252573_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252573_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:34:10.15 +62:09:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252574_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252574_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 252582_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252582_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252588_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252588_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 252594_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252594_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252598_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252598_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252602_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252602_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 252604_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252604_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252607_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252607_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252615_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252615_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252616_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252616_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252619_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252619_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252623_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252623_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:37:13.72 +58:38:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252628_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252628_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:51:55.97 +58:13:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252632_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252632_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252633_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252633_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252643_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252643_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252652_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252652_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252653_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252653_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252655_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252655_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252673_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252673_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252684_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252684_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252686_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252686_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:58:04.19 +57:58:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252687_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252687_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252690_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252690_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252695_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252695_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252696_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252696_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252706_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252706_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 252708_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252708_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:00:23.52 +59:45:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252713_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252713_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:16:24.21 +58:04:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252718_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252718_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 252719_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252719_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:46:38.03 +58:16:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252727_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252727_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:07:40.20 +63:30:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252733_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252733_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:16:36.29 +64:57:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252734_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252734_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:08:30.42 +58:24:18.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252737_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252737_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252741_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252741_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252742_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252742_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:14:00.56 +59:02:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252747_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252747_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252748_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252748_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:06:45.34 +59:50:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252753_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252753_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252760_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252760_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252761_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252761_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252775_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252775_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:53:59.18 +56:47:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252777_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252777_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252779_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252779_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:39:24.13 +58:23:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252782_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252782_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 252783_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252783_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252785_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252785_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:01:11.53 +59:09:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252788_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252788_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252799_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252799_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252803_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252803_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252809_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252809_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252815_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252815_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:03:04.71 +57:10:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252819_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252819_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:21:07.41 +56:45:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252825_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252825_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252830_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252830_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:02:06.45 +58:56:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252831_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252831_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:01:14.90 +59:23:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252837_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252837_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:11:50.55 +59:02:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252842_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252842_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:23:01.08 +57:15:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252843_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252843_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:46:50.90 +60:39:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252853_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252853_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252855_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252855_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:03:24.30 +57:34:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252858_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252858_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252861_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252861_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 252862_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252862_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252865_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252865_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252866_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252866_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:37:41.28 +58:37:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252867_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252867_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:18:04.86 +57:29:36.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252868_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252868_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252870_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252870_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:31:32.56 +61:02:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252875_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252875_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252883_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252883_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252892_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252892_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252909_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252909_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:14:41.93 +58:46:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252919_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252919_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:45:14.53 +64:24:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252921_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252921_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:30:16.05 +57:48:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252928_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252928_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252935_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252935_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252936_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252936_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:46:01.68 +57:50:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252949_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252949_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:33:24.79 +58:21:27.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252952_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252952_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:37:13.17 +58:38:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252953_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252953_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252956_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252956_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:21:01.44 +57:11:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252961_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252961_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252974_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252974_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 252977_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252977_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252978_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252978_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 252981_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252981_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252984_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 252984_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 252986_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252986_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:06:12.29 +57:43:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252989_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252989_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252991_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252991_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:29:30.30 +60:40:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252997_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252997_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 252999_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 252999_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:54:18.84 +63:38:07.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 253000_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253000_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253004_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253004_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:47:12.47 +59:53:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253005_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253005_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:44:56.56 +59:46:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253006_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253006_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253014_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253014_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 253017_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253017_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253024_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253024_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:58:13.78 +60:44:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253038_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253038_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253041_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253041_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253042_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253042_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 253044_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253044_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253046_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253046_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:54:01.06 +59:48:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253050_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253050_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 253051_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253051_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:48:39.96 +59:09:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253052_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253052_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:11:36.05 +57:37:16.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253060_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253060_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253062_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253062_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 253068_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253068_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 253075_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253075_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253076_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253076_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253077_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253077_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253078_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253078_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253079_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253079_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:29:46.63 +58:31:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253083_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253083_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253092_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253092_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:54:06.38 +61:05:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253097_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253097_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:29:34.09 +63:19:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253098_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253098_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 253102_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253102_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253113_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253113_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:38:12.01 +61:01:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253116_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253116_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253120_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253120_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:46:18.29 +60:59:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253127_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253127_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:46:03.02 +58:23:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253131_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253131_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:59:38.40 +63:14:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253135_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253135_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:58:56.52 +58:04:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253138_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253138_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253139_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253139_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:39:54.31 +57:11:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253143_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253143_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:34:00.06 +57:01:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253147_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253147_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:58:52.01 +59:58:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253157_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253157_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253158_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253158_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253159_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253159_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253161_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253161_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253162_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253162_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253168_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253168_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:03:25.39 +57:50:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253172_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253172_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253174_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253174_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253175_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253175_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253183_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253183_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253186_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253186_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253190_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253190_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253201_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253201_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253204_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253204_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 253206_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253206_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253213_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253213_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253217_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253217_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:20:50.44 +58:20:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253224_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253224_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253226_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253226_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:30:09.17 +57:48:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253257_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253257_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:31:29.20 +58:12:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253261_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253261_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253262_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253262_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 253274_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253274_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253276_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253276_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253294_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253294_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253300_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253300_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253306_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253306_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253322_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253322_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253325_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253325_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253338_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253338_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253339_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253339_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:50:28.28 +57:04:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253351_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253351_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253355_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253355_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253364_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253364_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253365_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253365_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253368_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253368_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253372_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253372_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253381_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253381_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253385_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253385_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:24:22.15 +57:36:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253392_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253392_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:55:52.82 +56:59:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253407_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253407_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253411_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253411_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 253416_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253416_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:35:21.85 +61:07:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253420_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253420_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253437_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253437_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253446_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253446_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 253463_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253463_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:41:35.66 +57:32:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253464_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253464_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253468_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253468_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 253491_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253491_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:55:32.83 +64:09:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253507_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253507_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 253540_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253540_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253548_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253548_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253552_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253552_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253556_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253556_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:09:17.70 +56:58:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253564_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253564_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253583_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253583_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253590_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253590_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 253597_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253597_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 253603_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253603_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253618_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253618_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:20:42.00 +57:11:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253621_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253621_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:12:42.16 +57:56:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253636_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253636_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253650_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253650_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253661_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253661_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:00:35.49 +58:32:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253668_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253668_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
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Considering the candidate 253675_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253675_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:56:25.46 +62:05:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253686_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253686_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 253690_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253690_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:48:34.78 +58:41:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253711_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253711_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 253728_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253728_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 253753_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253753_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 253761_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 253761_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253764_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253764_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:44:29.99 +60:37:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253766_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253766_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 253772_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253772_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 253775_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253775_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 253798_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253798_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 253808_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253808_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 253827_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253827_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 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 253835_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 253835_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 233663_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 233663_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 235846_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 235846_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 176011_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 176011_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:32:46.24 +56:29:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76113_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 76113_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:02:02.23 +62:41:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212588_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 212588_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 214314_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 214314_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 71539_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 71539_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 214209_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 214209_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220392_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 220392_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46105_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 46105_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:38:01.06 +63:01:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67097_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 67097_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:37:00.23 +63:08:01.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 215315_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 215315_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178237_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 178237_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211875_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 211875_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:11:03.57 +57:20:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135864_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 135864_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 170264_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 170264_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
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Considering the candidate 70271_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 70271_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:20:32.62 +62:32:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237872_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 237872_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34359_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 34359_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:34:27.54 +64:32:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218015_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 218015_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55535_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 55535_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180134_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 180134_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 222553_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 222553_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235811_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 235811_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:53:02.81 +60:35:48.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39378_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 39378_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 01:47:55.47 +64:32:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174224_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 174224_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233560_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 233560_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193780_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 193780_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 00:54:53.92 +58:33:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63215_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
The candidate 63215_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328 did not pass the final checks
**** FOUND 02:30:27.27 +62:31:45.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21028_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 21028_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211642_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
Preparing report for the candidate 211642_fd_Cas-03-Q1b1x1_2026-05-09_04-59-59_20.00sec_-4.90C_LIGHTs_0328
make_report_in_HTML.sh Phase 2 (HTML assembly): 23s
make_report_in_HTML.sh TOTAL: 725s
Prepared the HTML report for the field Cas-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:37:00.24 +63:08:01.5
02:34:27.89 +57:30:42.7
02:29:03.07 +56:34:20.1
02:33:52.85 +56:31:18.5
02:34:05.94 +56:37:27.5
02:49:57.09 +63:51:39.7
02:28:35.24 +56:03:02.7
02:26:40.29 +56:09:51.2
02:34:00.02 +55:56:27.7
02:27:56.21 +56:10:22.8
02:33:51.39 +55:58:25.7
02:34:13.39 +56:03:48.2
02:29:11.65 +56:22:44.6
02:27:52.20 +56:32:26.7
02:46:03.81 +63:32:43.3
02:28:46.53 +56:00:06.1
02:32:01.70 +57:03:30.6
01:49:54.28 +63:40:38.1
01:26:01.91 +57:08:04.9
01:57:29.18 +60:09:19.3
01:50:10.11 +57:10:52.0
01:29:45.03 +59:58:32.3
01:11:20.01 +61:17:54.4
01:10:01.79 +66:17:40.5
02:30:11.32 +66:01:46.4
01:02:07.21 +61:19:23.6
01:58:50.68 +56:57:17.7
01:19:26.87 +57:22:51.4
01:22:50.45 +58:12:42.0
02:03:02.00 +56:50:06.8
01:06:16.04 +57:53:24.3
01:15:36.33 +63:27:54.0
01:27:12.82 +58:27:16.9
01:47:04.43 +59:18:55.3
01:13:09.81 +64:30:33.5
00:49:57.44 +60:17:56.5
00:44:47.70 +66:11:33.2
01:09:10.52 +58:09:35.5
01:08:39.16 +60:32:40.7
02:21:32.56 +56:32:12.5
01:10:12.02 +59:17:25.4
01:50:46.76 +58:00:38.2
01:07:39.08 +59:59:18.1
01:09:22.85 +58:34:03.2
01:06:37.45 +60:22:38.2
01:15:44.77 +60:02:45.6
01:29:49.42 +58:16:02.6
01:25:52.13 +57:05:24.0
01:07:00.11 +61:28:29.9
01:01:11.29 +65:10:55.4
02:47:22.83 +63:30:07.2
00:46:55.69 +60:00:23.1
01:47:27.75 +64:31:09.8
02:24:32.99 +56:11:30.8
00:58:14.09 +60:18:23.5
02:17:30.25 +56:22:50.2
01:12:59.76 +57:33:52.4
00:49:18.55 +65:56:10.8
01:30:34.21 +59:44:32.0
01:13:01.33 +61:00:58.3
01:02:18.44 +60:28:18.8
00:44:18.35 +64:55:16.2
02:32:09.71 +57:05:33.2
01:03:55.36 +59:40:27.1
02:12:41.30 +62:42:19.4
00:41:18.92 +60:08:55.3
01:05:58.37 +57:11:40.4
01:39:34.88 +57:01:21.5
00:46:51.53 +58:59:59.8
00:53:08.48 +64:49:01.1
01:11:50.78 +61:46:45.6
02:08:04.25 +58:11:23.1
02:18:03.99 +56:20:30.9
00:51:14.86 +61:05:30.2
01:29:58.56 +63:18:25.9
02:08:50.87 +57:39:27.2
02:46:16.46 +65:01:23.9
02:31:03.24 +56:42:27.2
01:02:12.18 +57:26:33.6
01:11:44.80 +61:13:57.3
00:49:39.69 +61:23:34.4
00:47:23.55 +61:04:59.8
01:35:32.85 +57:32:34.4
00:44:21.47 +58:18:53.3
01:06:13.02 +59:33:47.1
01:13:44.64 +57:24:50.1
00:38:16.23 +61:49:05.9
01:30:26.42 +58:11:55.8
01:02:05.20 +57:40:27.8
01:50:50.32 +57:13:03.4
00:41:02.79 +63:36:12.4
01:35:27.63 +60:33:46.7
02:10:55.92 +62:17:08.9
02:25:34.99 +57:05:41.3
01:50:40.43 +57:43:29.4
01:31:23.18 +59:33:44.1
00:53:53.44 +63:42:25.3
00:36:46.02 +61:48:23.6
00:59:54.65 +59:58:35.3
00:53:44.86 +60:23:25.2
01:32:21.95 +60:27:29.1
00:51:03.58 +65:42:57.2
00:51:29.89 +65:11:40.6
00:51:33.76 +58:43:24.3
01:44:30.72 +57:38:51.1
02:04:04.10 +64:05:48.9
01:07:34.08 +60:52:43.7
01:03:21.67 +58:04:37.8
00:54:13.13 +64:20:25.0
01:42:44.36 +58:39:03.4
00:54:30.87 +59:24:00.8
00:45:45.53 +59:54:30.7
00:58:15.67 +62:45:20.2
01:19:24.09 +58:26:40.3
01:32:19.13 +59:45:28.6
01:17:48.27 +57:17:35.5
01:29:33.76 +57:55:08.9
01:38:10.65 +60:44:57.1
01:25:15.49 +64:40:35.1
01:00:37.27 +58:32:33.2
00:51:09.10 +60:42:14.5
02:04:10.77 +57:54:39.3
01:14:22.29 +57:12:42.3
01:03:35.50 +60:28:06.7
00:50:30.95 +58:09:49.1
00:47:11.40 +58:35:25.7
02:11:52.89 +59:02:30.7
01:02:45.68 +58:39:34.8
01:01:40.14 +64:15:03.0
00:53:20.61 +57:37:02.3
01:03:04.31 +57:50:55.9
01:45:34.97 +59:18:10.9
01:03:02.73 +58:09:40.5
01:27:35.64 +57:56:59.8
01:46:34.07 +59:44:09.6
00:52:55.23 +58:28:51.8
01:25:38.40 +59:16:00.1
01:49:03.59 +61:04:33.8
01:11:16.06 +61:08:30.1
00:51:25.61 +62:25:15.4
00:56:45.56 +58:52:45.9
01:01:40.03 +58:50:24.2
01:25:26.55 +60:57:45.1
01:01:25.47 +57:50:13.8
02:22:36.82 +56:49:53.5
02:26:52.85 +57:11:10.4
00:40:25.93 +61:07:16.2
01:53:47.19 +60:15:59.3
00:51:21.61 +57:15:53.7
01:35:23.69 +60:39:00.6
00:55:44.64 +58:25:59.4
01:28:26.73 +60:23:26.9
00:58:00.34 +57:24:03.5
00:50:57.59 +60:47:11.6
00:36:43.22 +64:22:48.1
02:31:49.82 +56:26:31.7
00:52:48.90 +64:02:29.2
01:20:24.34 +59:10:25.1
01:52:09.01 +58:27:40.6
00:52:40.01 +60:08:46.7
01:19:47.65 +61:38:29.2
01:25:56.72 +59:35:11.7
02:34:02.55 +56:37:43.2
01:40:53.21 +57:14:54.4
00:40:25.55 +62:13:05.2
00:54:29.86 +59:30:21.8
02:36:31.37 +57:11:41.5
02:30:45.63 +55:56:53.3
02:31:26.25 +55:59:07.8
02:34:11.08 +55:50:02.2
02:34:34.68 +56:21:56.3
02:34:44.54 +56:06:08.1
02:33:35.07 +55:54:27.1
01:47:13.15 +57:44:19.2
02:31:46.11 +55:57:58.2
02:33:34.64 +56:11:51.0
02:32:14.58 +55:56:24.6
02:34:13.31 +56:12:38.9
02:35:29.23 +56:28:22.8
02:33:05.57 +56:13:00.8
02:31:00.53 +56:00:30.9
01:44:52.14 +57:41:43.0
00:59:37.43 +59:16:40.0
00:41:14.50 +61:35:32.2
02:33:34.36 +55:49:28.4
02:30:44.35 +55:58:12.9
02:34:13.08 +56:11:55.4
02:33:52.04 +56:11:00.6
02:34:03.60 +56:00:36.3
02:33:51.13 +55:59:56.4
02:33:43.06 +55:51:19.0
02:34:08.57 +55:49:36.3
02:34:14.08 +56:19:37.9
02:33:49.28 +55:57:07.5
02:30:41.72 +55:56:24.9
02:34:22.75 +56:20:28.3
02:35:16.32 +56:26:20.6
02:32:37.64 +56:00:40.9
02:33:06.79 +56:00:36.9
01:21:20.04 +56:57:25.3
02:33:40.44 +56:00:07.9
02:33:28.43 +56:01:32.1
02:34:32.09 +56:11:10.8
02:34:06.92 +56:06:17.2
02:29:26.16 +55:58:53.6
01:48:07.33 +59:50:53.1
02:34:41.51 +56:11:02.0
02:34:19.33 +56:07:37.8
02:32:01.75 +55:53:20.4
02:31:04.78 +56:05:05.6
02:34:14.64 +56:14:11.5
02:32:30.22 +55:59:10.3
01:58:16.32 +59:38:59.1
02:34:10.27 +56:06:39.8
00:55:26.78 +60:51:04.8
01:18:14.18 +61:44:36.2
02:34:25.79 +56:10:43.4
02:33:11.33 +56:00:07.8
02:34:50.95 +56:14:16.1
02:32:09.03 +55:55:39.6
01:14:45.30 +60:30:04.8
02:31:58.20 +56:05:41.8
01:54:04.65 +57:00:35.8
01:18:28.22 +58:11:22.5
01:58:55.84 +57:26:42.4
01:03:22.70 +60:32:14.0
01:44:32.29 +58:45:36.3
02:31:42.28 +56:00:52.2
02:32:31.89 +56:04:32.8
02:33:01.37 +56:09:30.5
02:33:07.17 +56:01:46.1
02:30:56.83 +56:00:04.8
02:32:56.82 +56:04:05.6
02:31:53.23 +55:53:50.7
01:33:15.70 +56:57:52.0
02:34:47.05 +56:16:36.7
02:31:23.81 +55:56:10.2
01:16:30.98 +57:14:55.3
00:51:32.85 +59:59:13.6
02:35:07.08 +56:20:15.3
00:47:11.29 +58:29:06.0
00:33:46.94 +63:27:56.6
01:51:54.81 +57:35:15.7
01:05:57.35 +63:03:31.2
02:33:21.52 +56:04:02.2
02:33:20.71 +55:51:56.8
02:32:39.77 +55:52:01.6
01:46:13.78 +57:54:08.3
02:34:48.63 +56:07:35.8
01:17:41.01 +57:07:19.9
02:30:39.08 +56:07:12.9
01:01:14.73 +57:14:39.1
02:07:35.01 +56:36:56.3
02:37:49.70 +57:46:16.6
02:34:28.10 +56:04:39.7
02:33:15.77 +55:52:19.1
02:32:04.79 +56:03:54.2
01:09:22.48 +57:26:31.4
02:30:46.93 +55:56:09.0
02:11:23.25 +61:21:06.1
01:35:19.56 +58:24:48.5
01:58:40.24 +59:15:59.7
02:30:44.71 +56:03:12.4
01:00:17.82 +60:23:28.8
02:33:51.70 +56:01:15.0
02:32:26.77 +56:07:14.1
02:33:31.71 +55:59:51.2
02:32:17.00 +55:59:24.0
00:57:06.54 +58:58:31.2
02:34:06.54 +56:16:48.1
01:53:10.31 +58:09:47.0
01:25:06.70 +59:33:57.1
02:32:53.75 +56:02:28.7
02:33:02.37 +56:01:38.3
01:04:33.85 +57:23:33.9
02:31:19.12 +56:02:17.6
01:46:38.52 +60:07:33.4
02:33:17.19 +56:06:00.2
01:38:07.73 +61:01:40.6
00:55:18.16 +60:03:32.6
01:19:41.36 +62:51:05.1
02:18:59.76 +57:04:00.7
02:33:57.45 +56:01:33.1
02:34:24.39 +55:59:28.1
02:32:04.89 +55:55:17.2
01:44:30.83 +57:33:34.1
02:33:36.90 +55:50:23.1
01:13:54.30 +58:12:33.7
02:19:57.86 +59:32:26.9
02:34:47.29 +56:12:09.8
02:34:19.23 +56:15:01.8
00:50:03.30 +57:23:20.9
02:07:25.40 +57:54:58.4
02:10:23.96 +60:01:13.7
02:33:04.96 +56:00:14.2
01:11:41.02 +58:17:27.9
01:59:33.38 +60:01:45.4
01:48:01.86 +57:39:19.3
02:29:49.57 +56:00:09.6
02:34:55.55 +56:12:20.3
01:13:38.95 +58:10:50.4
02:32:38.56 +55:54:40.8
02:21:28.82 +63:55:29.7
02:34:28.15 +56:03:40.0
01:38:33.84 +60:47:24.6
02:35:13.46 +56:19:56.7
00:56:42.62 +58:03:48.0
01:57:13.86 +57:26:43.7
02:28:46.17 +56:02:23.7
02:31:39.66 +56:01:58.4
01:38:06.27 +58:10:40.1
00:50:31.13 +64:31:47.5
01:46:23.23 +61:12:56.7
01:26:28.54 +59:41:35.0
02:34:09.98 +55:51:55.6
01:59:05.94 +59:55:34.3
01:28:07.91 +58:50:39.6
02:34:19.54 +56:15:41.6
00:44:10.04 +64:27:25.8
02:32:09.39 +56:09:40.6
01:43:03.30 +58:57:12.9
02:02:53.90 +60:15:42.0
02:33:46.62 +55:56:04.6
02:35:02.29 +56:14:22.9
01:24:55.22 +57:12:20.0
01:34:42.46 +58:42:15.2
02:05:23.30 +59:19:31.5
02:32:58.07 +56:06:56.5
01:19:29.17 +59:25:20.5
01:36:50.88 +59:55:48.3
02:39:10.93 +63:43:59.5
02:20:14.56 +59:20:12.7
02:32:27.21 +55:53:12.4
00:50:58.17 +59:43:06.7
01:48:30.79 +58:02:54.6
02:33:09.09 +56:06:53.6
01:25:45.38 +59:01:19.8
00:59:00.02 +59:04:33.1
01:52:55.36 +59:33:30.6
01:08:11.66 +62:14:23.2
01:46:56.97 +57:21:54.8
02:02:32.20 +58:06:03.8
00:58:34.73 +57:44:23.1
01:36:37.08 +58:44:43.7
02:32:25.16 +56:00:34.4
01:31:55.84 +59:26:39.9
01:07:30.37 +60:38:18.7
02:44:06.26 +62:20:01.3
01:29:32.61 +63:18:22.4
########### Completed Cas-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
00:37:00.24 +63:08:01.5
01:49:54.28 +63:40:38.1
01:26:01.91 +57:08:04.9
01:57:29.18 +60:09:19.3
01:50:10.11 +57:10:52.0
01:29:45.03 +59:58:32.3
01:11:20.01 +61:17:54.4
01:10:01.79 +66:17:40.5
02:30:11.32 +66:01:46.4
01:02:07.21 +61:19:23.6
01:58:50.68 +56:57:17.7
01:19:26.87 +57:22:51.4
01:22:50.45 +58:12:42.0
02:03:02.00 +56:50:06.8
01:06:16.04 +57:53:24.3
01:15:36.33 +63:27:54.0
01:27:12.82 +58:27:16.9
01:47:04.43 +59:18:55.3
01:13:09.81 +64:30:33.5
00:49:57.44 +60:17:56.5
00:44:47.70 +66:11:33.2
01:09:10.52 +58:09:35.5
01:08:39.16 +60:32:40.7
02:21:32.56 +56:32:12.5
01:10:12.02 +59:17:25.4
01:50:46.76 +58:00:38.2
01:07:39.08 +59:59:18.1
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02:33:49.28 +55:57:07.5
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02:33:06.79 +56:00:36.9
01:21:20.04 +56:57:25.3
02:33:40.44 +56:00:07.9
02:33:28.43 +56:01:32.1
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02:34:06.92 +56:06:17.2
02:29:26.16 +55:58:53.6
01:48:07.33 +59:50:53.1
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02:32:01.75 +55:53:20.4
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02:32:30.22 +55:59:10.3
01:58:16.32 +59:38:59.1
02:34:10.27 +56:06:39.8
00:55:26.78 +60:51:04.8
01:18:14.18 +61:44:36.2
02:34:25.79 +56:10:43.4
02:33:11.33 +56:00:07.8
02:34:50.95 +56:14:16.1
02:32:09.03 +55:55:39.6
01:14:45.30 +60:30:04.8
02:31:58.20 +56:05:41.8
01:54:04.65 +57:00:35.8
01:18:28.22 +58:11:22.5
01:58:55.84 +57:26:42.4
01:03:22.70 +60:32:14.0
01:44:32.29 +58:45:36.3
02:31:42.28 +56:00:52.2
02:32:31.89 +56:04:32.8
02:33:01.37 +56:09:30.5
02:33:07.17 +56:01:46.1
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02:32:56.82 +56:04:05.6
02:31:53.23 +55:53:50.7
01:33:15.70 +56:57:52.0
02:34:47.05 +56:16:36.7
02:31:23.81 +55:56:10.2
01:16:30.98 +57:14:55.3
00:51:32.85 +59:59:13.6
02:35:07.08 +56:20:15.3
00:47:11.29 +58:29:06.0
00:33:46.94 +63:27:56.6
01:51:54.81 +57:35:15.7
01:05:57.35 +63:03:31.2
02:33:21.52 +56:04:02.2
02:33:20.71 +55:51:56.8
02:32:39.77 +55:52:01.6
01:46:13.78 +57:54:08.3
02:34:48.63 +56:07:35.8
01:17:41.01 +57:07:19.9
02:30:39.08 +56:07:12.9
01:01:14.73 +57:14:39.1
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02:37:49.70 +57:46:16.6
02:34:28.10 +56:04:39.7
02:33:15.77 +55:52:19.1
02:32:04.79 +56:03:54.2
01:09:22.48 +57:26:31.4
02:30:46.93 +55:56:09.0
02:11:23.25 +61:21:06.1
01:35:19.56 +58:24:48.5
01:58:40.24 +59:15:59.7
02:30:44.71 +56:03:12.4
01:00:17.82 +60:23:28.8
02:33:51.70 +56:01:15.0
02:32:26.77 +56:07:14.1
02:33:31.71 +55:59:51.2
02:32:17.00 +55:59:24.0
00:57:06.54 +58:58:31.2
02:34:06.54 +56:16:48.1
01:53:10.31 +58:09:47.0
01:25:06.70 +59:33:57.1
02:32:53.75 +56:02:28.7
02:33:02.37 +56:01:38.3
01:04:33.85 +57:23:33.9
02:31:19.12 +56:02:17.6
01:46:38.52 +60:07:33.4
02:33:17.19 +56:06:00.2
01:38:07.73 +61:01:40.6
00:55:18.16 +60:03:32.6
01:19:41.36 +62:51:05.1
02:18:59.76 +57:04:00.7
02:33:57.45 +56:01:33.1
02:34:24.39 +55:59:28.1
02:32:04.89 +55:55:17.2
01:44:30.83 +57:33:34.1
02:33:36.90 +55:50:23.1
01:13:54.30 +58:12:33.7
02:19:57.86 +59:32:26.9
02:34:47.29 +56:12:09.8
02:34:19.23 +56:15:01.8
00:50:03.30 +57:23:20.9
02:07:25.40 +57:54:58.4
02:10:23.96 +60:01:13.7
02:33:04.96 +56:00:14.2
01:11:41.02 +58:17:27.9
01:59:33.38 +60:01:45.4
01:48:01.86 +57:39:19.3
02:29:49.57 +56:00:09.6
02:34:55.55 +56:12:20.3
01:13:38.95 +58:10:50.4
02:32:38.56 +55:54:40.8
02:21:28.82 +63:55:29.7
02:34:28.15 +56:03:40.0
01:38:33.84 +60:47:24.6
02:35:13.46 +56:19:56.7
00:56:42.62 +58:03:48.0
01:57:13.86 +57:26:43.7
02:28:46.17 +56:02:23.7
02:31:39.66 +56:01:58.4
01:38:06.27 +58:10:40.1
00:50:31.13 +64:31:47.5
01:46:23.23 +61:12:56.7
01:26:28.54 +59:41:35.0
02:34:09.98 +55:51:55.6
01:59:05.94 +59:55:34.3
01:28:07.91 +58:50:39.6
02:34:19.54 +56:15:41.6
00:44:10.04 +64:27:25.8
02:32:09.39 +56:09:40.6
01:43:03.30 +58:57:12.9
02:02:53.90 +60:15:42.0
02:33:46.62 +55:56:04.6
02:35:02.29 +56:14:22.9
01:24:55.22 +57:12:20.0
01:34:42.46 +58:42:15.2
02:05:23.30 +59:19:31.5
02:32:58.07 +56:06:56.5
01:19:29.17 +59:25:20.5
01:36:50.88 +59:55:48.3
02:39:10.93 +63:43:59.5
02:20:14.56 +59:20:12.7
02:32:27.21 +55:53:12.4
00:50:58.17 +59:43:06.7
01:48:30.79 +58:02:54.6
02:33:09.09 +56:06:53.6
01:25:45.38 +59:01:19.8
00:59:00.02 +59:04:33.1
01:52:55.36 +59:33:30.6
01:08:11.66 +62:14:23.2
01:46:56.97 +57:21:54.8
02:02:32.20 +58:06:03.8
00:58:34.73 +57:44:23.1
01:36:37.08 +58:44:43.7
02:32:25.16 +56:00:34.4
01:31:55.84 +59:26:39.9
01:07:30.37 +60:38:18.7
02:28:46.53 +56:00:06.1
02:32:01.70 +57:03:30.6
02:26:40.29 +56:09:51.2
02:27:56.21 +56:10:22.8
01:29:32.61 +63:18:22.4
02:34:00.02 +55:56:27.7
02:29:11.65 +56:22:44.6
02:33:51.39 +55:58:25.7
02:33:52.85 +56:31:18.5
02:34:27.89 +57:30:42.7
02:34:13.39 +56:03:48.2
02:44:06.26 +62:20:01.3
02:34:05.94 +56:37:27.5
02:27:52.20 +56:32:26.7
02:29:03.07 +56:34:20.1
02:46:03.81 +63:32:43.3
02:49:57.09 +63:51:39.7
02:28:35.24 +56:03:02.7
###################################################################################
00:37:00.24 +63:08:01.5 -- not an asteroid (will add it to exclusion list)
01:49:54.28 +63:40:38.1 -- not an asteroid (will add it to exclusion list)
01:26:01.91 +57:08:04.9 -- not an asteroid (will add it to exclusion list)
01:57:29.18 +60:09:19.3 -- not an asteroid (will add it to exclusion list)
01:50:10.11 +57:10:52.0 -- not an asteroid (will add it to exclusion list)
01:29:45.03 +59:58:32.3 -- not an asteroid (will add it to exclusion list)
01:11:20.01 +61:17:54.4 -- not an asteroid (will add it to exclusion list)
01:10:01.79 +66:17:40.5 -- not an asteroid (will add it to exclusion list)
02:30:11.32 +66:01:46.4 -- not an asteroid (will add it to exclusion list)
01:02:07.21 +61:19:23.6 -- not an asteroid (will add it to exclusion list)
01:58:50.68 +56:57:17.7 -- not an asteroid (will add it to exclusion list)
01:19:26.87 +57:22:51.4 -- not an asteroid (will add it to exclusion list)
01:22:50.45 +58:12:42.0 -- not an asteroid (will add it to exclusion list)
02:03:02.00 +56:50:06.8 -- not an asteroid (will add it to exclusion list)
01:06:16.04 +57:53:24.3 -- not an asteroid (will add it to exclusion list)
01:15:36.33 +63:27:54.0 -- not an asteroid (will add it to exclusion list)
01:27:12.82 +58:27:16.9 -- not an asteroid (will add it to exclusion list)
01:47:04.43 +59:18:55.3 -- not an asteroid (will add it to exclusion list)
01:13:09.81 +64:30:33.5 -- not an asteroid (will add it to exclusion list)
00:49:57.44 +60:17:56.5 -- not an asteroid (will add it to exclusion list)
00:44:47.70 +66:11:33.2 -- not an asteroid (will add it to exclusion list)
01:09:10.52 +58:09:35.5 -- not an asteroid (will add it to exclusion list)
01:08:39.16 +60:32:40.7 -- not an asteroid (will add it to exclusion list)
02:21:32.56 +56:32:12.5 -- not an asteroid (will add it to exclusion list)
01:10:12.02 +59:17:25.4 -- not an asteroid (will add it to exclusion list)
01:50:46.76 +58:00:38.2 -- not an asteroid (will add it to exclusion list)
01:07:39.08 +59:59:18.1 -- not an asteroid (will add it to exclusion list)
01:09:22.85 +58:34:03.2 -- not an asteroid (will add it to exclusion list)
01:06:37.45 +60:22:38.2 -- not an asteroid (will add it to exclusion list)
01:15:44.77 +60:02:45.6 -- not an asteroid (will add it to exclusion list)
01:29:49.42 +58:16:02.6 -- not an asteroid (will add it to exclusion list)
01:25:52.13 +57:05:24.0 -- not an asteroid (will add it to exclusion list)
01:07:00.11 +61:28:29.9 -- not an asteroid (will add it to exclusion list)
01:01:11.29 +65:10:55.4 -- not an asteroid (will add it to exclusion list)
02:47:22.83 +63:30:07.2 -- not an asteroid (will add it to exclusion list)
00:46:55.69 +60:00:23.1 -- not an asteroid (will add it to exclusion list)
01:47:27.75 +64:31:09.8 -- not an asteroid (will add it to exclusion list)
02:24:32.99 +56:11:30.8 -- not an asteroid (will add it to exclusion list)
00:58:14.09 +60:18:23.5 -- not an asteroid (will add it to exclusion list)
02:17:30.25 +56:22:50.2 -- not an asteroid (will add it to exclusion list)
01:12:59.76 +57:33:52.4 -- not an asteroid (will add it to exclusion list)
00:49:18.55 +65:56:10.8 -- not an asteroid (will add it to exclusion list)
01:30:34.21 +59:44:32.0 -- not an asteroid (will add it to exclusion list)
01:13:01.33 +61:00:58.3 -- not an asteroid (will add it to exclusion list)
01:02:18.44 +60:28:18.8 -- not an asteroid (will add it to exclusion list)
00:44:18.35 +64:55:16.2 -- not an asteroid (will add it to exclusion list)
02:32:09.71 +57:05:33.2 -- not an asteroid (will add it to exclusion list)
01:03:55.36 +59:40:27.1 -- not an asteroid (will add it to exclusion list)
02:12:41.30 +62:42:19.4 -- not an asteroid (will add it to exclusion list)
00:41:18.92 +60:08:55.3 -- not an asteroid (will add it to exclusion list)
01:05:58.37 +57:11:40.4 -- not an asteroid (will add it to exclusion list)
01:39:34.88 +57:01:21.5 -- not an asteroid (will add it to exclusion list)
00:46:51.53 +58:59:59.8 -- not an asteroid (will add it to exclusion list)
00:53:08.48 +64:49:01.1 -- not an asteroid (will add it to exclusion list)
01:11:50.78 +61:46:45.6 -- not an asteroid (will add it to exclusion list)
02:08:04.25 +58:11:23.1 -- not an asteroid (will add it to exclusion list)
02:18:03.99 +56:20:30.9 -- not an asteroid (will add it to exclusion list)
00:51:14.86 +61:05:30.2 -- not an asteroid (will add it to exclusion list)
01:29:58.56 +63:18:25.9 -- not an asteroid (will add it to exclusion list)
02:08:50.87 +57:39:27.2 -- not an asteroid (will add it to exclusion list)
02:46:16.46 +65:01:23.9 -- not an asteroid (will add it to exclusion list)
02:31:03.24 +56:42:27.2 -- not an asteroid (will add it to exclusion list)
01:02:12.18 +57:26:33.6 -- not an asteroid (will add it to exclusion list)
01:11:44.80 +61:13:57.3 -- not an asteroid (will add it to exclusion list)
00:49:39.69 +61:23:34.4 -- not an asteroid (will add it to exclusion list)
00:47:23.55 +61:04:59.8 -- not an asteroid (will add it to exclusion list)
01:35:32.85 +57:32:34.4 -- not an asteroid (will add it to exclusion list)
00:44:21.47 +58:18:53.3 -- not an asteroid (will add it to exclusion list)
01:06:13.02 +59:33:47.1 -- not an asteroid (will add it to exclusion list)
01:13:44.64 +57:24:50.1 -- not an asteroid (will add it to exclusion list)
00:38:16.23 +61:49:05.9 -- not an asteroid (will add it to exclusion list)
01:30:26.42 +58:11:55.8 -- not an asteroid (will add it to exclusion list)
01:02:05.20 +57:40:27.8 -- not an asteroid (will add it to exclusion list)
01:50:50.32 +57:13:03.4 -- not an asteroid (will add it to exclusion list)
00:41:02.79 +63:36:12.4 -- not an asteroid (will add it to exclusion list)
01:35:27.63 +60:33:46.7 -- not an asteroid (will add it to exclusion list)
02:10:55.92 +62:17:08.9 -- not an asteroid (will add it to exclusion list)
02:25:34.99 +57:05:41.3 -- not an asteroid (will add it to exclusion list)
01:50:40.43 +57:43:29.4 -- not an asteroid (will add it to exclusion list)
01:31:23.18 +59:33:44.1 -- not an asteroid (will add it to exclusion list)
00:53:53.44 +63:42:25.3 -- not an asteroid (will add it to exclusion list)
00:36:46.02 +61:48:23.6 -- not an asteroid (will add it to exclusion list)
00:59:54.65 +59:58:35.3 -- not an asteroid (will add it to exclusion list)
00:53:44.86 +60:23:25.2 -- not an asteroid (will add it to exclusion list)
01:32:21.95 +60:27:29.1 -- not an asteroid (will add it to exclusion list)
00:51:03.58 +65:42:57.2 -- not an asteroid (will add it to exclusion list)
00:51:29.89 +65:11:40.6 -- not an asteroid (will add it to exclusion list)
00:51:33.76 +58:43:24.3 -- not an asteroid (will add it to exclusion list)
01:44:30.72 +57:38:51.1 -- not an asteroid (will add it to exclusion list)
02:04:04.10 +64:05:48.9 -- not an asteroid (will add it to exclusion list)
01:07:34.08 +60:52:43.7 -- not an asteroid (will add it to exclusion list)
01:03:21.67 +58:04:37.8 -- not an asteroid (will add it to exclusion list)
00:54:13.13 +64:20:25.0 -- not an asteroid (will add it to exclusion list)
01:42:44.36 +58:39:03.4 -- not an asteroid (will add it to exclusion list)
00:54:30.87 +59:24:00.8 -- not an asteroid (will add it to exclusion list)
00:45:45.53 +59:54:30.7 -- not an asteroid (will add it to exclusion list)
00:58:15.67 +62:45:20.2 -- not an asteroid (will add it to exclusion list)
01:19:24.09 +58:26:40.3 -- not an asteroid (will add it to exclusion list)
01:32:19.13 +59:45:28.6 -- not an asteroid (will add it to exclusion list)
01:17:48.27 +57:17:35.5 -- not an asteroid (will add it to exclusion list)
01:29:33.76 +57:55:08.9 -- not an asteroid (will add it to exclusion list)
01:38:10.65 +60:44:57.1 -- not an asteroid (will add it to exclusion list)
01:25:15.49 +64:40:35.1 -- not an asteroid (will add it to exclusion list)
01:00:37.27 +58:32:33.2 -- not an asteroid (will add it to exclusion list)
00:51:09.10 +60:42:14.5 -- not an asteroid (will add it to exclusion list)
02:04:10.77 +57:54:39.3 -- not an asteroid (will add it to exclusion list)
01:14:22.29 +57:12:42.3 -- not an asteroid (will add it to exclusion list)
01:03:35.50 +60:28:06.7 -- not an asteroid (will add it to exclusion list)
00:50:30.95 +58:09:49.1 -- not an asteroid (will add it to exclusion list)
00:47:11.40 +58:35:25.7 -- not an asteroid (will add it to exclusion list)
02:11:52.89 +59:02:30.7 -- not an asteroid (will add it to exclusion list)
01:02:45.68 +58:39:34.8 -- not an asteroid (will add it to exclusion list)
01:01:40.14 +64:15:03.0 -- not an asteroid (will add it to exclusion list)
00:53:20.61 +57:37:02.3 -- not an asteroid (will add it to exclusion list)
01:03:04.31 +57:50:55.9 -- not an asteroid (will add it to exclusion list)
01:45:34.97 +59:18:10.9 -- not an asteroid (will add it to exclusion list)
01:03:02.73 +58:09:40.5 -- not an asteroid (will add it to exclusion list)
01:27:35.64 +57:56:59.8 -- not an asteroid (will add it to exclusion list)
01:46:34.07 +59:44:09.6 -- not an asteroid (will add it to exclusion list)
00:52:55.23 +58:28:51.8 -- not an asteroid (will add it to exclusion list)
01:25:38.40 +59:16:00.1 -- not an asteroid (will add it to exclusion list)
01:49:03.59 +61:04:33.8 -- not an asteroid (will add it to exclusion list)
01:11:16.06 +61:08:30.1 -- not an asteroid (will add it to exclusion list)
00:51:25.61 +62:25:15.4 -- not an asteroid (will add it to exclusion list)
00:56:45.56 +58:52:45.9 -- not an asteroid (will add it to exclusion list)
01:01:40.03 +58:50:24.2 -- not an asteroid (will add it to exclusion list)
01:25:26.55 +60:57:45.1 -- not an asteroid (will add it to exclusion list)
01:01:25.47 +57:50:13.8 -- not an asteroid (will add it to exclusion list)
02:22:36.82 +56:49:53.5 -- not an asteroid (will add it to exclusion list)
02:26:52.85 +57:11:10.4 -- not an asteroid (will add it to exclusion list)
00:40:25.93 +61:07:16.2 -- not an asteroid (will add it to exclusion list)
01:53:47.19 +60:15:59.3 -- not an asteroid (will add it to exclusion list)
00:51:21.61 +57:15:53.7 -- not an asteroid (will add it to exclusion list)
01:35:23.69 +60:39:00.6 -- not an asteroid (will add it to exclusion list)
00:55:44.64 +58:25:59.4 -- not an asteroid (will add it to exclusion list)
01:28:26.73 +60:23:26.9 -- not an asteroid (will add it to exclusion list)
00:58:00.34 +57:24:03.5 -- not an asteroid (will add it to exclusion list)
00:50:57.59 +60:47:11.6 -- not an asteroid (will add it to exclusion list)
00:36:43.22 +64:22:48.1 -- not an asteroid (will add it to exclusion list)
02:31:49.82 +56:26:31.7 -- not an asteroid (will add it to exclusion list)
00:52:48.90 +64:02:29.2 -- not an asteroid (will add it to exclusion list)
01:20:24.34 +59:10:25.1 -- not an asteroid (will add it to exclusion list)
01:52:09.01 +58:27:40.6 -- not an asteroid (will add it to exclusion list)
00:52:40.01 +60:08:46.7 -- not an asteroid (will add it to exclusion list)
01:19:47.65 +61:38:29.2 -- not an asteroid (will add it to exclusion list)
01:25:56.72 +59:35:11.7 -- not an asteroid (will add it to exclusion list)
02:34:02.55 +56:37:43.2 -- not an asteroid (will add it to exclusion list)
01:40:53.21 +57:14:54.4 -- not an asteroid (will add it to exclusion list)
00:40:25.55 +62:13:05.2 -- not an asteroid (will add it to exclusion list)
00:54:29.86 +59:30:21.8 -- not an asteroid (will add it to exclusion list)
02:36:31.37 +57:11:41.5 -- not an asteroid (will add it to exclusion list)
02:30:45.63 +55:56:53.3 -- not an asteroid (will add it to exclusion list)
02:31:26.25 +55:59:07.8 -- not an asteroid (will add it to exclusion list)
02:34:11.08 +55:50:02.2 -- not an asteroid (will add it to exclusion list)
02:34:34.68 +56:21:56.3 -- not an asteroid (will add it to exclusion list)
02:34:44.54 +56:06:08.1 -- not an asteroid (will add it to exclusion list)
02:33:35.07 +55:54:27.1 -- not an asteroid (will add it to exclusion list)
01:47:13.15 +57:44:19.2 -- not an asteroid (will add it to exclusion list)
02:31:46.11 +55:57:58.2 -- not an asteroid (will add it to exclusion list)
02:33:34.64 +56:11:51.0 -- not an asteroid (will add it to exclusion list)
02:32:14.58 +55:56:24.6 -- not an asteroid (will add it to exclusion list)
02:34:13.31 +56:12:38.9 -- not an asteroid (will add it to exclusion list)
02:35:29.23 +56:28:22.8 -- not an asteroid (will add it to exclusion list)
02:33:05.57 +56:13:00.8 -- not an asteroid (will add it to exclusion list)
02:31:00.53 +56:00:30.9 -- not an asteroid (will add it to exclusion list)
01:44:52.14 +57:41:43.0 -- not an asteroid (will add it to exclusion list)
00:59:37.43 +59:16:40.0 -- not an asteroid (will add it to exclusion list)
00:41:14.50 +61:35:32.2 -- not an asteroid (will add it to exclusion list)
02:33:34.36 +55:49:28.4 -- not an asteroid (will add it to exclusion list)
02:30:44.35 +55:58:12.9 -- not an asteroid (will add it to exclusion list)
02:34:13.08 +56:11:55.4 -- not an asteroid (will add it to exclusion list)
02:33:52.04 +56:11:00.6 -- not an asteroid (will add it to exclusion list)
02:34:03.60 +56:00:36.3 -- not an asteroid (will add it to exclusion list)
02:33:51.13 +55:59:56.4 -- not an asteroid (will add it to exclusion list)
02:33:43.06 +55:51:19.0 -- not an asteroid (will add it to exclusion list)
02:34:08.57 +55:49:36.3 -- not an asteroid (will add it to exclusion list)
02:34:14.08 +56:19:37.9 -- not an asteroid (will add it to exclusion list)
02:33:49.28 +55:57:07.5 -- not an asteroid (will add it to exclusion list)
02:30:41.72 +55:56:24.9 -- not an asteroid (will add it to exclusion list)
02:34:22.75 +56:20:28.3 -- not an asteroid (will add it to exclusion list)
02:35:16.32 +56:26:20.6 -- not an asteroid (will add it to exclusion list)
02:32:37.64 +56:00:40.9 -- not an asteroid (will add it to exclusion list)
02:33:06.79 +56:00:36.9 -- not an asteroid (will add it to exclusion list)
01:21:20.04 +56:57:25.3 -- not an asteroid (will add it to exclusion list)
02:33:40.44 +56:00:07.9 -- not an asteroid (will add it to exclusion list)
02:33:28.43 +56:01:32.1 -- not an asteroid (will add it to exclusion list)
02:34:32.09 +56:11:10.8 -- not an asteroid (will add it to exclusion list)
02:34:06.92 +56:06:17.2 -- not an asteroid (will add it to exclusion list)
02:29:26.16 +55:58:53.6 -- not an asteroid (will add it to exclusion list)
01:48:07.33 +59:50:53.1 -- not an asteroid (will add it to exclusion list)
02:34:41.51 +56:11:02.0 -- not an asteroid (will add it to exclusion list)
02:34:19.33 +56:07:37.8 -- not an asteroid (will add it to exclusion list)
02:32:01.75 +55:53:20.4 -- not an asteroid (will add it to exclusion list)
02:31:04.78 +56:05:05.6 -- not an asteroid (will add it to exclusion list)
02:34:14.64 +56:14:11.5 -- not an asteroid (will add it to exclusion list)
02:32:30.22 +55:59:10.3 -- not an asteroid (will add it to exclusion list)
01:58:16.32 +59:38:59.1 -- not an asteroid (will add it to exclusion list)
02:34:10.27 +56:06:39.8 -- not an asteroid (will add it to exclusion list)
00:55:26.78 +60:51:04.8 -- not an asteroid (will add it to exclusion list)
01:18:14.18 +61:44:36.2 -- not an asteroid (will add it to exclusion list)
02:34:25.79 +56:10:43.4 -- not an asteroid (will add it to exclusion list)
02:33:11.33 +56:00:07.8 -- not an asteroid (will add it to exclusion list)
02:34:50.95 +56:14:16.1 -- not an asteroid (will add it to exclusion list)
02:32:09.03 +55:55:39.6 -- not an asteroid (will add it to exclusion list)
01:14:45.30 +60:30:04.8 -- not an asteroid (will add it to exclusion list)
02:31:58.20 +56:05:41.8 -- not an asteroid (will add it to exclusion list)
01:54:04.65 +57:00:35.8 -- not an asteroid (will add it to exclusion list)
01:18:28.22 +58:11:22.5 -- not an asteroid (will add it to exclusion list)
01:58:55.84 +57:26:42.4 -- not an asteroid (will add it to exclusion list)
01:03:22.70 +60:32:14.0 -- not an asteroid (will add it to exclusion list)
01:44:32.29 +58:45:36.3 -- not an asteroid (will add it to exclusion list)
02:31:42.28 +56:00:52.2 -- not an asteroid (will add it to exclusion list)
02:32:31.89 +56:04:32.8 -- not an asteroid (will add it to exclusion list)
02:33:01.37 +56:09:30.5 -- not an asteroid (will add it to exclusion list)
02:33:07.17 +56:01:46.1 -- not an asteroid (will add it to exclusion list)
02:30:56.83 +56:00:04.8 -- not an asteroid (will add it to exclusion list)
02:32:56.82 +56:04:05.6 -- not an asteroid (will add it to exclusion list)
02:31:53.23 +55:53:50.7 -- not an asteroid (will add it to exclusion list)
01:33:15.70 +56:57:52.0 -- not an asteroid (will add it to exclusion list)
02:34:47.05 +56:16:36.7 -- not an asteroid (will add it to exclusion list)
02:31:23.81 +55:56:10.2 -- not an asteroid (will add it to exclusion list)
01:16:30.98 +57:14:55.3 -- not an asteroid (will add it to exclusion list)
00:51:32.85 +59:59:13.6 -- not an asteroid (will add it to exclusion list)
02:35:07.08 +56:20:15.3 -- not an asteroid (will add it to exclusion list)
00:47:11.29 +58:29:06.0 -- not an asteroid (will add it to exclusion list)
00:33:46.94 +63:27:56.6 -- not an asteroid (will add it to exclusion list)
01:51:54.81 +57:35:15.7 -- not an asteroid (will add it to exclusion list)
01:05:57.35 +63:03:31.2 -- not an asteroid (will add it to exclusion list)
02:33:21.52 +56:04:02.2 -- not an asteroid (will add it to exclusion list)
02:33:20.71 +55:51:56.8 -- not an asteroid (will add it to exclusion list)
02:32:39.77 +55:52:01.6 -- not an asteroid (will add it to exclusion list)
01:46:13.78 +57:54:08.3 -- not an asteroid (will add it to exclusion list)
02:34:48.63 +56:07:35.8 -- not an asteroid (will add it to exclusion list)
01:17:41.01 +57:07:19.9 -- not an asteroid (will add it to exclusion list)
02:30:39.08 +56:07:12.9 -- not an asteroid (will add it to exclusion list)
01:01:14.73 +57:14:39.1 -- not an asteroid (will add it to exclusion list)
02:07:35.01 +56:36:56.3 -- not an asteroid (will add it to exclusion list)
02:37:49.70 +57:46:16.6 -- not an asteroid (will add it to exclusion list)
02:34:28.10 +56:04:39.7 -- not an asteroid (will add it to exclusion list)
02:33:15.77 +55:52:19.1 -- not an asteroid (will add it to exclusion list)
02:32:04.79 +56:03:54.2 -- not an asteroid (will add it to exclusion list)
01:09:22.48 +57:26:31.4 -- not an asteroid (will add it to exclusion list)
02:30:46.93 +55:56:09.0 -- not an asteroid (will add it to exclusion list)
02:11:23.25 +61:21:06.1 -- not an asteroid (will add it to exclusion list)
01:35:19.56 +58:24:48.5 -- not an asteroid (will add it to exclusion list)
01:58:40.24 +59:15:59.7 -- not an asteroid (will add it to exclusion list)
02:30:44.71 +56:03:12.4 -- not an asteroid (will add it to exclusion list)
01:00:17.82 +60:23:28.8 -- not an asteroid (will add it to exclusion list)
02:33:51.70 +56:01:15.0 -- not an asteroid (will add it to exclusion list)
02:32:26.77 +56:07:14.1 -- not an asteroid (will add it to exclusion list)
02:33:31.71 +55:59:51.2 -- not an asteroid (will add it to exclusion list)
02:32:17.00 +55:59:24.0 -- not an asteroid (will add it to exclusion list)
00:57:06.54 +58:58:31.2 -- not an asteroid (will add it to exclusion list)
02:34:06.54 +56:16:48.1 -- not an asteroid (will add it to exclusion list)
01:53:10.31 +58:09:47.0 -- not an asteroid (will add it to exclusion list)
01:25:06.70 +59:33:57.1 -- not an asteroid (will add it to exclusion list)
02:32:53.75 +56:02:28.7 -- not an asteroid (will add it to exclusion list)
02:33:02.37 +56:01:38.3 -- not an asteroid (will add it to exclusion list)
01:04:33.85 +57:23:33.9 -- not an asteroid (will add it to exclusion list)
02:31:19.12 +56:02:17.6 -- not an asteroid (will add it to exclusion list)
01:46:38.52 +60:07:33.4 -- not an asteroid (will add it to exclusion list)
02:33:17.19 +56:06:00.2 -- not an asteroid (will add it to exclusion list)
01:38:07.73 +61:01:40.6 -- not an asteroid (will add it to exclusion list)
00:55:18.16 +60:03:32.6 -- not an asteroid (will add it to exclusion list)
01:19:41.36 +62:51:05.1 -- not an asteroid (will add it to exclusion list)
02:18:59.76 +57:04:00.7 -- not an asteroid (will add it to exclusion list)
02:33:57.45 +56:01:33.1 -- not an asteroid (will add it to exclusion list)
02:34:24.39 +55:59:28.1 -- not an asteroid (will add it to exclusion list)
02:32:04.89 +55:55:17.2 -- not an asteroid (will add it to exclusion list)
01:44:30.83 +57:33:34.1 -- not an asteroid (will add it to exclusion list)
02:33:36.90 +55:50:23.1 -- not an asteroid (will add it to exclusion list)
01:13:54.30 +58:12:33.7 -- not an asteroid (will add it to exclusion list)
02:19:57.86 +59:32:26.9 -- not an asteroid (will add it to exclusion list)
02:34:47.29 +56:12:09.8 -- not an asteroid (will add it to exclusion list)
02:34:19.23 +56:15:01.8 -- not an asteroid (will add it to exclusion list)
00:50:03.30 +57:23:20.9 -- not an asteroid (will add it to exclusion list)
02:07:25.40 +57:54:58.4 -- not an asteroid (will add it to exclusion list)
02:10:23.96 +60:01:13.7 -- not an asteroid (will add it to exclusion list)
02:33:04.96 +56:00:14.2 -- not an asteroid (will add it to exclusion list)
01:11:41.02 +58:17:27.9 -- not an asteroid (will add it to exclusion list)
01:59:33.38 +60:01:45.4 -- not an asteroid (will add it to exclusion list)
01:48:01.86 +57:39:19.3 -- not an asteroid (will add it to exclusion list)
02:29:49.57 +56:00:09.6 -- not an asteroid (will add it to exclusion list)
02:34:55.55 +56:12:20.3 -- not an asteroid (will add it to exclusion list)
01:13:38.95 +58:10:50.4 -- not an asteroid (will add it to exclusion list)
02:32:38.56 +55:54:40.8 -- not an asteroid (will add it to exclusion list)
02:21:28.82 +63:55:29.7 -- not an asteroid (will add it to exclusion list)
02:34:28.15 +56:03:40.0 -- not an asteroid (will add it to exclusion list)
01:38:33.84 +60:47:24.6 -- not an asteroid (will add it to exclusion list)
02:35:13.46 +56:19:56.7 -- not an asteroid (will add it to exclusion list)
00:56:42.62 +58:03:48.0 -- not an asteroid (will add it to exclusion list)
01:57:13.86 +57:26:43.7 -- not an asteroid (will add it to exclusion list)
02:28:46.17 +56:02:23.7 -- not an asteroid (will add it to exclusion list)
02:31:39.66 +56:01:58.4 -- not an asteroid (will add it to exclusion list)
01:38:06.27 +58:10:40.1 -- not an asteroid (will add it to exclusion list)
00:50:31.13 +64:31:47.5 -- not an asteroid (will add it to exclusion list)
01:46:23.23 +61:12:56.7 -- not an asteroid (will add it to exclusion list)
01:26:28.54 +59:41:35.0 -- not an asteroid (will add it to exclusion list)
02:34:09.98 +55:51:55.6 -- not an asteroid (will add it to exclusion list)
01:59:05.94 +59:55:34.3 -- not an asteroid (will add it to exclusion list)
01:28:07.91 +58:50:39.6 -- not an asteroid (will add it to exclusion list)
02:34:19.54 +56:15:41.6 -- not an asteroid (will add it to exclusion list)
00:44:10.04 +64:27:25.8 -- not an asteroid (will add it to exclusion list)
02:32:09.39 +56:09:40.6 -- not an asteroid (will add it to exclusion list)
01:43:03.30 +58:57:12.9 -- not an asteroid (will add it to exclusion list)
02:02:53.90 +60:15:42.0 -- not an asteroid (will add it to exclusion list)
02:33:46.62 +55:56:04.6 -- not an asteroid (will add it to exclusion list)
02:35:02.29 +56:14:22.9 -- not an asteroid (will add it to exclusion list)
01:24:55.22 +57:12:20.0 -- not an asteroid (will add it to exclusion list)
01:34:42.46 +58:42:15.2 -- not an asteroid (will add it to exclusion list)
02:05:23.30 +59:19:31.5 -- not an asteroid (will add it to exclusion list)
02:32:58.07 +56:06:56.5 -- not an asteroid (will add it to exclusion list)
01:19:29.17 +59:25:20.5 -- not an asteroid (will add it to exclusion list)
01:36:50.88 +59:55:48.3 -- not an asteroid (will add it to exclusion list)
02:39:10.93 +63:43:59.5 -- not an asteroid (will add it to exclusion list)
02:20:14.56 +59:20:12.7 -- not an asteroid (will add it to exclusion list)
02:32:27.21 +55:53:12.4 -- not an asteroid (will add it to exclusion list)
00:50:58.17 +59:43:06.7 -- not an asteroid (will add it to exclusion list)
01:48:30.79 +58:02:54.6 -- not an asteroid (will add it to exclusion list)
02:33:09.09 +56:06:53.6 -- not an asteroid (will add it to exclusion list)
01:25:45.38 +59:01:19.8 -- not an asteroid (will add it to exclusion list)
00:59:00.02 +59:04:33.1 -- not an asteroid (will add it to exclusion list)
01:52:55.36 +59:33:30.6 -- not an asteroid (will add it to exclusion list)
01:08:11.66 +62:14:23.2 -- not an asteroid (will add it to exclusion list)
01:46:56.97 +57:21:54.8 -- not an asteroid (will add it to exclusion list)
02:02:32.20 +58:06:03.8 -- not an asteroid (will add it to exclusion list)
00:58:34.73 +57:44:23.1 -- not an asteroid (will add it to exclusion list)
01:36:37.08 +58:44:43.7 -- not an asteroid (will add it to exclusion list)
02:32:25.16 +56:00:34.4 -- not an asteroid (will add it to exclusion list)
01:31:55.84 +59:26:39.9 -- not an asteroid (will add it to exclusion list)
01:07:30.37 +60:38:18.7 -- not an asteroid (will add it to exclusion list)
02:28:46.53 +56:00:06.1 -- not an asteroid (will add it to exclusion list)
02:32:01.70 +57:03:30.6 -- not an asteroid (will add it to exclusion list)
02:26:40.29 +56:09:51.2 -- not an asteroid (will add it to exclusion list)
02:27:56.21 +56:10:22.8 -- not an asteroid (will add it to exclusion list)
01:29:32.61 +63:18:22.4 -- not an asteroid (will add it to exclusion list)
02:34:00.02 +55:56:27.7 -- not an asteroid (will add it to exclusion list)
02:29:11.65 +56:22:44.6 -- not an asteroid (will add it to exclusion list)
02:33:51.39 +55:58:25.7 -- not an asteroid (will add it to exclusion list)
02:33:52.85 +56:31:18.5 -- not an asteroid (will add it to exclusion list)
02:34:27.89 +57:30:42.7 -- not an asteroid (will add it to exclusion list)
02:34:13.39 +56:03:48.2 -- not an asteroid (will add it to exclusion list)
02:44:06.26 +62:20:01.3 -- not an asteroid (will add it to exclusion list)
02:34:05.94 +56:37:27.5 -- not an asteroid (will add it to exclusion list)
02:27:52.20 +56:32:26.7 -- not an asteroid (will add it to exclusion list)
02:29:03.07 +56:34:20.1 -- not an asteroid (will add it to exclusion list)
02:46:03.81 +63:32:43.3 -- not an asteroid (will add it to exclusion list)
02:49:57.09 +63:51:39.7 -- not an asteroid (will add it to exclusion list)
02:28:35.24 +56:03:02.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:33:46.94 +63:27:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:43.22 +64:22:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:46.02 +61:48:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:00.24 +63:08:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:16.23 +61:49:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:25.55 +62:13:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:25.93 +61:07:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:02.79 +63:36:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:14.50 +61:35:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:18.92 +60:08:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:10.04 +64:27:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:18.35 +64:55:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:21.47 +58:18:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:47.70 +66:11:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:45.53 +59:54:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:51.53 +58:59:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:55.69 +60:00:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:11.29 +58:29:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:11.40 +58:35:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:23.55 +61:04:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:18.55 +65:56:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:39.69 +61:23:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:57.44 +60:17:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:03.30 +57:23:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:30.95 +58:09:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:31.13 +64:31:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:57.59 +60:47:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:58.17 +59:43:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:03.58 +65:42:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:09.10 +60:42:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:14.86 +61:05:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:21.61 +57:15:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:25.61 +62:25:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:29.89 +65:11:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:32.85 +59:59:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:33.76 +58:43:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:40.01 +60:08:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:48.90 +64:02:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:55.23 +58:28:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:08.48 +64:49:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:20.61 +57:37:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:44.86 +60:23:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:53:53.44 +63:42:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:13.13 +64:20:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:29.86 +59:30:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:30.87 +59:24:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:18.16 +60:03:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:26.78 +60:51:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:44.64 +58:25:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:42.62 +58:03:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:45.56 +58:52:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:06.54 +58:58:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:00.34 +57:24:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:14.09 +60:18:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:15.67 +62:45:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:34.73 +57:44:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:00.02 +59:04:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:37.43 +59:16:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:59:54.65 +59:58:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:00:17.82 +60:23:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:00:37.27 +58:32:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:11.29 +65:10:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:14.73 +57:14:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:25.47 +57:50:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:40.03 +58:50:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:01:40.14 +64:15:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:05.20 +57:40:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:07.21 +61:19:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:12.18 +57:26:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:18.44 +60:28:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:45.68 +58:39:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:02.73 +58:09:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:04.31 +57:50:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:21.67 +58:04:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:22.70 +60:32:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:35.50 +60:28:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:55.36 +59:40:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:04:33.85 +57:23:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:57.35 +63:03:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:58.37 +57:11:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:13.02 +59:33:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:16.04 +57:53:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:37.45 +60:22:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:00.11 +61:28:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:30.37 +60:38:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:34.08 +60:52:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:39.08 +59:59:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:11.66 +62:14:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:08:39.16 +60:32:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:10.52 +58:09:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.48 +57:26:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:22.85 +58:34:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:01.79 +66:17:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:12.02 +59:17:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:16.06 +61:08:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:20.01 +61:17:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:41.02 +58:17:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:44.80 +61:13:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:50.78 +61:46:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:59.76 +57:33:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:01.33 +61:00:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:09.81 +64:30:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:38.95 +58:10:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:44.64 +57:24:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:54.30 +58:12:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:22.29 +57:12:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:45.30 +60:30:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:36.33 +63:27:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:44.77 +60:02:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:30.98 +57:14:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:41.01 +57:07:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:48.27 +57:17:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:14.18 +61:44:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:18:28.22 +58:11:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:24.09 +58:26:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:26.87 +57:22:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:29.17 +59:25:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:41.36 +62:51:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:47.65 +61:38:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:24.34 +59:10:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:20.04 +56:57:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:50.45 +58:12:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:55.22 +57:12:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:06.70 +59:33:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:15.49 +64:40:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:26.55 +60:57:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:38.40 +59:16:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:45.38 +59:01:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:52.13 +57:05:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:56.72 +59:35:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:01.91 +57:08:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:28.54 +59:41:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:12.82 +58:27:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:27:35.64 +57:56:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:07.91 +58:50:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:26.73 +60:23:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:32.61 +63:18:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:33.76 +57:55:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:45.03 +59:58:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:49.42 +58:16:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:58.56 +63:18:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:26.42 +58:11:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:30:34.21 +59:44:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:23.18 +59:33:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:55.84 +59:26:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:19.13 +59:45:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:32:21.95 +60:27:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:15.70 +56:57:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:34:42.46 +58:42:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:19.56 +58:24:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:23.69 +60:39:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:27.63 +60:33:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:32.85 +57:32:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:37.08 +58:44:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:50.88 +59:55:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:06.27 +58:10:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:07.73 +61:01:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:10.65 +60:44:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:33.84 +60:47:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:34.88 +57:01:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:53.21 +57:14:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:44.36 +58:39:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:03.30 +58:57:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:30.72 +57:38:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:30.83 +57:33:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:32.29 +58:45:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:52.14 +57:41:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:34.97 +59:18:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:13.78 +57:54:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:23.23 +61:12:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:34.07 +59:44:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.52 +60:07:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:56.97 +57:21:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:04.43 +59:18:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:13.15 +57:44:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:27.75 +64:31:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:01.86 +57:39:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:07.33 +59:50:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:30.79 +58:02:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:03.59 +61:04:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:54.28 +63:40:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:10.11 +57:10:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:40.43 +57:43:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:46.76 +58:00:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:50.32 +57:13:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:54.81 +57:35:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:09.01 +58:27:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:55.36 +59:33:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:10.31 +58:09:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:47.19 +60:15:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:04.65 +57:00:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:13.86 +57:26:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:29.18 +60:09:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:16.32 +59:38:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:40.24 +59:15:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:50.68 +56:57:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:55.84 +57:26:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:05.94 +59:55:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:33.38 +60:01:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:32.20 +58:06:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:02:53.90 +60:15:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:03:02.00 +56:50:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:04.10 +64:05:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:04:10.77 +57:54:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:05:23.30 +59:19:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:25.40 +57:54:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:07:35.01 +56:36:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:04.25 +58:11:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:08:50.87 +57:39:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:23.96 +60:01:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:10:55.92 +62:17:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:23.25 +61:21:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:52.89 +59:02:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:12:41.30 +62:42:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:17:30.25 +56:22:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:03.99 +56:20:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:59.76 +57:04:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:19:57.86 +59:32:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:20:14.56 +59:20:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:28.82 +63:55:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:21:32.56 +56:32:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:36.82 +56:49:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:24:32.99 +56:11:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:34.99 +57:05:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:40.29 +56:09:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:26:52.85 +57:11:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:52.20 +56:32:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:27:56.21 +56:10:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:35.24 +56:03:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:46.17 +56:02:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:46.53 +56:00:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:03.07 +56:34:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:11.65 +56:22:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:26.16 +55:58:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:29:49.57 +56:00:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:11.32 +66:01:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:39.08 +56:07:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:41.72 +55:56:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:44.35 +55:58:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:44.71 +56:03:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:45.63 +55:56:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:46.93 +55:56:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:30:56.83 +56:00:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:00.53 +56:00:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:03.24 +56:42:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:04.78 +56:05:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:19.12 +56:02:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:23.81 +55:56:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:26.25 +55:59:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:39.66 +56:01:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:42.28 +56:00:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:46.11 +55:57:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:49.82 +56:26:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:53.23 +55:53:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:31:58.20 +56:05:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:01.70 +57:03:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:01.75 +55:53:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:04.79 +56:03:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:04.89 +55:55:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:09.03 +55:55:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:09.39 +56:09:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:09.71 +57:05:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:14.58 +55:56:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:17.00 +55:59:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:25.16 +56:00:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:26.77 +56:07:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:27.21 +55:53:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:30.22 +55:59:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:31.89 +56:04:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:37.64 +56:00:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:38.56 +55:54:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:39.77 +55:52:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:53.75 +56:02:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:56.82 +56:04:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:58.07 +56:06:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:01.37 +56:09:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:02.37 +56:01:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:04.96 +56:00:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:05.57 +56:13:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:06.79 +56:00:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:07.17 +56:01:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:09.09 +56:06:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:11.33 +56:00:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:15.77 +55:52:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:17.19 +56:06:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:20.71 +55:51:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:21.52 +56:04:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:28.43 +56:01:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:31.71 +55:59:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:34.36 +55:49:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:34.64 +56:11:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:35.07 +55:54:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:36.90 +55:50:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:40.44 +56:00:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:43.06 +55:51:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:46.62 +55:56:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:49.28 +55:57:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:51.13 +55:59:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:51.39 +55:58:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:51.70 +56:01:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:52.04 +56:11:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:52.85 +56:31:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:57.45 +56:01:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:00.02 +55:56:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:02.55 +56:37:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:03.60 +56:00:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:05.94 +56:37:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:06.54 +56:16:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:06.92 +56:06:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:08.57 +55:49:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:09.98 +55:51:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:10.27 +56:06:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:11.08 +55:50:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:13.08 +56:11:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:13.31 +56:12:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:13.39 +56:03:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:14.08 +56:19:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:14.64 +56:14:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:19.23 +56:15:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:19.33 +56:07:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:19.54 +56:15:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:22.75 +56:20:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:24.39 +55:59:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:25.79 +56:10:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:27.89 +57:30:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:28.10 +56:04:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:28.15 +56:03:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:32.09 +56:11:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:34.68 +56:21:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:41.51 +56:11:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:44.54 +56:06:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:47.05 +56:16:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:47.29 +56:12:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:48.63 +56:07:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:50.95 +56:14:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:34:55.55 +56:12:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:02.29 +56:14:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:07.08 +56:20:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:13.46 +56:19:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:16.32 +56:26:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:29.23 +56:28:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:31.37 +57:11:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:37:49.70 +57:46:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:39:10.93 +63:43:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:44:06.26 +62:20:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:46:03.81 +63:32:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:46:16.46 +65:01:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:47:22.83 +63:30:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:49:57.09 +63:51:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:33:46.94 +63:27:56.6 -- not a known variable star
00:36:43.22 +64:22:48.1 -- not a known variable star
00:36:46.02 +61:48:23.6 -- a known variable star
00:37:00.24 +63:08:01.5 -- a known variable star
00:38:16.23 +61:49:05.9 -- not a known variable star
00:40:25.55 +62:13:05.2 -- a known variable star
00:40:25.93 +61:07:16.2 -- not a known variable star
00:41:02.79 +63:36:12.4 -- a known variable star
00:41:14.50 +61:35:32.2 -- a known variable star
00:41:18.92 +60:08:55.3 -- not a known variable star
00:44:10.04 +64:27:25.8 -- a known variable star
00:44:18.35 +64:55:16.2 -- not a known variable star
00:44:21.47 +58:18:53.3 -- not a known variable star
00:44:47.70 +66:11:33.2 -- not a known variable star
00:45:45.53 +59:54:30.7 -- not a known variable star
00:46:51.53 +58:59:59.8 -- not a known variable star
00:46:55.69 +60:00:23.1 -- not a known variable star
00:47:11.29 +58:29:06.0 -- not a known variable star
00:47:11.40 +58:35:25.7 -- a known variable star
00:47:23.55 +61:04:59.8 -- not a known variable star
00:49:18.55 +65:56:10.8 -- not a known variable star
00:49:39.69 +61:23:34.4 -- a known variable star
00:49:57.44 +60:17:56.5 -- not a known variable star
00:50:03.30 +57:23:20.9 -- not a known variable star
00:50:30.95 +58:09:49.1 -- not a known variable star
00:50:31.13 +64:31:47.5 -- not a known variable star
00:50:57.59 +60:47:11.6 -- not a known variable star
00:50:58.17 +59:43:06.7 -- a known variable star
00:51:03.58 +65:42:57.2 -- not a known variable star
00:51:09.10 +60:42:14.5 -- not a known variable star
00:51:14.86 +61:05:30.2 -- not a known variable star
00:51:21.61 +57:15:53.7 -- not a known variable star
00:51:25.61 +62:25:15.4 -- not a known variable star
00:51:29.89 +65:11:40.6 -- a known variable star
00:51:32.85 +59:59:13.6 -- not a known variable star
00:51:33.76 +58:43:24.3 -- not a known variable star
00:52:40.01 +60:08:46.7 -- not a known variable star
00:52:48.90 +64:02:29.2 -- not a known variable star
00:52:55.23 +58:28:51.8 -- not a known variable star
00:53:08.48 +64:49:01.1 -- not a known variable star
00:53:20.61 +57:37:02.3 -- a known variable star
00:53:44.86 +60:23:25.2 -- a known variable star
00:53:53.44 +63:42:25.3 -- not a known variable star
00:54:13.13 +64:20:25.0 -- a known variable star
00:54:29.86 +59:30:21.8 -- not a known variable star
00:54:30.87 +59:24:00.8 -- a known variable star
00:55:18.16 +60:03:32.6 -- not a known variable star
00:55:26.78 +60:51:04.8 -- not a known variable star
00:55:44.64 +58:25:59.4 -- a known variable star
00:56:42.62 +58:03:48.0 -- not a known variable star
00:56:45.56 +58:52:45.9 -- not a known variable star
00:57:06.54 +58:58:31.2 -- not a known variable star
00:58:00.34 +57:24:03.5 -- not a known variable star
00:58:14.09 +60:18:23.5 -- not a known variable star
00:58:15.67 +62:45:20.2 -- not a known variable star
00:58:34.73 +57:44:23.1 -- a known variable star
00:59:00.02 +59:04:33.1 -- not a known variable star
00:59:37.43 +59:16:40.0 -- not a known variable star
00:59:54.65 +59:58:35.3 -- a known variable star
01:00:17.82 +60:23:28.8 -- not a known variable star
01:00:37.27 +58:32:33.2 -- a known variable star
01:01:11.29 +65:10:55.4 -- not a known variable star
01:01:14.73 +57:14:39.1 -- a known variable star
01:01:25.47 +57:50:13.8 -- not a known variable star
01:01:40.03 +58:50:24.2 -- not a known variable star
01:01:40.14 +64:15:03.0 -- not a known variable star
01:02:05.20 +57:40:27.8 -- not a known variable star
01:02:07.21 +61:19:23.6 -- not a known variable star
01:02:12.18 +57:26:33.6 -- not a known variable star
01:02:18.44 +60:28:18.8 -- not a known variable star
01:02:45.68 +58:39:34.8 -- a known variable star
01:03:02.73 +58:09:40.5 -- a known variable star
01:03:04.31 +57:50:55.9 -- not a known variable star
01:03:21.67 +58:04:37.8 -- not a known variable star
01:03:22.70 +60:32:14.0 -- not a known variable star
01:03:35.50 +60:28:06.7 -- not a known variable star
01:03:55.36 +59:40:27.1 -- not a known variable star
01:04:33.85 +57:23:33.9 -- not a known variable star
01:05:57.35 +63:03:31.2 -- not a known variable star
01:05:58.37 +57:11:40.4 -- not a known variable star
01:06:13.02 +59:33:47.1 -- not a known variable star
01:06:16.04 +57:53:24.3 -- not a known variable star
01:06:37.45 +60:22:38.2 -- not a known variable star
01:07:00.11 +61:28:29.9 -- a known variable star
01:07:30.37 +60:38:18.7 -- not a known variable star
01:07:34.08 +60:52:43.7 -- not a known variable star
01:07:39.08 +59:59:18.1 -- not a known variable star
01:08:11.66 +62:14:23.2 -- a known variable star
01:08:39.16 +60:32:40.7 -- not a known variable star
01:09:10.52 +58:09:35.5 -- not a known variable star
01:09:22.48 +57:26:31.4 -- not a known variable star
01:09:22.85 +58:34:03.2 -- not a known variable star
01:10:01.79 +66:17:40.5 -- not a known variable star
01:10:12.02 +59:17:25.4 -- not a known variable star
01:11:16.06 +61:08:30.1 -- a known variable star
01:11:20.01 +61:17:54.4 -- not a known variable star
01:11:41.02 +58:17:27.9 -- not a known variable star
01:11:44.80 +61:13:57.3 -- a known variable star
01:11:50.78 +61:46:45.6 -- not a known variable star
01:12:59.76 +57:33:52.4 -- not a known variable star
01:13:01.33 +61:00:58.3 -- a known variable star
01:13:09.81 +64:30:33.5 -- not a known variable star
01:13:38.95 +58:10:50.4 -- not a known variable star
01:13:44.64 +57:24:50.1 -- not a known variable star
01:13:54.30 +58:12:33.7 -- not a known variable star
01:14:22.29 +57:12:42.3 -- not a known variable star
01:14:45.30 +60:30:04.8 -- not a known variable star
01:15:36.33 +63:27:54.0 -- a known variable star
01:15:44.77 +60:02:45.6 -- not a known variable star
01:16:30.98 +57:14:55.3 -- not a known variable star
01:17:41.01 +57:07:19.9 -- a known variable star
01:17:48.27 +57:17:35.5 -- not a known variable star
01:18:14.18 +61:44:36.2 -- not a known variable star
01:18:28.22 +58:11:22.5 -- not a known variable star
01:19:24.09 +58:26:40.3 -- not a known variable star
01:19:26.87 +57:22:51.4 -- not a known variable star
01:19:29.17 +59:25:20.5 -- not a known variable star
01:19:41.36 +62:51:05.1 -- not a known variable star
01:19:47.65 +61:38:29.2 -- not a known variable star
01:20:24.34 +59:10:25.1 -- not a known variable star
01:21:20.04 +56:57:25.3 -- not a known variable star
01:22:50.45 +58:12:42.0 -- a known variable star
01:24:55.22 +57:12:20.0 -- not a known variable star
01:25:06.70 +59:33:57.1 -- a known variable star
01:25:15.49 +64:40:35.1 -- not a known variable star
01:25:26.55 +60:57:45.1 -- not a known variable star
01:25:38.40 +59:16:00.1 -- not a known variable star
01:25:45.38 +59:01:19.8 -- not a known variable star
01:25:52.13 +57:05:24.0 -- a known variable star
01:25:56.72 +59:35:11.7 -- not a known variable star
01:26:01.91 +57:08:04.9 -- not a known variable star
01:26:28.54 +59:41:35.0 -- not a known variable star
01:27:12.82 +58:27:16.9 -- not a known variable star
01:27:35.64 +57:56:59.8 -- not a known variable star
01:28:07.91 +58:50:39.6 -- a known variable star
01:28:26.73 +60:23:26.9 -- not a known variable star
01:29:32.61 +63:18:22.4 -- a known variable star
01:29:33.76 +57:55:08.9 -- not a known variable star
01:29:45.03 +59:58:32.3 -- not a known variable star
01:29:49.42 +58:16:02.6 -- not a known variable star
01:29:58.56 +63:18:25.9 -- a known variable star
01:30:26.42 +58:11:55.8 -- not a known variable star
01:30:34.21 +59:44:32.0 -- not a known variable star
01:31:23.18 +59:33:44.1 -- not a known variable star
01:31:55.84 +59:26:39.9 -- not a known variable star
01:32:19.13 +59:45:28.6 -- a known variable star
01:32:21.95 +60:27:29.1 -- not a known variable star
01:33:15.70 +56:57:52.0 -- not a known variable star
01:34:42.46 +58:42:15.2 -- not a known variable star
01:35:19.56 +58:24:48.5 -- not a known variable star
01:35:23.69 +60:39:00.6 -- a known variable star
01:35:27.63 +60:33:46.7 -- not a known variable star
01:35:32.85 +57:32:34.4 -- a known variable star
01:36:37.08 +58:44:43.7 -- a known variable star
01:36:50.88 +59:55:48.3 -- a known variable star
01:38:06.27 +58:10:40.1 -- a known variable star
01:38:07.73 +61:01:40.6 -- not a known variable star
01:38:10.65 +60:44:57.1 -- not a known variable star
01:38:33.84 +60:47:24.6 -- not a known variable star
01:39:34.88 +57:01:21.5 -- not a known variable star
01:40:53.21 +57:14:54.4 -- not a known variable star
01:42:44.36 +58:39:03.4 -- not a known variable star
01:43:03.30 +58:57:12.9 -- not a known variable star
01:44:30.72 +57:38:51.1 -- not a known variable star
01:44:30.83 +57:33:34.1 -- not a known variable star
01:44:32.29 +58:45:36.3 -- not a known variable star
01:44:52.14 +57:41:43.0 -- a known variable star
01:45:34.97 +59:18:10.9 -- not a known variable star
01:46:13.78 +57:54:08.3 -- not a known variable star
01:46:23.23 +61:12:56.7 -- a known variable star
01:46:34.07 +59:44:09.6 -- not a known variable star
01:46:38.52 +60:07:33.4 -- not a known variable star
01:46:56.97 +57:21:54.8 -- not a known variable star
01:47:04.43 +59:18:55.3 -- not a known variable star
01:47:13.15 +57:44:19.2 -- a known variable star
01:47:27.75 +64:31:09.8 -- not a known variable star
01:48:01.86 +57:39:19.3 -- not a known variable star
01:48:07.33 +59:50:53.1 -- not a known variable star
01:48:30.79 +58:02:54.6 -- not a known variable star
01:49:03.59 +61:04:33.8 -- not a known variable star
01:49:54.28 +63:40:38.1 -- not a known variable star
01:50:10.11 +57:10:52.0 -- not a known variable star
01:50:40.43 +57:43:29.4 -- a known variable star
01:50:46.76 +58:00:38.2 -- not a known variable star
01:50:50.32 +57:13:03.4 -- not a known variable star
01:51:54.81 +57:35:15.7 -- not a known variable star
01:52:09.01 +58:27:40.6 -- not a known variable star
01:52:55.36 +59:33:30.6 -- a known variable star
01:53:10.31 +58:09:47.0 -- not a known variable star
01:53:47.19 +60:15:59.3 -- not a known variable star
01:54:04.65 +57:00:35.8 -- not a known variable star
01:57:13.86 +57:26:43.7 -- not a known variable star
01:57:29.18 +60:09:19.3 -- not a known variable star
01:58:16.32 +59:38:59.1 -- not a known variable star
01:58:40.24 +59:15:59.7 -- a known variable star
01:58:50.68 +56:57:17.7 -- not a known variable star
01:58:55.84 +57:26:42.4 -- not a known variable star
01:59:05.94 +59:55:34.3 -- not a known variable star
01:59:33.38 +60:01:45.4 -- a known variable star
02:02:32.20 +58:06:03.8 -- not a known variable star
02:02:53.90 +60:15:42.0 -- not a known variable star
02:03:02.00 +56:50:06.8 -- not a known variable star
02:04:04.10 +64:05:48.9 -- not a known variable star
02:04:10.77 +57:54:39.3 -- a known variable star
02:05:23.30 +59:19:31.5 -- a known variable star
02:07:25.40 +57:54:58.4 -- not a known variable star
02:07:35.01 +56:36:56.3 -- not a known variable star
02:08:04.25 +58:11:23.1 -- a known variable star
02:08:50.87 +57:39:27.2 -- a known variable star
02:10:23.96 +60:01:13.7 -- not a known variable star
02:10:55.92 +62:17:08.9 -- a known variable star
02:11:23.25 +61:21:06.1 -- a known variable star
02:11:52.89 +59:02:30.7 -- not a known variable star
02:12:41.30 +62:42:19.4 -- not a known variable star
02:17:30.25 +56:22:50.2 -- a known variable star
02:18:03.99 +56:20:30.9 -- a known variable star
02:18:59.76 +57:04:00.7 -- not a known variable star
02:19:57.86 +59:32:26.9 -- not a known variable star
02:20:14.56 +59:20:12.7 -- not a known variable star
02:21:28.82 +63:55:29.7 -- not a known variable star
02:21:32.56 +56:32:12.5 -- not a known variable star
02:22:36.82 +56:49:53.5 -- not a known variable star
02:24:32.99 +56:11:30.8 -- not a known variable star
02:25:34.99 +57:05:41.3 -- a known variable star
02:26:40.29 +56:09:51.2 -- not a known variable star
02:26:52.85 +57:11:10.4 -- not a known variable star
02:27:52.20 +56:32:26.7 -- not a known variable star
02:27:56.21 +56:10:22.8 -- not a known variable star
02:28:35.24 +56:03:02.7 -- not a known variable star
02:28:46.17 +56:02:23.7 -- not a known variable star
02:28:46.53 +56:00:06.1 -- not a known variable star
02:29:03.07 +56:34:20.1 -- not a known variable star
02:29:11.65 +56:22:44.6 -- not a known variable star
02:29:26.16 +55:58:53.6 -- a known variable star
02:29:49.57 +56:00:09.6 -- a known variable star
02:30:11.32 +66:01:46.4 -- not a known variable star
02:30:39.08 +56:07:12.9 -- not a known variable star
02:30:41.72 +55:56:24.9 -- a known variable star
02:30:44.35 +55:58:12.9 -- not a known variable star
02:30:44.71 +56:03:12.4 -- not a known variable star
02:30:45.63 +55:56:53.3 -- not a known variable star
02:30:46.93 +55:56:09.0 -- a known variable star
02:30:56.83 +56:00:04.8 -- not a known variable star
02:31:00.53 +56:00:30.9 -- not a known variable star
02:31:03.24 +56:42:27.2 -- not a known variable star
02:31:04.78 +56:05:05.6 -- a known variable star
02:31:19.12 +56:02:17.6 -- a known variable star
02:31:23.81 +55:56:10.2 -- not a known variable star
02:31:26.25 +55:59:07.8 -- a known variable star
02:31:39.66 +56:01:58.4 -- not a known variable star
02:31:42.28 +56:00:52.2 -- a known variable star
02:31:46.11 +55:57:58.2 -- not a known variable star
02:31:49.82 +56:26:31.7 -- not a known variable star
02:31:53.23 +55:53:50.7 -- not a known variable star
02:31:58.20 +56:05:41.8 -- not a known variable star
02:32:01.70 +57:03:30.6 -- not a known variable star
02:32:01.75 +55:53:20.4 -- not a known variable star
02:32:04.79 +56:03:54.2 -- not a known variable star
02:32:04.89 +55:55:17.2 -- not a known variable star
02:32:09.03 +55:55:39.6 -- not a known variable star
02:32:09.39 +56:09:40.6 -- a known variable star
02:32:09.71 +57:05:33.2 -- a known variable star
02:32:14.58 +55:56:24.6 -- a known variable star
02:32:17.00 +55:59:24.0 -- not a known variable star
02:32:25.16 +56:00:34.4 -- not a known variable star
02:32:26.77 +56:07:14.1 -- not a known variable star
02:32:27.21 +55:53:12.4 -- not a known variable star
02:32:30.22 +55:59:10.3 -- not a known variable star
02:32:31.89 +56:04:32.8 -- a known variable star
02:32:37.64 +56:00:40.9 -- not a known variable star
02:32:38.56 +55:54:40.8 -- not a known variable star
02:32:39.77 +55:52:01.6 -- not a known variable star
02:32:53.75 +56:02:28.7 -- a known variable star
02:32:56.82 +56:04:05.6 -- not a known variable star
02:32:58.07 +56:06:56.5 -- not a known variable star
02:33:01.37 +56:09:30.5 -- not a known variable star
02:33:02.37 +56:01:38.3 -- not a known variable star
02:33:04.96 +56:00:14.2 -- not a known variable star
02:33:05.57 +56:13:00.8 -- not a known variable star
02:33:06.79 +56:00:36.9 -- not a known variable star
02:33:07.17 +56:01:46.1 -- not a known variable star
02:33:09.09 +56:06:53.6 -- not a known variable star
02:33:11.33 +56:00:07.8 -- not a known variable star
02:33:15.77 +55:52:19.1 -- a known variable star
02:33:17.19 +56:06:00.2 -- not a known variable star
02:33:20.71 +55:51:56.8 -- not a known variable star
02:33:21.52 +56:04:02.2 -- a known variable star
02:33:28.43 +56:01:32.1 -- a known variable star
02:33:31.71 +55:59:51.2 -- not a known variable star
02:33:34.36 +55:49:28.4 -- not a known variable star
02:33:34.64 +56:11:51.0 -- a known variable star
02:33:35.07 +55:54:27.1 -- not a known variable star
02:33:36.90 +55:50:23.1 -- not a known variable star
02:33:40.44 +56:00:07.9 -- a known variable star
02:33:43.06 +55:51:19.0 -- not a known variable star
02:33:46.62 +55:56:04.6 -- not a known variable star
02:33:49.28 +55:57:07.5 -- not a known variable star
02:33:51.13 +55:59:56.4 -- not a known variable star
02:33:51.39 +55:58:25.7 -- not a known variable star
02:33:51.70 +56:01:15.0 -- not a known variable star
02:33:52.04 +56:11:00.6 -- not a known variable star
02:33:52.85 +56:31:18.5 -- not a known variable star
02:33:57.45 +56:01:33.1 -- not a known variable star
02:34:00.02 +55:56:27.7 -- a known variable star
02:34:02.55 +56:37:43.2 -- a known variable star
02:34:03.60 +56:00:36.3 -- not a known variable star
02:34:05.94 +56:37:27.5 -- a known variable star
02:34:06.54 +56:16:48.1 -- not a known variable star
02:34:06.92 +56:06:17.2 -- a known variable star
02:34:08.57 +55:49:36.3 -- not a known variable star
02:34:09.98 +55:51:55.6 -- not a known variable star
02:34:10.27 +56:06:39.8 -- a known variable star
02:34:11.08 +55:50:02.2 -- a known variable star
02:34:13.08 +56:11:55.4 -- not a known variable star
02:34:13.31 +56:12:38.9 -- a known variable star
02:34:13.39 +56:03:48.2 -- not a known variable star
02:34:14.08 +56:19:37.9 -- not a known variable star
02:34:14.64 +56:14:11.5 -- not a known variable star
02:34:19.23 +56:15:01.8 -- not a known variable star
02:34:19.33 +56:07:37.8 -- not a known variable star
02:34:19.54 +56:15:41.6 -- a known variable star
02:34:22.75 +56:20:28.3 -- not a known variable star
02:34:24.39 +55:59:28.1 -- not a known variable star
02:34:25.79 +56:10:43.4 -- a known variable star
02:34:27.89 +57:30:42.7 -- not a known variable star
02:34:28.10 +56:04:39.7 -- not a known variable star
02:34:28.15 +56:03:40.0 -- not a known variable star
02:34:32.09 +56:11:10.8 -- not a known variable star
02:34:34.68 +56:21:56.3 -- not a known variable star
02:34:41.51 +56:11:02.0 -- not a known variable star
02:34:44.54 +56:06:08.1 -- not a known variable star
02:34:47.05 +56:16:36.7 -- not a known variable star
02:34:47.29 +56:12:09.8 -- not a known variable star
02:34:48.63 +56:07:35.8 -- not a known variable star
02:34:50.95 +56:14:16.1 -- a known variable star
02:34:55.55 +56:12:20.3 -- not a known variable star
02:35:02.29 +56:14:22.9 -- not a known variable star
02:35:07.08 +56:20:15.3 -- not a known variable star
02:35:13.46 +56:19:56.7 -- not a known variable star
02:35:16.32 +56:26:20.6 -- not a known variable star
02:35:29.23 +56:28:22.8 -- a known variable star
02:36:31.37 +57:11:41.5 -- not a known variable star
02:37:49.70 +57:46:16.6 -- not a known variable star
02:39:10.93 +63:43:59.5 -- not a known variable star
02:44:06.26 +62:20:01.3 -- not a known variable star
02:46:03.81 +63:32:43.3 -- not a known variable star
02:46:16.46 +65:01:23.9 -- not a known variable star
02:47:22.83 +63:30:07.2 -- a known variable star
02:49:57.09 +63:51:39.7 -- not a known variable star
Found 263 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
349 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 349 (excluding asteroids and hot pixels, 263 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)2461169.91610925 -observatory V36
02:40:25.93 +14:49:07.3 Mercury (-1.6mag)
05:07:40.65 +24:08:46.5 Venus (-3.9mag)
01:24:12.45 +07:57:40.0 Mars (1.2mag)
07:25:53.23 +22:22:08.2 Jupiter (-2.0mag)
00:39:06.19 +01:49:35.8 Saturn (0.9mag)
03:53:00.49 +20:04:05.9 Uranus (5.8mag)
00:13:38.69 +00:02:02.8 Neptune (7.8mag)
20:34:14.50 -22:55:38.8 Pluto (14.5mag)
21:06:53.37 -19:22:57.0 Moon (-10.5mag)
-rw-r--r-- 1 apache apache 363 May 9 05:02 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461169.91610925:
07:26:00.59 +22:21:51.6 Io (5.9mag)
07:25:46.02 +22:22:24.4 Europa (6.0mag)
07:25:44.26 +22:22:24.6 Ganymede (5.5mag)
07:25:29.77 +22:22:58.3 Callisto (6.7mag)
07:27:59.34 +22:01:15.3 Himalia (15.5mag)
07:25:56.55 +22:22:01.0 Thebe (16.4mag)
07:28:27.61 +22:28:44.8 Elara (17.4mag)
07:26:19.53 +22:49:50.8 Pasiphae (17.6mag)
07:33:35.38 +22:21:56.9 Carme (18.7mag)
00:39:05.16 +01:49:22.8 Titan (8.7mag)
00:39:08.67 +01:49:31.8 Rhea (10.0mag)
00:38:50.12 +01:47:33.0 Iapetus (11.4mag)
00:39:06.76 +01:50:04.8 Hyperion (14.7mag)
00:40:21.87 +01:55:37.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 May 9 05:02 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461169.91610925:
16:53:16.05 -28:33:59.8 JWST
19:36:53.32 +04:40:23.4 Chandra
20:52:10.63 +39:16:02.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 9 05:02 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461169.91610925 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
07:27:36.57 +26:50:31.0 17.7mag P/2009 WX51 (Catalina)
18:55:43.06 -30:21:13.6 13.7mag P/2010 H2 (Vales)
05:25:33.00 -68:43:03.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:38:44.61 +31:37:49.7 17.4mag C/2017 K2 (PANSTARRS)
17:25:38.02 +13:06:35.4 17.7mag C/2021 G2 (ATLAS)
23:14:25.89 +30:16:01.6 17.1mag C/2022 E2 (ATLAS)
04:57:20.68 +26:35:29.0 16.2mag C/2022 N2 (PANSTARRS)
09:11:40.08 +31:52:21.3 16.4mag C/2022 QE78 (ATLAS)
08:37:07.12 +02:01:42.3 17.5mag C/2022 R6 (PANSTARRS)
18:45:20.62 +20:18:14.3 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:31:36.53 -11:11:33.8 17.5mag P/2023 B1 (PANSTARRS)
09:00:39.42 -08:32:21.5 17.9mag C/2023 F3 (ATLAS)
22:11:41.60 +64:27:27.9 17.6mag C/2023 H5 (Lemmon)
18:49:48.50 -04:28:02.3 13.9mag C/2023 R1 (PANSTARRS)
16:53:48.52 +88:16:41.7 17.9mag C/2023 X2 (Lemmon)
06:35:03.49 +63:36:39.9 17.4mag C/2024 A1 (ATLAS)
05:58:33.38 +24:01:41.7 12.4mag C/2024 E1 (Wierzchos)
16:01:51.87 +10:02:11.1 17.3mag C/2024 G6 (ATLAS)
20:23:29.23 +22:01:48.9 14.3mag C/2024 J3 (ATLAS)
03:48:24.02 -19:08:01.3 16.2mag C/2024 T5 (ATLAS)
05:37:49.56 +40:02:59.9 17.8mag C/2025 J1 (Borisov)
12:16:47.54 +52:59:05.4 16.2mag C/2025 L1 (ATLAS)
05:23:49.46 -06:57:35.9 10.0mag C/2025 R3 (PANSTARRS)
12:45:03.70 +04:10:47.2 17.3mag C/2025 Y1 (ATLAS)
05:20:32.00 +01:26:21.8 17.5mag C/2026 A1 (MAPS)
00:59:59.23 +40:40:22.7 15.3mag C/2026 B2 (Sun-Gao)
19:28:03.96 -08:30:23.9 10.4mag 10P/Tempel
14:30:57.45 +00:06:09.6 16.1mag 24P/Schaumasse
10:59:06.77 -00:58:18.1 15.8mag 29P/Schwassmann-Wachmann
10:42:12.07 -02:48:03.3 17.4mag 43P/Wolf-Harrington
02:25:11.67 +21:19:00.1 17.4mag 47P/Ashbrook-Jackson
07:57:00.85 +31:39:18.3 16.9mag 63P/Wild
23:57:10.09 -08:51:23.0 15.7mag 65P/Gunn
05:09:48.59 +28:12:15.8 16.2mag 76P/West-Kohoutek-Ikemura
01:58:35.76 +12:37:27.7 14.1mag 78P/Gehrels
00:09:10.18 -02:35:53.9 15.0mag 88P/Howell
03:19:54.33 +26:08:56.1 15.1mag 93P/Lovas
05:42:26.48 +33:11:57.4 15.9mag 123P/West-Hartley
09:00:53.36 +27:41:33.3 16.3mag 124P/Mrkos
03:10:17.06 +16:48:27.2 16.4mag 128P/Shoemaker-Holt
03:33:59.53 +17:00:36.8 17.6mag 131P/Mueller
03:32:33.58 +18:53:52.9 11.2mag 141P/Machholz
03:37:11.75 +12:47:38.2 11.2mag 141P-A/Machholz
02:17:16.46 +08:52:31.0 10.7mag 141P-D/Machholz
02:35:29.36 -29:36:01.3 17.8mag 161P/Hartley-IRAS
02:09:12.04 +10:15:12.4 14.9mag 162P/SidingSpring
17:13:16.31 -11:04:49.8 16.1mag 235P/LINEAR
06:26:42.05 +35:49:16.3 17.1mag 240P/NEAT
07:52:56.20 -03:02:51.8 17.9mag 242P/Spahr
23:15:46.50 -13:53:05.9 17.2mag 260P/McNaught
02:49:12.49 +26:10:46.7 17.8mag 295P/LINEAR
15:31:07.03 +08:09:07.7 17.4mag 391P/Kowalski
07:45:59.38 +21:16:55.3 17.8mag 450P/LONEOS
06:11:45.73 +43:38:54.5 17.7mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K May 9 05:02 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
21:35:33.81 -14:05:16.30 2026-05-6.29 14.51
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:35:33.81 -14:05:16.30 2026-05-6.29 14.51
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 2026-04-9.29 13.32
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
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
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
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
-rw-r--r-- 1 apache apache 5.8K May 9 05:02 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
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
-rw-r--r-- 1 apache apache 188K May 9 05:02 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:05:18.133 -10:24:28.89 AT 2026kzs 2026-04-07.27 19.663
19:10:27.552 +13:28:45.06 AT 2026kzr 2026-04-28.47 18.725
18:12:17.366 +00:39:40.36 AT 2026kzq 2026-04-15.45 19.645
18:26:11.280 +39:33:34.13 AT 2026kzp 2026-04-22.78 20.95
17:35:57.150 +46:21:21.92 AT 2026kzo 2026-04-09.81 21.73
16:01:38.350 +55:55:13.06 AT 2026kzn 2026-04-09.81 20.89
15:34:13.600 +52:13:29.48 AT 2026kzm 2026-04-09.80 21.57
19:12:37.740 +53:04:22.65 AT 2026kzl 2026-04-08.90 21.67
18:01:42.100 +21:32:35.13 AT 2026kzk 2026-04-03.90 20.91
16:00:29.470 +56:42:30.56 AT 2026kzj 2026-03-30.82 20.63
15:00:42.230 +43:44:51.39 AT 2026kzi 2026-03-23.79 22.16
14:06:25.970 +03:12:50.08 AT 2026kzh 2026-04-24.65 21.75
14:10:15.440 -01:10:59.11 AT 2026kzg 2026-04-24.65 21.84
13:47:04.130 +01:13:46.03 AT 2026kzf 2026-04-24.65 22.19
13:47:52.620 +02:27:07.29 AT 2026kze 2026-04-22.73 22.16
13:08:17.370 +04:32:05.97 AT 2026kzd 2026-04-22.71 22.33
14:08:10.510 +04:19:24.63 AT 2026kzc 2026-04-20.75 21.92
14:13:53.820 -01:39:30.67 AT 2026kzb 2026-04-12.73 22.21
11:27:55.560 -13:38:57.45 SN 2026kza 2026-04-23.30 19.353
22:41:38.669 +02:38:13.00 AT 2026kyz 2026-04-28.49 19.0985
-rw-r--r-- 1 apache apache 30K May 9 05:02 tns_transients_list.txt
